<subfield code="a">ALEPH experiment: Candidate of Higgs boson production</subfield>
</datafield>
<datafield tag="246" ind1="" ind2="1">
<subfield code="a">Expérience ALEPH: Candidat de la production d'un boson Higgs</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">14 06 2000</subfield>
</datafield>
<datafield tag="340" ind1="" ind2="">
<subfield code="a">FILM</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Candidate for the associated production of the Higgs boson and Z boson. Both, the Higgs and Z boson decay into 2 jets each. The green and the yellow jets belong to the Higgs boson. They represent the fragmentation of a bottom andanti-bottom quark. The red and the blue jets stem from the decay of the Z boson into a quark anti-quark pair. Left: View of the event along the beam axis. Bottom right: Zoom around the interaction point at the centre showing detailsof the fragmentation of the bottom and anti-bottom quarks. As expected for b quarks, in each jet the decay of a long-lived B meson is visible. Top right: "World map" showing the spatial distribution of the jets in the event.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">Press</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Experiments and Tracks</subfield>
<subfield code="a">The first CERN-built module of the barrel section of ATLAS's electromagnetic calorimeter</subfield>
</datafield>
<datafield tag="246" ind1="" ind2="1">
<subfield code="a">Premier module du tonneau du calorimètre electromagnétique d'ATLAS</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">10 Apr 2001</subfield>
</datafield>
<datafield tag="340" ind1="" ind2="">
<subfield code="a">DIGITAL</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Behind the module, left to right Ralf Huber, Andreas Bies and Jorgen Beck Hansen. In front of the module, left to right: Philippe Lançon and Edward Wood.</subfield>
</datafield>
<datafield tag="590" ind1="" ind2="">
<subfield code="a">Derrière le module, de gauche à droite: Ralf Huber, Andreas Bies, Jorgen Beck Hansen. Devant le module, de gauche à droite : Philippe Lançon et Edward Wood.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">CERN EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Experiments and Tracks</subfield>
<subfield code="a">In February, the Agreement establishing the European Molecular Biology Conference was signed at CERN. Willy Spuhler is signing for Switzerland.</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Personalities and History of CERN</subfield>
<subfield code="a">High energy cosmic rays striking atoms at the top of the atmosphere give the rise to showers of particles striking the Earth's surface</subfield>
</datafield>
<datafield tag="246" ind1="" ind2="1">
<subfield code="a">Des rayons cosmiques de haute energie heurtent des atomes dans la haute atmosphere et donnent ainsi naissance a des gerbes de particules projetees sur la surface terrestre</subfield>
<subfield code="s">eight Nobel prizewinners</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">1962</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">In 1962, CERN hosted the 11th International Conference on High Energy Physics. Among the distinguished visitors were eight Nobel prizewinners.Left to right: Cecil F. Powell, Isidor I. Rabi, Werner Heisenberg, Edwin M. McMillan, Emile Segre, Tsung Dao Lee, Chen Ning Yang and Robert Hofstadter.</subfield>
</datafield>
<datafield tag="590" ind1="" ind2="">
<subfield code="a">En 1962, le CERN est l'hote de la onzieme Conference Internationale de Physique des Hautes Energies. Parmi les visiteurs eminents se trouvaient huit laureats du prix Nobel.De gauche a droite: Cecil F. Powell, Isidor I. Rabi, Werner Heisenberg, Edwin M. McMillan, Emile Segre, Tsung Dao Lee, Chen Ning Yang et Robert Hofstadter.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">Press</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Personalities and History of CERN</subfield>
<subfield code="p">The Nobel Prize in Physics 1961 : Robert Hofstadter</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="P">
<subfield code="s">6002 (1962)</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">199830</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PICTURE</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">CERN-GE-9806033</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Tim Berners-Lee</subfield>
<subfield code="s">World-Wide Web inventor</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">28 Jun 1998</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Conference "Internet, Web, What's next?" on 26 June 1998 at CERN : Tim Berners-Lee, inventor of the World-Wide Web and Director of the W3C, explains how the Web came to be and give his views on the future.</subfield>
</datafield>
<datafield tag="590" ind1="" ind2="">
<subfield code="a">Conference "Internet, Web, What's next?" le 26 juin 1998 au CERN: Tim Berners-Lee, inventeur du World-Wide Web et directeur du W3C, explique comment le Web est ne, et donne ses opinions sur l'avenir.</subfield>
<subfield code="t">Le Pays Gessien : 3 Jul 1998</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="K">
<subfield code="b">0001037</subfield>
<subfield code="l">PRSPRS</subfield>
<subfield code="t">Le Temps : 27 Jun 1998</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="K">
<subfield code="b">0000809</subfield>
<subfield code="l">PRSPRS</subfield>
<subfield code="t">La Tribune de Geneve : 27 Jun 1998</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="P">
<subfield code="p">Bldg. 60</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="P">
<subfield code="r">Calder, N</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">199827</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PICTURE</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">astro-ph/9812226</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Efstathiou, G P</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Constraints on $\Omega_{\Lambda}$ and $\Omega_{m}$from Distant Type 1a Supernovae and Cosmic Microwave Background Anisotropies</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">14 Dec 1998</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">6 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We perform a combined likelihood analysis of the latest cosmic microwave background anisotropy data and distant Type 1a Supernova data of Perlmutter etal (1998a). Our analysis is restricted tocosmological models where structure forms from adiabatic initial fluctuations characterised by a power-law spectrum with negligible tensor component. Marginalizing over other parameters, our bestfit solution gives Omega_m = 0.25 (+0.18, -0.12) and Omega_Lambda = 0.63 (+0.17, -0.23) (95 % confidence errors) for the cosmic densities contributed by matter and a cosmological constantrespectively. The results therefore strongly favour a nearly spatially flat Universe with a non-zero cosmological constant.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Astrophysics and Astronomy</subfield>
<subfield code="p">Mon. Not. R. Astron. Soc.</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="O">
<subfield code="i">SLAC</subfield>
<subfield code="s">4162242</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="5">
<subfield code="b">CER</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200231</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond, J.R. 1996, Theory and Observations of the Cosmic Background Radiation, in "Cosmology and Large Scale Structure", Les Houches Session LX, August 1993, eds. R. Schaeffer, J. Silk, M. Spiro and J. Zinn-Justin, Elsevier SciencePress, Amsterdam, p469</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond J.R., Efstathiou G., Tegmark M., 1997</subfield>
<subfield code="p">L33</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">291</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond, J.R., Jaffe, A. 1997, in Proc. XXXI Rencontre de Moriond, ed. F. Bouchet, Edition Fronti eres, in press</subfield>
<subfield code="r">astro-ph/9610091</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Bond J.R., Jaffe A.H. and Knox L.E., 1998</subfield>
<subfield code="r">astro-ph/9808264</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Burles S., Tytler D., 1998a, to appear in the Proceedings of the Second Oak Ridge Symposium on Atomic & Nuclear Astrophysics, ed. A. Mezzacappa, Institute of Physics, Bristol</subfield>
<subfield code="r">astro-ph/9803071</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Burles S., Tytler D., 1998b, Astrophys. J.in press</subfield>
<subfield code="r">astro-ph/9712109</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Caldwell, R.R., Dave, R., Steinhardt P.J., 1998</subfield>
<subfield code="m">Devlin M.J., De Oliveira-Costa A., Herbig T., Miller A.D., Netterfield C.B., Page L., Tegmark M., 1998, submitted to Astrophys. J</subfield>
<subfield code="r">astro-ph/9808043</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Efstathiou G. 1996, Observations of Large-Scale Structure in the Universe, in "Cosmology and Large Scale Structure", Les Houches Session LX, August 1993, eds. R. Schaeffer, J. Silk, M. Spiro and J. Zinn-Justin, Elsevier SciencePress, Amsterdam, p135. Efstathiou G., Bond J.R., Mon. Not. R. Astron. Soc.in press</subfield>
<subfield code="r">astro-ph/9807130</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Evrard G., 1998, submitted to Mon. Not. R. Astron. Soc</subfield>
<subfield code="m">Peebles P.J.E., 1993, Principles of Physical Cosmology, Princeton University Press, Princeton, New Jersey. Perlmutter S, et al., 1995, In Presentations at the NATO ASI in Aiguablava, Spain, LBL-38400; also published in Thermonuclear Supernova, P. Ruiz-Lapuente, R. Cana and J. Isern (eds), Dordrecht, Kluwer, 1997, p749. Perlmutter S, et al., 1997</subfield>
<subfield code="p">565</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">483</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Perlmutter S. et al., 1998a, Astrophys. J.in press. (P98)</subfield>
<subfield code="r">astro-ph/9812133</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Perlmutter S. et al., 1998b, In Presentation at the January 1988 Meeting of the American Astronomical Society, Washington D.C., LBL-42230, available at www-supernova.lbl.gov; B.A.A.S., volume : 29 (1997) 1351Perlmutter S, et al., 1998c</subfield>
<subfield code="a">Search for R-Parity Violating Production of Single Sneutrinos in $e^{+}e^{-}$ Collisions at $\sqrt{s}$ = 189-209 GeV</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Geneva</subfield>
<subfield code="b">CERN</subfield>
<subfield code="c">17 Dec 2001</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">22 p</subfield>
</datafield>
<datafield tag="490" ind1="" ind2="">
<subfield code="a">ALEPH Papers</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">A search for single sneutrino production under the assumption that $R$-parity is violated via a single dominant $LL\bar{E}$ coupling is presented. This search considers the process ${\rm e} \gamma\;{\smash{\mathop{\rightarrow}}}\;\tilde{\nu}\ell$ and is performed using the data collected by the ALEPH detector at centre-of-mass energies from 189\,GeV up to 209\,GeV corresponding to an integrated luminosity of637.1\,$\mathrm{pb}^{-1}$. The numbers of observed candidate events are in agreement with Standard Model expectations and 95\% confidence level upper limits on five of the $LL\bar{E}$ couplings are given as a function of the assumedsneutrino mass.</subfield>
<subfield code="m">For reviews, see for example: H.P. Nilles</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">110</subfield>
<subfield code="y">1984</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H.E. Haber and G. L. Kane</subfield>
<subfield code="p">75</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">117</subfield>
<subfield code="y">1985</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Farrar and P. Fayet</subfield>
<subfield code="p">575</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">76</subfield>
<subfield code="y">1978</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Weinberg</subfield>
<subfield code="p">287</subfield>
<subfield code="t">Phys. Rev., B</subfield>
<subfield code="v">26</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Sakai and T. Yanagida</subfield>
<subfield code="p">83</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">197</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Dimopoulos, S. Raby and F. Wilczek</subfield>
<subfield code="p">133</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">212</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B.C. Allanach, H. Dreiner, P. Morawitz and M.D. Williams, "Single Sneutrino/Slepton Production at LEP2 and the NLC"</subfield>
<subfield code="p">307</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">420</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">ALEPH Collaboration, "Search for R-Parity Violating Decays of Supersymmetric Particles in e+e- Collisions at Centre-of-Mass Energies between s = 189202 GeV"</subfield>
<subfield code="p">415</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">19</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">ALEPH Collaboration, "ALEPH: a detector for electron-positron annihilations at LEP", Nucl. Instrum. and Methods. A : 294 (1990) 121</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Cantini, Yu. L. Dokshitzer, M. Olsson, G. Turnock and B.R. Webber, `New clustering algorithm for multijet cross sections in e+e- annihilation"</subfield>
<subfield code="p">432</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">269</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">ALEPH Collaboration, "Performance of the ALEPH detector at LEP", Nucl. Instrum. and Methods. A : 360 (1995) 481</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Katsanevas and P. Morawitz, "SUSYGEN 2.2 - A Monte Carlo Event Generator for MSSM Sparticle Production at e+e- Colliders"</subfield>
<subfield code="m">J.A.M. Vermaseren, in Proceedings of the IVth International Workshop on Gamma Gamma Interactions, Eds. G. Cochard and P. Kessler, Springer Verlag, 1980</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. -F. Grivaz and F. Le Diberder, "Complementary analyses and acceptance optimization in new particle searches", LAL preprint # 92-37 (1992)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">ALEPH Collaboration, "Search for Supersymmetry with a dominant R-Parity Violating LL ¯ E Coupling in e+e- Collisions at Centre-of-Mass Energies of 130 GeV to 172 GeV"</subfield>
<subfield code="p">433</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">4</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">For reviews see for example: H. Dreiner, "An Introduction to Explicit R-parity Violation"</subfield>
<subfield code="r">hep-ph/9707435</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">published in Perspectives on Supersymmetry, ed. G.L. Kane, World Scientific, Singapore (1998); G. Bhattacharyya</subfield>
<subfield code="p">83</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">52</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">12</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">astro-ph/0101431</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Gray, M E</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Infrared constraints on the dark mass concentration observed in the cluster Abell 1942</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">24 Jan 2001</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">8 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We present a deep H-band image of the region in the vicinity of the cluster Abell 1942 containing the puzzling dark matter concentration detected in an optical weak lensing study by Erben et al. (2000). We demonstrate that ourlimiting magnitude, H=22, would be sufficient to detect clusters of appropriate mass out to redshifts comparable with the mean redshift of the background sources. Despite this, our infrared image reveals no obvious overdensity ofsources at the location of the lensing mass peak, nor an excess of sources in the I-H vs. H colour-magnitude diagram. We use this to further constrain the luminosity and mass-to-light ratio of the putative dark clump as a function ofits redshift. We find that for spatially-flat cosmologies, background lensing clusters with reasonable mass-to-light ratios lying in the redshift range 0<z<1 are strongly excluded, leaving open the possibility that the massconcentration is a new type of truly dark object.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Astrophysics and Astronomy</subfield>
<subfield code="y">Mahon, Richard G. Mc</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="y">Firth, Andrew E.</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="4">
<subfield code="p">Mon. Not. R. Astron. Soc.</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200104</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0105155</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="088" ind1="" ind2="">
<subfield code="a">CERN-TH-2001-131</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Mangano, M L</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Physics at the front-end of a neutrino factory : a quantitative appraisal</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Geneva</subfield>
<subfield code="b">CERN</subfield>
<subfield code="c">16 May 2001</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">1 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We present a quantitative appraisal of the physics potential for neutrino experiments at the front-end of a muon storage ring. We estimate the forseeable accuracy in the determination of several interesting observables, and explorethe consequences of these measurements. We discuss the extraction of individual quark and antiquark densities from polarized and unpolarized deep-inelastic scattering. In particular we study the implications for the undertanding ofthe nucleon spin structure. We assess the determination of alpha_s from scaling violation of structure functions, and from sum rules, and the determination of sin^2(theta_W) from elastic nu-e and deep-inelastic nu-p scattering. Wethen consider the production of charmed hadrons, and the measurement of their absolute branching ratios. We study the polarization of Lambda baryons produced in the current and target fragmentation regions. Finally, we discuss thesensitivity to physics beyond the Standard Model.</subfield>
<subfield code="u">nuDIS Working group of the ECFA-CERN Neutrino-Factory Study Group</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">2001-05-17</subfield>
<subfield code="l">50</subfield>
<subfield code="m">2001-05-25</subfield>
<subfield code="o">MH</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="O">
<subfield code="i">SLAC</subfield>
<subfield code="s">4628020</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="5">
<subfield code="b">CER</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200231</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[1]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Geer</subfield>
<subfield code="p">6989</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">57</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9712290</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[Erratum</subfield>
<subfield code="p">039903</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">59</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">The Muon Collider Collab., µ+µ- Collider: a feasibility study, Report BNL-52503, Fermilab-Conf-96/092, LBNL-38946 (1996); B. Autin, A. Blondel and J. Ellis (eds.), Prospective study of muon storage rings at CERN, Report CERN 99-02, ECFA 99-197 (Geneva, 1999)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. Bigi et al., The potential for neutrino physics at muon colliders and dedicated high current muon storage rings, Report BNL-67404</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Albright et al</subfield>
<subfield code="r">hep-ex/0008064</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R.D. Ball, D.A. Harris and K.S. McFarland</subfield>
<subfield code="r">hep-ph/0009223</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">submitted to the Proceedings of the Nufact '00 Workshop, June 2000, Monterey</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H.L. Lai et al</subfield>
<subfield code="p">1280</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">55</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9606399</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Barone, C. Pascaud and F. Zomer</subfield>
<subfield code="p">243</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">12</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9907512</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. I. Alekhin</subfield>
<subfield code="p">094022</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">63</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0011002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">65</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Ridolfi</subfield>
<subfield code="p">278</subfield>
<subfield code="t">Nucl. Phys., A</subfield>
<subfield code="v">666</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R.D. Ball and H.A.M. Tallini</subfield>
<subfield code="p">1327</subfield>
<subfield code="t">J. Phys., G</subfield>
<subfield code="v">25</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Forte</subfield>
<subfield code="r">hep-ph/9409416</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="r">hep-ph/9610238</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Forte, M.L. Mangano and G. Ridolfi</subfield>
<subfield code="r">hep-ph/0101192</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">to appear in Nucl. Phys., B</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Blümlein and N. Kochelev</subfield>
<subfield code="p">296</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">381</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">285</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">498</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D.A. Dicus</subfield>
<subfield code="p">1637</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">5</subfield>
<subfield code="y">1972</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Anselmino, P. Gambino and J. Kalinowski</subfield>
<subfield code="p">267</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">64</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Maul et al</subfield>
<subfield code="p">443</subfield>
<subfield code="t">Z. Phys., A</subfield>
<subfield code="v">356</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Blümlein and N. Kochelev</subfield>
<subfield code="p">285</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">498</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Ravishankar</subfield>
<subfield code="p">309</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">374</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Ehrnsperger and A. Schäfer</subfield>
<subfield code="p">619</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">348</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Lichtenstadt and H.J. Lipkin</subfield>
<subfield code="p">119</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">353</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Dai et al</subfield>
<subfield code="p">273</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">53</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P.G. Ratcliffe</subfield>
<subfield code="p">383</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">365</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N.W. Park, J. Schechter and H. Weigel</subfield>
<subfield code="p">420</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">228</subfield>
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.O. Bazarko et al</subfield>
<subfield code="p">189</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">65</subfield>
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Mertig and W.L. van Neerven</subfield>
<subfield code="p">637</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">70</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Vogelsang</subfield>
<subfield code="p">2023</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">54</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. de Florian and R. Sassot</subfield>
<subfield code="p">6052</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">51</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R.D. Ball, S. Forte and G. Ridolfi</subfield>
<subfield code="p">255</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">378</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli, S. Forte and G. Ridolfi</subfield>
<subfield code="p">277</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">534</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">138</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">74</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli, R.D. Ball, S. Forte and G. Ridolfi</subfield>
<subfield code="p">1145</subfield>
<subfield code="t">Acta Phys. Pol., B</subfield>
<subfield code="v">29</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9803237</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H.L. Lai et al. (CTEQ Collab.)</subfield>
<subfield code="p">375</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">12</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9903282</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli, R.D. Ball, S. Forte and G. Ridolfi</subfield>
<subfield code="p">337</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">496</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">1145</subfield>
<subfield code="t">Acta Phys. Pol., B</subfield>
<subfield code="v">29</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli and G.G. Ross</subfield>
<subfield code="p">391</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">212</subfield>
<subfield code="y">1988</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. V. Efremov and O. V. Teryaev, JINR-E2-88-287, in Proceedings of Symposium on Hadron Interactions-Theory and Phenomenology, Bechyne, June 26- July 1, 1988; ed. by J. Fischer et al (Czech. Acad. ScienceInst. Phys., 1988) p.432; R.D. Carlitz, J.C. Collins and A.H. Mueller</subfield>
<subfield code="p">229</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">214</subfield>
<subfield code="y">1988</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli and B. Lampe</subfield>
<subfield code="p">315</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">47</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Vogelsang</subfield>
<subfield code="p">275</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">50</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[24]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G.M. Shore and G. Veneziano</subfield>
<subfield code="p">75</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">244</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">23</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">381</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">see also G. M. Shore</subfield>
<subfield code="r">hep-ph/9812355</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[25]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Forte</subfield>
<subfield code="p">189</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">224</subfield>
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">331</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Forte and E.V. Shuryak</subfield>
<subfield code="p">153</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">357</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[26]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.J. Brodsky and B.-Q. Ma</subfield>
<subfield code="p">317</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">381</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">66</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[27]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.J. Brodsky, J. Ellis and M. Karliner</subfield>
<subfield code="p">309</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">206</subfield>
<subfield code="y">1988</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Ellis and M. Karliner</subfield>
<subfield code="r">hep-ph/9601280</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Glück et al</subfield>
<subfield code="r">hep-ph/0011215</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Adams et al. (Spin Muon Collab.)</subfield>
<subfield code="m">C. Adloff et al. (H1 Collab.)</subfield>
<subfield code="r">hep-ex/0012052</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[63]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.D. Martin, R.G. Roberts, W.J. Stirling and R.S. Thorne</subfield>
<subfield code="p">117</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">18</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0007099</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[64]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E.B. Zijlstra and W.L. van Neerven</subfield>
<subfield code="p">525</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">383</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[65]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.G. Gorishny and S.A. Larin</subfield>
<subfield code="p">109</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">172</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.A. Larin and J.A.M. Vermaseren</subfield>
<subfield code="p">345</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">259</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[66]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.L. Kataev and A.V. Sidorov, preprint CERN-TH/7235-94</subfield>
<subfield code="r">hep-ph/9405254</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">in Proceedings of Rencontre de Moriond - Hadronic session of `QCD and high energy hadronic interactions', M´eribel-les-Allues, 1994, ed. J. Tr an Thanh V an (Editions Fronti eres, Gif-sur-Yvette, 1995), p. 189</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[67]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J.H. Kim et al</subfield>
<subfield code="p">3595</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">81</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ex/9808015</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[68]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Chyla and A.L. Kataev</subfield>
<subfield code="p">385</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">297</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9209213</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[69]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.L. Kataev and A.V. Sidorov</subfield>
<subfield code="p">179</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">331</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9402342</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[70]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Blümlein and W. L. van Neerven</subfield>
<subfield code="p">417</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">450</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9811351</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[71]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.L. Kataev and V.V. Starshenko</subfield>
<subfield code="p">235</subfield>
<subfield code="t">Mod. Phys. Lett., A</subfield>
<subfield code="v">10</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9502348</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.A. Samuel, J. Ellis and M. Karliner</subfield>
<subfield code="p">4380</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">74</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9503411</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[72]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Bernreuther and W. Wetzel</subfield>
<subfield code="p">228</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">197</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[Erratum</subfield>
<subfield code="p">758</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">513</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">]; S.A. Larin, T. van Ritbergen and J.A. Vermaseren</subfield>
<subfield code="p">278</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">438</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9411260</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K.G. Chetyrkin, B.A. Kniehl and M. Steinhauser</subfield>
<subfield code="p">2184</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">79</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9706430</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[73]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E.V. Shuryak and A.I. Vainshtein</subfield>
<subfield code="p">451</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">199</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[74]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.A. Shifman, A.I. Vainshtein and V.I. Zakharov</subfield>
<subfield code="p">385</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">147</subfield>
<subfield code="y">1979</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[75]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V.M. Braun and A.V. Kolesnichenko</subfield>
<subfield code="p">723</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">283</subfield>
<subfield code="y">1987</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">68</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[76]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G.G. Ross and R.G. Roberts</subfield>
<subfield code="p">425</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">322</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9312237</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[77]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Balla, M.V. Polyakov and C. Weiss</subfield>
<subfield code="a">Cosmic equation of state, Gravitational Lensing Statistics and Merging of Galaxies</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">4 Apr 2001</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">28 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">In this paper we investigate observational constraints on the cosmic equation of state of dark energy ($p = w \rho$) using gravitational lensing statistics. We carry out likelihood analysis of the lens surveys to constrain thecosmological parameters $\Omega_{m}$ and $w$. We start by constraining $\Omega_{m}$ and $w$ in the no-evolution model of galaxies where the comoving number density of galaxies is constant. We extend our study to evolutionary modelsof galaxies - Volmerange $&$ Guiderdoni Model and Fast-Merging Model (of Broadhurst, Ellis $&$ Glazebrook). For the no-evolution model we get $w \leq -0.24$ and $\Omega_{m}\leq 0.48$ at $1\sigma$ (68% confidence level). For theVolmerange $&$ Guiderdoni Model we have $w \leq -0.2$ and $\Omega_{m} \leq 0.58$ at $1 \sigma$, and for the Fast Merging Model we get $w \leq -0.02$ and $\Omega_{m} \leq 0.93$ at $1\sigma$. For the case of constant $\Lambda$ ($w=-1$), all the models permit $\Omega_{m} = 0.3$ with 68% CL. We observe that the constraints on $w$ and $\Omega_{m}$ (and on $\Omega_{m}$ in the case of $w = -1$) obtained in the case of evolutionary models are weaker than thoseobtained in the case of the no-evolution model.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Astrophysics and Astronomy</subfield>
<subfield code="m">P. de Bernardis et al</subfield>
<subfield code="p">955</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">404</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. J. Ostriker & P. J. Steinhardt</subfield>
<subfield code="p">600</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">377</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Sahni & Alexei Starobinsky, IJMP, D : 9 (2000) 373</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. F. Bloomfield Torres & I. Waga</subfield>
<subfield code="p">712</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">279</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Silveira & I. Waga</subfield>
<subfield code="p">4890</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">50</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V.Silveira & I. Waga</subfield>
<subfield code="p">4625</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. Waga & Ana P. M. R. Miceli, Phy. Rev. D : 59 (1999) 103507</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. S. Turner & M. White, Phy. Rev. D : 56 (1997) 4439</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Huterer & M. S. Turner, Phy. Rev. D : 60 (1999) 081301</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Chiba, N. Sugiyama & T. Nakamura, Mon. Not. R. As-tron. Soc.: 289 (1997) L5</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Chiba, N. Sugiyama & T. Nakamura, Mon. Not. R. As-tron. Soc.: 301 (1998) 72</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. J. E. Peebles</subfield>
<subfield code="p">439</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">284</subfield>
<subfield code="y">1984</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Ratra & P. J. E. Peebles, Phy. Rev. D : 37 (1988) 3406</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. R. Caldwell, R. Dave & P. J. Steinhardt, Phy. Rev. Lett.: 80 (1998) 1582</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Efstathiou</subfield>
<subfield code="r">astro-ph/9904356</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(1999)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. A. S. Lima & J. S. Alcaniz</subfield>
<subfield code="p">893</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">317</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Wang et al</subfield>
<subfield code="p">17</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">530</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. W. Rix, D. Maoz, E. Turner & M. Fukugita</subfield>
<subfield code="p">49</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">435</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Mao & C. S. Kochanek</subfield>
<subfield code="p">569</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">268</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Jain, N. Panchapakesan, S. Mahajan & V. B. Bhatia, MPLA : 15 (2000) 41</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[24]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Broadhurst, R. Ellis & K. Glazebrook</subfield>
<subfield code="p">55</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">355</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[BEG]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[25]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Rocca-Volmerange & B. Guiderdoni, Mon. Not. R. As-tron. Soc.: 247 (1990) 166</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[26]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Toomre, in The Evolution of Galaxies and Stellar Pop-ulations eds: B. M. Tinsley & R. B. Larson ( Yale Univ. Observatory), p-401 (1977)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[27]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. Schwezier</subfield>
<subfield code="p">109</subfield>
<subfield code="t">Astron. J.</subfield>
<subfield code="v">111</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">O. J. Eggen, D. Lynden-Bell & A. R. Sandage</subfield>
<subfield code="p">748</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">136</subfield>
<subfield code="y">1962</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. B. Partridge & P. J. E. Peebles</subfield>
<subfield code="p">868</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">147</subfield>
<subfield code="y">1967</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. P. Driver et al</subfield>
<subfield code="p">L23</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">449</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[31]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. M. Burkey et al</subfield>
<subfield code="p">L13</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">429</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[32]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. M. Faber et al</subfield>
<subfield code="p">668</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">204</subfield>
<subfield code="y">1976</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[33]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. G. Carlberg et al</subfield>
<subfield code="p">540</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">435</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[34]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. E. Zepf</subfield>
<subfield code="p">377</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">390</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[35]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Glazebrook et al</subfield>
<subfield code="p">157</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">273</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[36]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. J. Lilly et al</subfield>
<subfield code="p">108</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">455</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[37]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. S. Ellis et al</subfield>
<subfield code="p">235</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">280</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[38]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. S. Ellis, Ann. Rev</subfield>
<subfield code="p">389</subfield>
<subfield code="t">Astron. Astrophys.</subfield>
<subfield code="v">35</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[39]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Guiderdoni & B. Rocca-Volmerange</subfield>
<subfield code="p">435</subfield>
<subfield code="t">Astron. Astrophys.</subfield>
<subfield code="v">252</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[40]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. E. Zepf, & D. C. Koo</subfield>
<subfield code="p">34</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">337</subfield>
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[41]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. K. C. Yee & E. Ellingson</subfield>
<subfield code="p">37</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">445</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[42]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Cole et al</subfield>
<subfield code="p">781</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">271</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[43]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. M. Baugh, S. Cole & C. S. Frenk</subfield>
<subfield code="p">L27</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">282</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[44]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. M. Baugh, S. Cole & C. S. Frenk</subfield>
<subfield code="p">1361</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">283</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[45]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. M. Baugh et al</subfield>
<subfield code="p">504</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">498</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[46]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Schechter</subfield>
<subfield code="p">297</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">203</subfield>
<subfield code="y">1976</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[47]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. H. Press & P. Schechter</subfield>
<subfield code="p">487</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">187</subfield>
<subfield code="y">1974</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[48]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. E. Gunn & J. R. Gott</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">176</subfield>
<subfield code="y">1972</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[49]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Loveday, B. A. Peterson, G. Efstathiou & S. J. Maddox</subfield>
<subfield code="p">338</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">390</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[50]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. L. Turner, J. P. ostriker & J. R. Gott III</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">284</subfield>
<subfield code="y">1984</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[51]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. L. Turner</subfield>
<subfield code="p">L43</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">365</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[52]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Fukugita & E. L. Turner</subfield>
<subfield code="p">99</subfield>
<subfield code="t">Mon. Not. R. Astron. Soc.</subfield>
<subfield code="v">253</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[53]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Fukugita, T. Futamase, M. Kasai & E. L. Turner, As-trophys. J.: 393 (1992) 3</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[54]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. S. Kochanek</subfield>
<subfield code="p">12</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">419</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[55]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. S. Kochanek</subfield>
<subfield code="p">638</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">466</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[56]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. D. A. Hartwich & D. Schade, Ann. Rev. Astron. Astro-phys.: 28 (1990) 437</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[57]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Yu-Chung N. Cheng & L. M. Krauss</subfield>
<subfield code="p">697</subfield>
<subfield code="t">Int. J. Mod. Phys., A</subfield>
<subfield code="v">15</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[58]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. N. Bahcall et al</subfield>
<subfield code="p">56</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">387</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[59]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. C. Hewett et al., Astron. J.109, 1498(LBQS) (1995)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[60]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Maoz et al., Astrophys. J.409, 28(Snapshot) (1993)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[61]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Crampton, R. D. McClure & J. M. Fletcher</subfield>
<subfield code="p">23</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">392</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[62]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. K. C. Yee, A. V. Filippenko & D. Tang</subfield>
<subfield code="p">7</subfield>
<subfield code="t">Astron. J.</subfield>
<subfield code="v">105</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[63]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Surdej et al</subfield>
<subfield code="p">2064</subfield>
<subfield code="t">Astron. J.</subfield>
<subfield code="v">105</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[64]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Jain, N. Panchapakesan, S. Mahajan & V. B. Bhatia</subfield>
<subfield code="r">astro-ph/9807129</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(1998)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[65]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Jain, N. Panchapakesan, S. Mahajan & V. B. Bhatia, IJMP, A : 13 (1998) 4227</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[66]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. lampton, B. Margon & S. Bowyer</subfield>
<subfield code="p">177</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">208</subfield>
<subfield code="y">1976</subfield>
</datafield>
</record>
<record>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="088" ind1="" ind2="">
<subfield code="a">DOE-ER-40048-24-P-4</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Abbott, R B</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Cosmological perturbations in Kaluza-Klein models</subfield>
<subfield code="g">AACHEN - BIRMINGHAM - CERN - HELSINKI - KIEL - IMP. COLL. LONDON - QUEEN MARY COLL. LONDON - MADRID CIEMAT - MIT - RUTHERFORD APPLETON LAB. - VIENNA Collaboration</subfield>
<subfield code="a">Not held by the library</subfield>
</datafield>
<datafield tag="502" ind1="" ind2="">
<subfield code="a">Ph.D. : Univ. Central Florida : 1999</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Recent advances in multimedia processing technologies, internetworking technologies, and the World Wide Web phenomenon have resulted in a vast creation and use of digital videos in all kinds of applications ranging fromentertainment, business solutions, to education. Designing efficient techniques for searching and retrieving videos over the networks becomes increasingly more important as future applications will include a huge volume of multimediacontent. One practical approach to search for a video segment is as follows. Step 1: Apply an initial search to determine the set of candidate videos. Step 2: Browse the candidates to identify the relevant videos. Step 3: Searchwithin the relevant videos for interesting video segments. In practice, a user might have to iterate through these steps multiple times in order to locate the desired video segments. Independently, database researchers have beeninvestigating techniques for the initial search in Step 1. Multimedia researchers have proposed several techniques for video browsing in Step 2. Computer communications researchers have been investigating video delivery techniques. Iidentify that searching for video data is an interactive process which involves the transmission of video data. Developing techniques for each step independently could result in a system with less performance. In this dissertation, Ipresent a unified approach taking into accounts all fundamental characteristics of multimedia data. I evaluated the proposed techniques through both simulation and system implementation. The resulting system is less expensive andoffers better performance. The simulation results demonstrate that the proposed technique can offer video browsing and search operations with little delays and with minimum storage overhead at the server. Client machines can handletheir search operations without involving the server making the design more scalable, which is vital for large systems deployed over the Internet. The implemented system shows that the visual quality of the browsing and the searchoperations are excellent.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">PROQUEST200009</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Computing and Computers</subfield>
<subfield code="a">Neural Networks For Speech Recognition Of A Phonetic Language</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Long Beach, CA</subfield>
<subfield code="b">Calif. State Univ.</subfield>
<subfield code="c">1999</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">55 p</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">No fulltext</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">Not held by the library</subfield>
</datafield>
<datafield tag="502" ind1="" ind2="">
<subfield code="a">Ms : California State Univ. : 1999</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">The goal of this thesis is to explore a possibility for a viable alternative/replacement to the Amharic typewriter. Amharic is the national language of Ethiopia. It is one of the oldest languages in the world. Actually, the root-language of Amharic, called Geez, is a descendent of Sabean, which is the direct ancestor of all Semitic languages including English. A phonetic language with 276 phonemes/characters, Amharic has posed quite a challenge to those who,like the author of this thesis, have attempted to design an easy-to-use word processor that interfaces with the conventional keyboard. With current Amharic word processing software, each character requires an average of threekeystrokes thus making typing Amharic literature quite a task. This thesis researches the feasibility of developing a PC-based speech recognition system to recognize the spoken phonemes of the Amharic language. Artificial NeuralNetworks are used for the recognition of spoken alphabets that form Amharic words. A neural network with feed-forward architecture is trained with a series of alphabets and is evaluated on its ability to recognize subsequent testdata. The neural network used in this project is a static classification network; that is, it focuses on the frequency domain of speech while making no attempt to process temporal information. The network training procedure uses thegeneralized Delta Rule. The recognition system developed in this project is an Isolated Speech Recognition System. The approach taken is to recognize the spoken word character by character. This approach is expected to work well dueto the phonetic nature of Amharic.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">PROQUEST200009</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Computing and Computers</subfield>
</datafield>
<datafield tag="690" ind1="C" ind2="">
<subfield code="a">THESIS</subfield>
</datafield>
<datafield tag="690" ind1="C" ind2="">
<subfield code="a">notheld</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="b">14</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">2000-09-22</subfield>
<subfield code="l">00</subfield>
<subfield code="m">2002-02-22</subfield>
<subfield code="o">BATCH</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="O">
<subfield code="i">PROQUEST</subfield>
<subfield code="s">1397120</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="O">
<subfield code="i">PROQUEST</subfield>
<subfield code="s">MAI38/02p448Apr2000</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200034</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">THESIS</subfield>
</datafield>
</record>
<record>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Topcuoglu, H R</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Scheduling Task Graphs In Heterogeneous Computing Environments</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Syracuse, NY</subfield>
<subfield code="b">Syracuse Univ.</subfield>
<subfield code="c">1999</subfield>
</datafield>
<datafield tag="270" ind1="" ind2="">
<subfield code="g">dir.</subfield>
<subfield code="p">Hariri, S</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">126 p</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">No fulltext</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">Not held by the library</subfield>
<subfield code="a">Efficient application scheduling is critical for achieving high performance in heterogeneous computing environments. An application is represented by a directed acyclic graph (DAG) whose nodes represent tasks and whose edgesrepresent communication messages and precedence constraints among the tasks. The general task-scheduling problem maps the tasks of an application on processors and orders their execution so that task precedence requirements aresatisfied and a minimum schedule length is obtained. The task-scheduling problem has been shown to be NP- complete in general cases as well as in several restricted cases. Although a large number of scheduling heuristics arepresented in the literature, most of them target homogeneous processors. Existing algorithms for heterogeneous processors are not generally efficient because of their high complexity and the quality of their results. This thesisstudies the scheduling of DAG-structured application tasks on heterogeneous domains. We develop two novel low-complexity and efficient scheduling algorithms for bounded number of heterogeneous processors, the HeterogeneousEarliest-Finish-Time (HEFT) algorithm and the Critical-Path-on-a-Processor (CPOP) algorithm. The experimental work presented in this thesis shows that these algorithms significantly surpass previous approaches in terms of performance(schedule length ratio, speed-up, and frequency of best results) and cost (running time and time complexity). Our experimental work includes randomly generated graphs and graphs deducted from real applications. As part of thecomparison study, a parametric graph generator is introduced to generate graphs with various characteristics. We also present a further optimization of the HEFT Algorithm by introducing alternative methods for task prioritizing andprocessor selection phases. A novel processor selection policy based on the earliest finish time of the critical child task improves the performance of the HEFT algorithm. Several strategies for selecting the critical child task of agiven task are presented. This thesis addresses embedding the task scheduling algorithms into an application-development environment for distributed resources. An analytical model is introduced for setting the computation costs oftasks and communication costs of edges of a graph. As part of the design framework of our application development environment, a novel, two-phase, distributed scheduling algorithm is presented for scheduling an application overwide-area distributed resources.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">PROQUEST200009</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Computing and Computers</subfield>
<subfield code="a">Software De Apoyo Educativo Al Concepto De Funcion En Precalculo I (spanish Text)</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Rio Piedras</subfield>
<subfield code="b">Puerto Rico Univ.</subfield>
<subfield code="c">1999</subfield>
</datafield>
<datafield tag="270" ind1="" ind2="">
<subfield code="g">dir.</subfield>
<subfield code="p">Monroy, H</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">64 p</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">No fulltext</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">Not held by the library</subfield>
</datafield>
<datafield tag="502" ind1="" ind2="">
<subfield code="a">Ms : Univ. Puerto Rico : 1999</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">This thesis reports on the evaluation of the use of an educational software, designed to improve student's learning of the concept of mathematical function. The students in the study were registered in Precalculus I at theUniversity of Puerto Rico, Mayaguez Campus. The educational software allows the practice of changing the representation of a function among tabular, analytic, and graphical representations. To carry the evaluation, 59 students wereselected and were divided in two groups: control and experimental. Both groups received the 'traditional' classroom lectures on the topic. The experimental group, in addition, was allowed to practice with the educational software. Tomeasure their performance and the effect of the educational software, two tests were given: a pre-test and a post-test. The results of this study shows that the experimental group improved significantly more than the control group,thus demonstrating the validity of the educational software in the learning of the concept of mathematical function.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">PROQUEST200009</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Computing and Computers</subfield>
<subfield code="a">Systeme Multiagent Pour Les Environnements Riches En Informations (french Text)</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Laval</subfield>
<subfield code="b">Laval Univ.</subfield>
<subfield code="c">1999</subfield>
</datafield>
<datafield tag="270" ind1="" ind2="">
<subfield code="g">dir.</subfield>
<subfield code="p">Chaib-Draa, B</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">101 p</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">No fulltext</subfield>
</datafield>
<datafield tag="500" ind1="" ind2="">
<subfield code="a">Not held by the library</subfield>
</datafield>
<datafield tag="502" ind1="" ind2="">
<subfield code="a">Msc : Universite Laval : 1999</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">La croissance du Web est spectaculaire, puisqu'on estime aujourd'hui a plus de 50 millions, le nombre de pages sur le Web qui ne demandent qu'a etre consultees. Un simple calcul montre qu'en consacrant ne serait-ce qu'une minute parpage, il faudrait environ 95 ans pour consulter toutes ces pages. L'utilisation d'une strategie de recherche est donc vitale. Dans ce cadre, de nombreux outils de recherche ont ete proposes. Ces outils appeles souvent moteurs derecherche se sont averes aujourd'hui incapables de fournir de l'aide aux utilisateurs. Les raisons principales a cela sont les suivantes: (1) La nature ouverte de l'Internet: aucune supervision centrale ne s'applique quant audeveloppement d'Internet, puisque toute personne qui desire l'utiliser et/ou offrir des informations est libre de le faire; (2) La nature dynamique des informations: les informations qui ne sont pas disponibles aujourd'hui peuventl'etre demain et inversement; (3) La nature heterogene de l'information: l'information est offerte sous plusieurs formats et de plusieurs facons, compliquant ainsi la recherche automatique de l'information. Devant ce constat, ilsemble important de chercher de nouvelles solutions pour aider l'utilisateur dans sa recherche d'informations. (Abstract shortened by UMI.)</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">PROQUEST200009</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Computing and Computers</subfield>
<subfield code="a">Accelerators and Storage Rings</subfield>
</datafield>
<datafield tag="653" ind1="1" ind2="">
<subfield code="a">bibliography</subfield>
</datafield>
<datafield tag="690" ind1="C" ind2="">
<subfield code="a">REPORT</subfield>
</datafield>
<datafield tag="690" ind1="C" ind2="">
<subfield code="a">THESIS</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="b">14</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">1990-02-28</subfield>
<subfield code="l">50</subfield>
<subfield code="m">2002-03-22</subfield>
<subfield code="o">BATCH</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">h</subfield>
<subfield code="w">199010n</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">THESIS</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">gr-qc/0204045</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Khalatnikov, I M</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Comment about quasiisotropic solution of Einstein equations near cosmological singularity</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">7 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We generalize for the case of arbitrary hydrodynamical matter the quasiisotropic solution of Einstein equations near cosmological singularity, found by Lifshitz and Khalatnikov in 1960 for the case of radiation-dominated universe. Itis shown that this solution always exists, but dependence of terms in the quasiisotropic expansion acquires a more complicated form.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">General Relativity and Cosmology</subfield>
<subfield code="m">Lifshitz E M and Khalatnikov I M 1964 Sov. Phys. Uspekhi 6 495</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Landau L D and Lifshitz E M 1979 The Classical Theory of Fields (Perg-amon Press)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Starobinsky A A 1986 Stochastic De Sitter (inflationary stage) in the early universe in Field Theory, Quantum Gravity and Strings, (Eds. H.J. De Vega and N. Sanchez, Springer-Verlag, Berlin) 107; Linde A D 1990 Particle Physics and Inflationary Cosmology (Harward Academic Publishers, New York)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Banks T and Fischler W 2001 M theory observables for cosmolog-ical space-times</subfield>
<subfield code="m">Perlmutter S J et al 1999</subfield>
<subfield code="p">565</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">517</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Riess A et al 1998</subfield>
<subfield code="p">1009</subfield>
<subfield code="t">Astron. J.</subfield>
<subfield code="v">116</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Sahni V and Starobinsky A A 2000</subfield>
<subfield code="p">373</subfield>
<subfield code="t">Int. J. Mod. Phys., D</subfield>
<subfield code="v">9</subfield>
<subfield code="y">2000</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">gr-qc/0204046</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Bento, M C</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Supergravity Inflation on the Brane</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">5 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We study N=1 Supergravity inflation in the context of the braneworld scenario. Particular attention is paid to the problem of the onset of inflation at sub-Planckian field values and the ensued inflationary observables. We find thatthe so-called $\eta$-problem encountered in supergravity inspired inflationary models can be solved in the context of the braneworld scenario, for some range of the parameters involved. Furthermore, we obtain an upper bound on thescale of the fifth dimension, $M_5 \lsim 10^{-3} M_P$, in case the inflationary potential is quadratic in the inflaton field, $\phi$. If the inflationary potential is cubic in $\phi$, consistency with observational data requires that$M_5 \simeq 9.2 \times 10^{-4} M_P$.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">General Relativity and Cosmology</subfield>
</datafield>
<datafield tag="700" ind1="" ind2="">
<subfield code="a">Bertolami, O</subfield>
</datafield>
<datafield tag="700" ind1="" ind2="">
<subfield code="a">Sen, A A</subfield>
</datafield>
<datafield tag="856" ind1="0" ind2="">
<subfield code="f">Maria da Conceicao Bento <bento@sirius.ist.utl.pt></subfield>
<subfield code="a">Reply to 'Comment on "Solution of the Relativistic Dirac-Morse Problem"'</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">11 Apr 2002</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">This combines a reply to the Comment [hep-th/0203067 v1] by A. N. Vaidya and R. de L. Rodrigues with an erratum to our Letter [Phys. Rev. Lett. 87, 210405 (2001)]</subfield>
<subfield code="a">It has long been known that strings wound around incontractible cycles can play a vital role in cosmology. In particular, in a spacetime with toroidal spatial hypersurfaces, the dynamics of the winding modes may help yield threelarge spatial dimensions. However, toroidal compactifications are phenomenologically unrealistic. In this paper we therefore take a first step toward extending these cosmological considerations to $D$-dimensional toroidal orbifolds.We use numerical simulation to study the timescales over which "pseudo-wound" strings unwind on these orbifolds with trivial fundamental group. We show that pseudo-wound strings can persist for many ``Hubble times'' in some of thesespaces, suggesting that they may affect the dynamics in the same way as genuinely wound strings. We also outline some possible extensions that include higher-dimensional wrapped branes.</subfield>
<subfield code="m">R. Brandenberger and C. Vafa</subfield>
<subfield code="p">391</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">316</subfield>
<subfield code="y">1989</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. A. Tseytlin and C. Vafa</subfield>
<subfield code="p">443</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">372</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9109048</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Sakellariadou</subfield>
<subfield code="p">319</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">468</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9511075</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. G. Smith and A. Vilenkin</subfield>
<subfield code="p">990</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">36</subfield>
<subfield code="y">1987</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Brandenberger, D. A. Easson and D. Kimberly</subfield>
<subfield code="p">421</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">623</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0109165</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. R. Greene, A. D. Shapere, C. Vafa, and S. T. Yau</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">337</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Dixon, J. Harvey, C. Vafa and E. Witten</subfield>
<subfield code="p">678</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">261</subfield>
<subfield code="y">1985</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Dixon, J. Harvey, C. Vafa and E. Witten</subfield>
<subfield code="p">285</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">274</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Sakellariadou and A. Vilenkin</subfield>
<subfield code="p">885</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">37</subfield>
<subfield code="y">1988</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. J. Atick and E. Witten</subfield>
<subfield code="p">291</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">310</subfield>
<subfield code="y">1988</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Mitchell and N. Turok</subfield>
<subfield code="p">1577</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1987</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Imperial College report, 1987 (unpublished)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Alexander, R. Brandenberger, and D. Easson</subfield>
<subfield code="p">103509</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0005212</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Easson</subfield>
<subfield code="r">hep-th/0110225</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204132</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="088" ind1="" ind2="">
<subfield code="a">NUC-MINN-02-3-T</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Shovkovy, I A</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Thermal conductivity of dense quark matter and cooling of stars</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Minneapolis, MN</subfield>
<subfield code="b">Minnesota Univ.</subfield>
<subfield code="c">11 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">9 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">The thermal conductivity of the color-flavor locked phase of dense quark matter is calculated. The dominant contribution to the conductivity comes from photons and Nambu-Goldstone bosons associated with breaking of baryon numberwhich are trapped in the quark core. Because of their very large mean free path the conductivity is also very large. The cooling of the quark core arises mostly from the heat flux across the surface of direct contact with the nuclearmatter. As the thermal conductivity of the neighboring layer is also high, the whole interior of the star should be nearly isothermal. Our results imply that the cooling time of compact stars with color-flavor locked quark cores issimilar to that of ordinary neutron stars.</subfield>
<subfield code="m">J.C. Collins and M.J. Perry</subfield>
<subfield code="p">1353</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">34</subfield>
<subfield code="y">1975</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. C. Barrois</subfield>
<subfield code="p">390</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">129</subfield>
<subfield code="y">1977</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. C. Frautschi, in "Hadronic matter at extreme energy density", edited by N. Cabibbo and L. Sertorio (Plenum Press, 1980); D. Bailin and A. Love</subfield>
<subfield code="p">325</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">107</subfield>
<subfield code="y">1984</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. G. Alford, K. Rajagopal and F. Wilczek</subfield>
<subfield code="p">247</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">422</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Rapp, T. Schäfer, E. V. Shuryak and M. Velkovsky</subfield>
<subfield code="p">53</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">81</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. T. Son</subfield>
<subfield code="p">094019</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">59</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. D. Pisarski and D. H. Rischke</subfield>
<subfield code="p">37</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">83</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Schafer and F. Wilczek</subfield>
<subfield code="p">114033</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. K. Hong, V. A. Miransky, I. A. Shovkovy and L. C. R. Wijewardhana</subfield>
<subfield code="p">056001</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">erratum</subfield>
<subfield code="p">059903</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. D. Pisarski and D. H. Rischke</subfield>
<subfield code="p">051501</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. D. Hsu and M. Schwetz</subfield>
<subfield code="p">211</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">572</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. E. Brown, J. T. Liu and H. C. Ren</subfield>
<subfield code="p">114012</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. A. Shovkovy and L. C. R. Wijewardhana</subfield>
<subfield code="p">189</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">470</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Schäfer</subfield>
<subfield code="p">269</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">575</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Rajagopal and F. Wilczek, arXiv</subfield>
<subfield code="m">M. Alford and K. Rajagopal, arXiv</subfield>
<subfield code="r">hep-ph/0204001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Alford, K. Rajagopal and F. Wilczek</subfield>
<subfield code="p">443</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">537</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Casalbuoni and R. Gatto</subfield>
<subfield code="p">111</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">464</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. T. Son and M. A. Stephanov</subfield>
<subfield code="p">074012</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">erratum</subfield>
<subfield code="p">059902</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. F. Bedaque and T. Schäfer</subfield>
<subfield code="p">802</subfield>
<subfield code="t">Nucl. Phys., A</subfield>
<subfield code="v">697</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. A. Miransky and I. A. Shovkovy</subfield>
<subfield code="p">111601</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">88</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0108178</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Schafer, D. T. Son, M. A. Stephanov, D. Toublan and J. J. Ver-baarschot</subfield>
<subfield code="p">67</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">522</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0108210</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. T. Son, arXiv</subfield>
<subfield code="r">hep-ph/0108260</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Jaikumar, M. Prakash and T. Schäfer, arXiv</subfield>
<subfield code="r">astro-ph/0203088</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. J. Ferrer, V. P. Gusynin and V. de la Incera, arXiv: cond-matt/0203217</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. S. Gradshteyn and I. M. Ryzhik, Tables of Integrals, Series and Products (Academic, New York, 1965) 3.252.9</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. J. Freeman and A. C. Anderson</subfield>
<subfield code="p">5684</subfield>
<subfield code="t">Phys. Rev., B</subfield>
<subfield code="v">34</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Kittel, Introduction to Solid State Phys.(John Wi-ley & Sons, Inc., 1960) p. 139</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. P. Gusynin and I. A. Shovkovy</subfield>
<subfield code="p">577</subfield>
<subfield code="t">Nucl. Phys., A</subfield>
<subfield code="v">700</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. M. Khalatnikov, An introduction to the theory of su-perfluidity, (Addison-Wesley Pub. Co., 1989)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. A. Sturrock, Plasma Physics, (Cambridge University Press, 1994)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[24]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. M. Lattimer, K. A. Van Riper, M. Prakash and M. Prakash</subfield>
<subfield code="p">802</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">425</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[25]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. G. Alford, K. Rajagopal, S. Reddy and F. Wilczek</subfield>
<subfield code="p">074017</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">64</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[26]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. W. Carter and S. Reddy</subfield>
<subfield code="p">103002</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[27]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. W. Steiner, M. Prakash and J. M. Lattimer</subfield>
<subfield code="p">10</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">509</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">astro-ph/0101566</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Reddy, M. Sadzikowski and M. Tachibana, arXiv</subfield>
<subfield code="r">nucl-th/0203011</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Prakash, J. M. Lattimer, J. A. Pons, A. W. Steiner and S. Reddy</subfield>
<subfield code="p">364</subfield>
<subfield code="t">Lect. Notes Phys.</subfield>
<subfield code="v">578</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. L. Shapiro and S. A. Teukolsky, Black holes, white dwarfs, and neutron stars: the physics of compact ob-jects, (John Wiley & Sons, 1983)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[31]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Blaschke, H. Grigorian and D. N. Voskresensky, As-tron. Astrophys. : 368 (2001) 561</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[32]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Page, M. Prakash, J. M. Lattimer and A. W. Steiner</subfield>
<subfield code="p">2048</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">85</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[33]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Rajagopal and F. Wilczek</subfield>
<subfield code="p">3492</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">86</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[34]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. I. Kapusta, Finite-temperature field theory, (Cam-bridge University Press, 1989)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[35]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. M. Johns, P. J. Ellis and J. M. Lattimer</subfield>
<subfield code="p">1020</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">473</subfield>
<subfield code="y">1996</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204133</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Gomez, M E</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Lepton-Flavour Violation in SUSY with and without R-parity</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">11 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We study whether the individual violation of the lepton numbers L_{e,mu,tau} in the charged sector can lead to measurable rates for BR(mu->e gamma) and BR(tau->mu gamma). We consider three different scenarios, the fist onecorresponds to the Minimal Supersymmetric Standard Model with non-universal soft terms. In the other two cases the violation of flavor in the leptonic charged sector is associated to the neutrino problem in models with a see-sawmechanism and with R-parity violation respectively.</subfield>
<subfield code="b">TALK GIVEN BY M E G AT THE CORFU SUMMER INSTITUTE ON ELEMENTARY PARTICLE PHYSICS CORFU 2001 11 PAGES 5 FIGURES</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[1]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y. Fukuda et al., Super-Kamiokande collaboration</subfield>
<subfield code="p">9</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">433</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">33</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">436</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">1562</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">81</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Apollonio et al., Chooz collaboration</subfield>
<subfield code="p">397</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">420</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. N. Brown et al. [Muon g-2 Collaboration]</subfield>
<subfield code="p">2227</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">86</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ex/0102017</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Review of Particle Physics, D. E. Groom et al</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">15</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. F. Carvalho, M. E. Gomez and S. Khalil</subfield>
<subfield code="p">001</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">0107</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0104292</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. F. Carvalho, J. R. Ellis, M. Gomez and S. Lola</subfield>
<subfield code="p">323</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">515</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. F. Carvalho, M. E. Gomez and J. C. Romao</subfield>
<subfield code="r">hep-ph/0202054</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(to appear in Phys. Rev., D</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. R. Ellis, M. E. Gomez, G. K. Leontaris, S. Lola and D. V. Nanopoulos</subfield>
<subfield code="p">319</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">14</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Belyaev et al</subfield>
<subfield code="p">715</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">22</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Belyaev et al. [Kaon Physics Working Group Collaboration]</subfield>
<subfield code="r">hep-ph/0107046</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Hisano, T. Moroi, K. Tobe and M. Yamaguchi</subfield>
<subfield code="p">2442</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">53</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Hisano and D. Nomura</subfield>
<subfield code="p">116005</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">59</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Barbieri and L.J. Hall</subfield>
<subfield code="p">212</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">338</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Barbieri et al</subfield>
<subfield code="p">219</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">445</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Nima Arkani-Hamed, Hsin-Chia Cheng and L.J. Hall</subfield>
<subfield code="p">413</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">53</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Ciafaloni, A. Romanino and A. Strumia</subfield>
<subfield code="p">3</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">458</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. E. Gomez and H. Goldberg</subfield>
<subfield code="p">5244</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">53</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Hisano, D. Nomura, Y. Okada, Y. Shimizu and M. Tanaka</subfield>
<subfield code="p">116010</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. E. Gomez, G. K. Leontaris, S. Lola and J. D. Vergados</subfield>
<subfield code="p">116009</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">59</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G.K. Leontaris and N.D. Tracas</subfield>
<subfield code="p">90</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">431</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Buchmuller, D. Delepine and F. Vissani</subfield>
<subfield code="p">171</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">459</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Buchmuller, D. Delepine and L. T. Handoko</subfield>
<subfield code="p">445</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">576</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Q. Shafi and Z. Tavartkiladze</subfield>
<subfield code="p">145</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">473</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. L. Feng, Y. Nir and Y. Shadmi</subfield>
<subfield code="p">113005</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Brignole, L. E. Iba nez and C. Mu noz</subfield>
<subfield code="p">125</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">422</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[Erratum</subfield>
<subfield code="p">747</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">436</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Iba nez and G.G. Ross</subfield>
<subfield code="p">100</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">332</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G.K. Leontaris, S. Lola and G.G. Ross</subfield>
<subfield code="p">25</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">454</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Lola and G.G. Ross</subfield>
<subfield code="p">81</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">553</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Gell-Mann, P. Ramond and R. Slansky, Proceedings of the Stony Brook Super-gravity Workshop, New York, 1979, eds. P. Van Nieuwenhuizen and D. Freedman (North-Holland, Amsterdam)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. A. Casas and A. Ibarra</subfield>
<subfield code="p">171</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">618</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Lavignac, I. Masina and C. A. Savoy</subfield>
<subfield code="p">269</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">520</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="r">hep-ph/0202086</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. R. Ellis, D. V. Nanopoulos and K. A. Olive</subfield>
<subfield code="p">65</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">508</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. C. Romao, M. A. Diaz, M. Hirsch, W. Porod and J. W. Valle</subfield>
<subfield code="p">071703</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">113008</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. E. Gomez and K. Tamvakis</subfield>
<subfield code="p">057701</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Hirsch, W. Porod, J. W. F. Valle and J. C. Rom ao</subfield>
<subfield code="r">hep-ph/0202149</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. M. Barkov et al., Research Proposal to PSI, 1999</subfield>
<subfield code="m">Y. Kuno, Lep-ton Flavor Violation Experiments at KEK/JAERI Joint Project of High Intensity Proton Machine, in Proceedings of Workshop of "LOWNU/NOON 2000", Tokyo, December 4-8, 2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Porod, M. Hirsch, J. Rom ao and J. W. Valle</subfield>
<subfield code="p">115004</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">63</subfield>
<subfield code="y">2001</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204134</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Dzuba, V A</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Precise calculation of parity nonconservation in cesium and test of the standard model</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">24 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We have calculated the 6s-7s parity nonconserving (PNC) E1 transition amplitude, E_{PNC}, in cesium. We have used an improved all-order technique in the calculation of the correlations and have included all significant contributionsto E_{PNC}. Our final value E_{PNC} = 0.904 (1 +/- 0.5 %) \times 10^{-11}iea_{B}(-Q_{W}/N) has half the uncertainty claimed in old calculations used for the interpretation of Cs PNC experiments. The resulting nuclear weak chargeQ_{W} for Cs deviates by about 2 standard deviations from the value predicted by the standard model.</subfield>
<subfield code="m">R.J. Rafac, C.E. Tanner, A.E. Livingston, and H.G. Berry</subfield>
<subfield code="p">3648</subfield>
<subfield code="t">Phys. Rev., A</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[36]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.-A. Bouchiat, J. Gu´ena, and L. Pottier, J. Phys.(France) Lett. : 45 (1984) L523</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[37]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. Arimondo, M. Inguscio, and P. Violino</subfield>
<subfield code="p">31</subfield>
<subfield code="t">Rev. Mod. Phys.</subfield>
<subfield code="v">49</subfield>
<subfield code="y">1977</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[38]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.L. Gilbert, R.N. Watts, and C.E. Wieman</subfield>
<subfield code="p">581</subfield>
<subfield code="t">Phys. Rev., A</subfield>
<subfield code="v">27</subfield>
<subfield code="y">1983</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[39]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R.J. Rafac and C.E. Tanner</subfield>
<subfield code="p">1027</subfield>
<subfield code="t">Phys. Rev., A</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[40]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.-A. Bouchiat and J. Gu´ena, J. Phys.(France) : 49 (1988) 2037</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[41]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. Cho et al</subfield>
<subfield code="p">1007</subfield>
<subfield code="t">Phys. Rev., A</subfield>
<subfield code="v">55</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[42]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.A. Vasilyev, I.M. Savukov, M.S. Safronova, and H.G. Berry, e-print</subfield>
<subfield code="r">physics/0112071</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204135</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Bertin, V</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Neutrino Indirect Detection of Neutralino Dark Matter in the CMSSM</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">16 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We study potential signals of neutralino dark matter indirect detection by neutrino telescopes in a wide range of CMSSM parameters. We also compare with direct detection potential signals taking into account in both cases present andfuture experiment sensitivities. Only models with neutralino annihilation into gauge bosons can satisfy cosmological constraints and current neutrino indirect detection sensitivities. For both direct and indirect detection, only nextgeneration experiments will be able to really test this kind of models.</subfield>
<subfield code="a">Supersymmetry and a rationale for small CP violating phases</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">28 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We analyse the CP problem in the context of a supersymmetric extension of the standard model with universal strength of Yukawa couplings. A salient feature of these models is that the CP phases are constrained to be very small by thehierarchy of the quark masses, and the pattern of CKM mixing angles. This leads to a small amount of CP violation from the usual KM mechanism and a significant contribution from supersymmetry is required. Due to the large generationmixing in some of the supersymmetric interactions, the electric dipole moments impose severe constraints on the parameter space, forcing the trilinear couplings to be factorizable in matrix form. We find that the LL mass insertionsgive the dominant gluino contribution to saturate epsilon_K. The chargino contributions to epsilon'/epsilon are significant and can accommodate the experimental results. In this framework, the standard model gives a negligiblecontribution to the CP asymmetry in B-meson decay, a_{J/\psi K_s}. However, due to supersymmetric contributions to B_d-\bar{B}_d mixing, the recent large value of a_{J/\psi K_s} can be accommodated.</subfield>
<subfield code="m">M.B. Gavela, P. Hernandez, J. Orloff, O. P ene and C. Quimbay</subfield>
<subfield code="p">345</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">430</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">382</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">430</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.D. Dolgov</subfield>
<subfield code="r">hep-ph/9707419</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V.A. Rubakov and M.E. Shaposhnikov, Usp. Fiz. Nauk : 166 (1996) 493[</subfield>
<subfield code="p">461</subfield>
<subfield code="t">Phys. Usp.</subfield>
<subfield code="v">39</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Abel, S. Khalil and O. Lebedev</subfield>
<subfield code="p">151</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">606</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Pokorski, J. Rosiek and C. A. Savoy</subfield>
<subfield code="p">81</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">570</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Recent Developments in Gauge Theories, Proceedings of Nato Advanced Study Insti-tute (Carg ese, 1979), edited by G. 't Hooft et al., Plenum, New York (1980)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. C. Branco, J. I. Silva-Marcos and M. N. Rebelo</subfield>
<subfield code="p">446</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">237</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. C. Branco, D. EmmanuelCosta and J. I. Silva-Marcos</subfield>
<subfield code="p">107</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. M. Fishbane and P. Q. Hung</subfield>
<subfield code="p">2743</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">57</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Q. Hung and M. Seco</subfield>
<subfield code="r">hep-ph/0111013</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. C. Branco and J. I. Silva-Marcos</subfield>
<subfield code="p">166</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">359</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. V. Romalis, W. C. Griffith and E. N. Fortson</subfield>
<subfield code="p">2505</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">86</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. P. Jacobs et al</subfield>
<subfield code="p">3782</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">71</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">BABAR Collaboration, B. Aubert et al</subfield>
<subfield code="p">091801</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">87</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">BELLE Collaboration, K. Abe et al</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">10</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Khalil and O. Lebedev</subfield>
<subfield code="p">387</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">515</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. J. Buras</subfield>
<subfield code="r">hep-ph/0101336</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">See, for example, G. C. Branco, L. Lavoura and J. P. Silva, CP Violation, Interna-tional Series of Monographs on Physics (103), Oxford University Press, Clarendon (1999)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[31]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. Gabbiani, E. Gabrielli, A. Masiero and L. Silverstrini</subfield>
<subfield code="p">321</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">477</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[32]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Fanti et al</subfield>
<subfield code="p">335</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">465</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[33]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Gershon (NA48)</subfield>
<subfield code="r">hep-ex/0101034</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[34]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. J. Buras, M. Jamin and M. E. Lautenbacher</subfield>
<subfield code="p">209</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">408</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[35]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Bertolini, M. Fabbrichesi and E. Gabrielli</subfield>
<subfield code="p">136</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">327</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[36]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Colangelo and G. Isidori</subfield>
<subfield code="p">009</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">09</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Buras, G. Colan-gelo, G. Isidori, A. Romanino and L. Silvestrini</subfield>
<subfield code="p">3</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">566</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[37]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">OPAL Collaboration, K. Ackerstaff et al</subfield>
<subfield code="p">379</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">5</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">CDF Collaboration, T. Affolder et al</subfield>
<subfield code="p">072005</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">CDF Collaboration, C. A. Blocker, Proceedings of 3rd Workshop on Physics and Detectors for DAPHNE (DAPHNE 99), Frascati, Italy, 16-19 Nov 1999; ALEPH Collaboration, R. Barate et al</subfield>
<subfield code="p">259</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">492</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[38]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Bertolini, F. Borzumati, A. Masiero and G. Ridolfi</subfield>
<subfield code="p">591</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">353</subfield>
<subfield code="y">1991</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[39]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">CLEO Collaboration, S. Ahmed et al, CLEO-CONF-99-10</subfield>
<subfield code="r">hep-ex/9908022</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[40]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. Gabrielli, S. Khalil and E. TorrenteLujan</subfield>
<subfield code="p">3</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">594</subfield>
<subfield code="y">2001</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204137</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="088" ind1="" ind2="">
<subfield code="a">DO-TH-02-05</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Paschos, E A</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Leptogenesis with Majorana neutrinos</subfield>
<subfield code="a">I review the origin of the lepton asymmetry which is converted to a baryon excess at the electroweak scale. This scenario becomes more attractive if we can relate it to other physical phenomena. For this reason I elaborate on theconditions of the early universe which lead to a sizable lepton asymmetry. Then I describe methods and models which relate the low energy parameters of neutrinos to the high energy (cosmological) CP-violation and to neutrinolessdouble beta-decay.</subfield>
<subfield code="b">CONTRIBUTED TO 1ST WORKSHOP ON NEUTRINO - NUCLEUS INTERACTIONS IN THE FEW GEV REGION (NUINT01) TSUKUBA JAPAN 13-16 DEC 2001 6 PAGES 6 FIGURES</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">1.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Fukugida and Yanagida</subfield>
<subfield code="p">45</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">174</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">2.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Flanz, E.A. Paschos and U. Sarkar</subfield>
<subfield code="p">248</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">345</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">3.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Luty</subfield>
<subfield code="p">445</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">45</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">4.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Flanz, E.A. Paschos, U. Sarkar and J. Weiss</subfield>
<subfield code="p">693</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">389</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Flanz and E.A. Paschos</subfield>
<subfield code="p">113009</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">5.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Pilaftsis</subfield>
<subfield code="p">5431</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">6.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">W. Buchmüller and M. Plümacher</subfield>
<subfield code="p">354</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">431</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">7.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Covi, E. Roulet and F. Vissani</subfield>
<subfield code="p">169</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">384</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">8.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E.K. Akhmedov, V.A. Rubakov and A.Y. Smirnov</subfield>
<subfield code="p">1359</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">81</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">9.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.Y. Khlepnikov and M.E. Shaposhnikov</subfield>
<subfield code="a">We discuss the calculations for several neutrino induced reactions from low energies to the GeV region. Special attention is paid to nuclear corrections when the targets are medium or heavy nuclei. Finally, we present several ratiosof neutral to charged current reactions whose values on isoscalar targets can be estimated accurately. The ratios are useful for investigating neutrino oscillations in Long Baseline experiments.</subfield>
<subfield code="b">CONTRIBUTED TO 1ST WORKSHOP ON NEUTRINO - NUCLEUS INTERACTIONS IN THE FEW GEV REGION (NUINT01) TSUKUBA JAPAN 13-16 DEC 2001 9 PAGES 15 FIGURES</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">1.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. A. Paschos, L. Pasquali and J. Y. Yu</subfield>
<subfield code="p">263</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">588</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">2.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. A. Paschos and J. Y. Yu</subfield>
<subfield code="p">033002</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">65</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">3.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Albright and C. Jarlskog</subfield>
<subfield code="p">467</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">84</subfield>
<subfield code="y">1975</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">4.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. J. Baker et al</subfield>
<subfield code="p">617</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">25</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">5.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Hirai, S. Kumano and M. Miyama</subfield>
<subfield code="p">034003</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">64</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">6.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. J. Eskola, V. J. Kolhinen and P. V. Ru-uskanen</subfield>
<subfield code="p">351</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">535</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. J. Eskola, V. J. Kolhinen, P. V. Ruuskanen and C. A. Salgado</subfield>
<subfield code="p">645</subfield>
<subfield code="t">Nucl. Phys., A</subfield>
<subfield code="v">661</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">7.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">See Figure 1 in Ref. [2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">8.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. A. Schreiner and F. V. von Hippel</subfield>
<subfield code="p">333</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1973</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">9.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. L. Adler, S. Nussinov. and E. A. Paschos</subfield>
<subfield code="p">2125</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">9</subfield>
<subfield code="y">1974</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">10.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. L. Adler</subfield>
<subfield code="p">2644</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">12</subfield>
<subfield code="y">1975</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">11.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Musset and J. P. Vialle</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">39</subfield>
<subfield code="y">1978</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">12.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. Kluttig, J. G. Morfin and W. Van Do-minick</subfield>
<subfield code="p">446</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">71</subfield>
<subfield code="y">1977</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">13.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Merenyi et al</subfield>
<subfield code="p">743</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">45</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">14.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. K. Singh, M. T. Vicente-Vacas and E. Oset</subfield>
<subfield code="p">23</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">416</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">15.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. A. Paschos and L. Wolfenstein</subfield>
<subfield code="p">91</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">7</subfield>
<subfield code="y">1973</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">see equation (15)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">16.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. A. Paschos, Precise Ratios for Neutrino-Nucleon and Neutrino-Nucleus Interactions, Dortmund preprintDOTH 02/02; hep-ph 0204090</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">17.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Gounaris, E. A. Paschos and P. Porfyri-adis</subfield>
<subfield code="p">63</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">525</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">18.</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Bouchez and I. Giomataris, CEA/Saclay internal note, DAPNIA/01-07, June 2001</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204139</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Van Beveren, E</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Remarks on the f_0(400-1200) scalar meson as the dynamically generated chiral partner of the pion</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">15 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">The quark-level linear sigma model is revisited, in particular concerning the identification of the f_0(400-1200) (or \sigma(600)) scalar meson as the chiral partner of the pion. We demonstrate the predictive power of the linearsigma model through the pi-pi and pi-N s-wave scattering lengths, as well as several electromagnetic, weak, and strong decays of pseudoscalar and vector mesons. The ease with which the data for these observables are reproduced in thelinear sigma model lends credit to the necessity to include the sigma as a fundamental q\bar{q} degree of freedom, to be contrasted with approaches like chiral perturbation theory or the confining NJL model of Shakin and Wang.</subfield>
<subfield code="m">D. E. Groom et al. [Particle Data Group Collaboration]</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">15</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Isgur and J. Speth</subfield>
<subfield code="p">2332</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">77</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. A. Törnqvist and M. Roos</subfield>
<subfield code="p">1575</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">76</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9511210</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Harada, F. Sannino, and J. Schechter</subfield>
<subfield code="p">1603</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">78</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9609428</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. van Beveren, T. A. Rijken, K. Metzger, C. Dullemond, G. Rupp, and J. E. Ribeiro</subfield>
<subfield code="p">615</subfield>
<subfield code="t">Z. Phys., C</subfield>
<subfield code="v">30</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Eef van Beveren and George Rupp</subfield>
<subfield code="p">469</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">10</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9806246</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Boglione and M. R. Pennington</subfield>
<subfield code="r">hep-ph/0203149</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Gell-Mann and M. L´evy</subfield>
<subfield code="p">705</subfield>
<subfield code="t">Nuovo Cimento</subfield>
<subfield code="v">16</subfield>
<subfield code="y">1960</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">also see V. de Alfaro, S. Fubini, G. Furlan, and C. Rossetti, in Currents in Hadron Physics, North-Holland Publ., Amsterdam, Chap. 5 (1973)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Delbourgo and M. D. Scadron</subfield>
<subfield code="p">251</subfield>
<subfield code="t">Mod. Phys. Lett., A</subfield>
<subfield code="v">10</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9910242</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">657</subfield>
<subfield code="t">Int. J. Mod. Phys., A</subfield>
<subfield code="v">13</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9807504</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y. Nambu and G. Jona-Lasinio</subfield>
<subfield code="p">345</subfield>
<subfield code="t">Phys. Rev.</subfield>
<subfield code="v">122</subfield>
<subfield code="y">1961</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. M. Shakin and Huangsheng Wang</subfield>
<subfield code="p">094020</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">64</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. M. Shakin and Huangsheng Wang</subfield>
<subfield code="p">014019</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">63</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Rupp, E. van Beveren, and M. D. Scadron</subfield>
<subfield code="p">078501</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">65</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0104087</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Eef van Beveren, George Rupp, and Michael D. Scadron</subfield>
<subfield code="p">300</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">495</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[Erratum</subfield>
<subfield code="p">365</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">509</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">]</subfield>
<subfield code="r">hep-ph/0009265</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Frieder Kleefeld, Eef van Beveren, George Rupp, and Michael D. Scadron</subfield>
<subfield code="r">hep-ph/0109158</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. D. Scadron</subfield>
<subfield code="p">239</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">26</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">2076</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">29</subfield>
<subfield code="y">1984</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">669</subfield>
<subfield code="t">Mod. Phys. Lett., A</subfield>
<subfield code="v">7</subfield>
<subfield code="y">1992</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. L´evy</subfield>
<subfield code="p">23</subfield>
<subfield code="t">Nuovo Cimento, A</subfield>
<subfield code="v">52</subfield>
<subfield code="y">1967</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Gasiorowicz and D. A. Geffen</subfield>
<subfield code="p">531</subfield>
<subfield code="t">Rev. Mod. Phys.</subfield>
<subfield code="v">41</subfield>
<subfield code="y">1969</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Schechter and Y. Ueda</subfield>
<subfield code="a">A new model-independent way of extracting |V_ub/V_cb|</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="a">Geneva</subfield>
<subfield code="b">CERN</subfield>
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">20 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">The ratio between the photon spectrum in B -> X_s gamma and the differential semileptonic rate wrt the hadronic variable M_X/E_X is a short-distance quantity calculable in perturbation theory and independent of the Fermi motion ofthe b quark in the B meson. We present a NLO analysis of this ratio and show how it can be used to determine |V_ub/V_cb| independently of any model for the shape function. We also discuss how this relation can be used to test thevalidity of the shape-function theory on the data.</subfield>
<subfield code="m">C. W. Bauer, Z. Ligeti and M. E. Luke</subfield>
<subfield code="p">395</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">479</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0002161</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. W. Bauer, Z. Ligeti and M. E. Luke</subfield>
<subfield code="p">113004</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">64</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0107074</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">U. Aglietti, arXiv</subfield>
<subfield code="r">hep-ph/0010251</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">U. Aglietti</subfield>
<subfield code="p">308</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">515</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0103002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">U. Aglietti</subfield>
<subfield code="p">293</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">610</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0104020</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Ali and E. Pietarinen</subfield>
<subfield code="p">519</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">154</subfield>
<subfield code="y">1979</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Altarelli, N. Cabibbo, G. Corb o, L. Maiani and G. Martinelli</subfield>
<subfield code="p">365</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">208</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. L. Jaffe and L. Randall</subfield>
<subfield code="p">79</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">412</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9306201</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Neubert</subfield>
<subfield code="p">3392</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">49</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9311325</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">U. Aglietti, M. Ciuchini, G. Corb o, E. Franco, G. Martinelli and L. Silvestrini</subfield>
<subfield code="p">411</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">432</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9804416</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Catani, L. Trentadue, G. Turnock and B. R. Webber</subfield>
<subfield code="p">3</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">407</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Lubicz</subfield>
<subfield code="p">116</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">94</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-lat/0012003</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. J. Buras, M. Jamin, M. E. Lautenbacher and P. H. Weisz</subfield>
<subfield code="p">37</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">400</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9211304</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Ciuchini, E. Franco, G. Martinelli and L. Reina</subfield>
<subfield code="p">403</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">415</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9304257</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Chetyrkin, M. Misiak and M. Munz</subfield>
<subfield code="p">206</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">400</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[Erratum</subfield>
<subfield code="p">414</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">425</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">] [arXiv</subfield>
<subfield code="r">hep-ph/9612313</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and refs. therein</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Gambino and M. Misiak</subfield>
<subfield code="p">338</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">611</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0104034</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.B. Voloshin</subfield>
<subfield code="p">275</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">397</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Khodjamirian et al</subfield>
<subfield code="p">167</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">402</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Z. Ligeti, L. Randall and M.B. Wise</subfield>
<subfield code="p">178</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">402</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.K. Grant, A.G. Morgan, S. Nussinov and R.D. Peccei</subfield>
<subfield code="p">3151</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Buchalla, G. Isidori and S.J. Rey</subfield>
<subfield code="p">594</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">511</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Gambino and U. Haisch</subfield>
<subfield code="p">020</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">0110</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0109058</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">and</subfield>
<subfield code="p">001</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">0009</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0007259</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[24]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. De Fazio and M. Neubert</subfield>
<subfield code="p">017</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">9906</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9905351</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[25]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">U. Aglietti, arXiv</subfield>
<subfield code="r">hep-ph/0105168</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">to appear in the Proceedings of "XIII Convegno sulla Fisica al LEP (LEPTRE 2001)", Rome (Italy), 18-20 April 2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[26]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. van Ritbergen</subfield>
<subfield code="p">353</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">454</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[27]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. W. Bauer, M. E. Luke and T. Mannel, arXiv</subfield>
<subfield code="r">hep-ph/0102089</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">The Particle Data Group</subfield>
<subfield code="p">1</subfield>
<subfield code="t">Eur. Phys. J., C</subfield>
<subfield code="v">15</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Ciuchini et al</subfield>
<subfield code="p">013</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">0107</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0012308</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Chen et al., CLEO Coll</subfield>
<subfield code="p">251807</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">87</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[31]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Pott</subfield>
<subfield code="p">938</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">54</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9512252</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[32]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Greub, T. Hurth and D. Wyler</subfield>
<subfield code="p">3350</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">54</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/9603404</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. J. Buras, A. Czarnecki, M. Misiak and J. Urban</subfield>
<subfield code="p">488</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">611</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">[arXiv</subfield>
<subfield code="r">hep-ph/0105160</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[33]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. J. Buras, A. Czarnecki, M. Misiak and J. Urban, arXiv</subfield>
<subfield code="r">hep-ph/0203135</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204141</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Appelquist, T</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Neutrino Masses in Theories with Dynamical Electroweak Symmetry Breaking</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">4 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We address the problem of accounting for light neutrino masses in theories with dynamical electroweak symmetry breaking. As a possible solution, we embed (extended) technicolor in a theory in which a $|\Delta L|=2$ neutrinocondensate forms at a scale $\Lambda_N \gsim 10^{11}$ GeV, and produces acceptably small (Majorana) neutrino masses. We present an explicit model illustrating this mechanism.</subfield>
<subfield code="m">S. Fukuda et al., ibid, 5656 (2001) (SuperK) and Q.R. Ahmad et al</subfield>
<subfield code="p">071301</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">87</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(SNO). Other data is from the Homestake, Kamiokande, GALLEX, and SAGE experiments</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y. Fukuda et al</subfield>
<subfield code="p">9</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">433</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">1562</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">81</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">2644</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">82</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">185</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">467</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(SuperK) and data from Kamiokande, IMB, Soudan-2, and MACRO experiments. The data, which is consistent with results from K2K, indicates that |m( 3)2 - m( 2)2| |m( 3)2 - m( 1)2| 2.5 × 10-3 eV2. With a hierarchical mass assumption, one infers m( 3) m232 0.05 eV</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Weinberg</subfield>
<subfield code="p">1277</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">19</subfield>
<subfield code="y">1979</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Susskind</subfield>
<subfield code="p">2619</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">20</subfield>
<subfield code="y">1979</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. Eichten and K. Lane</subfield>
<subfield code="p">125</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">90</subfield>
<subfield code="y">1980</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Sikivie, L. Susskind, M. Voloshin, and V. Zakharov</subfield>
<subfield code="p">189</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">173</subfield>
<subfield code="y">1980</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Holdom</subfield>
<subfield code="p">301</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">150</subfield>
<subfield code="y">1985</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K Yamawaki, M. Bando, and K. Matumoto</subfield>
<subfield code="p">1335</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">56</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist, D. Karabali, and L. Wijeward-hana</subfield>
<subfield code="p">957</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">57</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist and L.C.R. Wijewardhana</subfield>
<subfield code="p">774</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">35</subfield>
<subfield code="y">1987</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">568</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">36</subfield>
<subfield code="y">1987</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Holdom</subfield>
<subfield code="p">1637</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">23</subfield>
<subfield code="y">1981</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">169</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">246</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist and J. Terning</subfield>
<subfield code="p">139</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">315</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist, J. Terning, and L. Wijewardhana</subfield>
<subfield code="p">1214</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">77</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">2767</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">79</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist, N. Evans, S. Selipsky</subfield>
<subfield code="p">145</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">374</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist and S. Selipsky</subfield>
<subfield code="p">364</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">400</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist, J. Terning</subfield>
<subfield code="p">2116</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">50</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Recent reviews include R. Chivukula</subfield>
<subfield code="r">hep-ph/0011264</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Lane</subfield>
<subfield code="r">hep-ph/0202255</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Hill E. Simmons</subfield>
<subfield code="r">hep-ph/0203079</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Gell-Mann, P. Ramond, R. Slansky, in Supergrav-ity (North Holland, Amsterdam, 1979), p. 315; T. Yanagida in proceedings of Workshop on Unified Theory and Baryon Number in the Universe, KEK, 1979</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Although we require our model to yield a small S, a re-analysis of precision electroweak data is called for in view of the value of sin2 W reported in G. Zeller et al</subfield>
<subfield code="p">091802</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">88</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">For a vectorial SU(N) theory with Nf fermions in the fundamental representation, an IRFP occurs if Nf > Nf,min,IR, where, perturbatively, Nf,min,IR 34N3/(13N2 -3). At this IRFP, using the criticality con-dition [13], the theory is expected to exist in a confining phase with S SB if Nf,min,IR < Nf < Nf,con, where Nf,con (2/5)N(50N2 - 33)/(5N2 - 3) and in a confor-mal phase if Nf,con < Nf < 11N/2. For N = 2 we have Nf,min,IR 5 and Nf,con 8, respectively. For attempts at lattice measurements, see R. Mawhinney</subfield>
<subfield code="p">57</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">83</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">In the approximation of a single-gauge-boson exchange, the critical coupling for the condensation of fermion rep-resentations R1 × R2 Rc is 3 2 C2 = 1, where C2 = [C2(R1) + C2(R2) - C2(Rc)], and C2(R) is the quadratic Casimir invariant. Instanton contributions are also important [7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Gasser, H. Leutwyler</subfield>
<subfield code="p">77</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">87</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. Leutwyler, in</subfield>
<subfield code="p">108</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">94</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Ali Khan et al</subfield>
<subfield code="p">4674</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">85</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Wingate et al., Int. J. Mod. Phys., A16 S B1 (2001) 585</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Here a = exp[ETC,a fF (dµ/µ) ( (µ))], and in walking TC theories the anomalous dimension 1 so a ETC,a/fF</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">By convention, we write SM-singlet neutrinos as right-handed fields j,R. These are assigned lepton number 1. Thus, in writing SU(4)PS SU(3)c × U(1), the U(1) is not U(1)B-L since some neutrinos in the model are SU(4)PS-singlet states</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Z. Maki, M. Nakagawa, S. Sakata</subfield>
<subfield code="p">870</subfield>
<subfield code="t">Prog. Theor. Phys.</subfield>
<subfield code="v">28</subfield>
<subfield code="y">1962</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(2 × 2 matrix); B. W. Lee, S. Pakvasa, R. Shrock, and H. Sugawara</subfield>
<subfield code="p">937</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">38</subfield>
<subfield code="y">1977</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">(3 × 3 matrix)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist and R. Shrock, to appear</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Dienes, E. Dudas, T. Gherghetta</subfield>
<subfield code="p">25</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">557</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and J. March-Russell</subfield>
<subfield code="r">hep-ph/9811448</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Appelquist, B. Dobrescu, E. Ponton, and H.-U. Yee</subfield>
<subfield code="a">We describe the effective supergravity theory present below the scale of spontaneous gauge symmetry breaking due to an anomalous U(1), obtained by integrating out tree-level interactions of massive modes. A simple case is examined insome detail. We find that the effective theory can be expressed in the linear multiplet formulation, with some interesting consequences. Among them, the modified linearity conditions lead to new interactions not present in the theorywithout an anomalous U(1). These additional interactions are compactly expressed through a superfield functional.</subfield>
<subfield code="a">Recent experimental data indicates that the fine structure constant alpha may be varying on cosmological time scales. We consider the possibility that such a variation could be induced by a second order phase transition which occursat late times (z ~ 1 - 3) and involves a change in the vacuum expectation value (vev) of a scalar with milli-eV mass. Such light scalars are natural in supersymmetric theories with low SUSY breaking scale. If the vev of this scalarcontributes to masses of electrically charged fields, the low-energy value of alpha changes during the phase transition. The observational predictions of this scenario include isotope-dependent deviations from Newtonian gravity atsub-millimeter distances, and (if the phase transition is a sharp event on cosmological time scales) the presence of a well-defined step-like feature in the alpha(z) plot. The relation between the fractional changes in alpha and theQCD confinement scale is highly model dependent, and even in grand unified theories the change in alpha does not need to be accompanied by a large shift in nucleon masses.</subfield>
<subfield code="m">J. K. Webb, M. T. Murphy, V. V. Flambaum, V. A. Dzuba, J. D. Barrow, C. W. Churchill, J. X. Prochaska and A. M. Wolfe</subfield>
<subfield code="p">091301</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">87</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/0012539</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">see also J. K. Webb, V. V. Flambaum, C. W. Churchill, M. J. Drinkwater and J. D. Barrow</subfield>
<subfield code="p">884</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">82</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/9803165</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. A. Dzuba, V. V. Flambaum, and J. K. Webb</subfield>
<subfield code="p">888</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">82</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. A. Dirac</subfield>
<subfield code="p">323</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">139</subfield>
<subfield code="y">1937</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">for an historial perspective, see F. Dyson, "The fundamental constants and their time variation", in Aspects of Quantum Theory, eds A. Salam and E. Wigner</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Damour</subfield>
<subfield code="r">gr-qc/0109063</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. D. Bekenstein</subfield>
<subfield code="p">1527</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">25</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. R. Dvali and M. Zaldarriaga</subfield>
<subfield code="p">091303</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">88</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0108217</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. A. Olive and M. Pospelov</subfield>
<subfield code="p">085044</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">65</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0110377</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Banks, M. Dine and M. R. Douglas</subfield>
<subfield code="p">131301</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">88</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0112059</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Langacker, G. Segr e and M. J. Strassler</subfield>
<subfield code="p">121</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">528</subfield>
<subfield code="y">2002</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0112233</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Y. Potekhin, A. V. Ivanchik, D. A. Varshalovich, K. M. Lanzetta, J. A. Bald-win, G. M. Williger and R. F. Carswell</subfield>
<subfield code="p">523</subfield>
<subfield code="t">Astrophys. J.</subfield>
<subfield code="v">505</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/9804116</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Weinberg</subfield>
<subfield code="p">3357</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">9</subfield>
<subfield code="y">1974</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Dolan and R. Jackiw</subfield>
<subfield code="p">3320</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">9</subfield>
<subfield code="y">1974</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Arkani-Hamed, L. J. Hall, C. Kolda and H. Murayama</subfield>
<subfield code="p">4434</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">85</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/0005111</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Dine, W. Fischler and M. Srednicki</subfield>
<subfield code="p">575</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">189</subfield>
<subfield code="y">1981</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Dimopou-los and S. Raby</subfield>
<subfield code="p">353</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">192</subfield>
<subfield code="y">1981</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Alvarez-Gaum´e, M. Claudson and M. B. Wise</subfield>
<subfield code="p">96</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">207</subfield>
<subfield code="y">1982</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Dine and A. E. Nelson</subfield>
<subfield code="p">1277</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">48</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9303230</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Dine, A. E. Nelson and Y. Shirman</subfield>
<subfield code="p">1362</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">51</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9408384</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Dine, A. E. Nelson, Y. Nir and Y. Shirman</subfield>
<subfield code="p">2658</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">53</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9507378</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N. Arkani-Hamed, S. Dimopoulos, N. Kaloper and R. Sundrum</subfield>
<subfield code="p">193</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">480</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0001197</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Kachru, M. Schulz and E. Silverstein</subfield>
<subfield code="p">045021</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0001206</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. Cs´aki, J. Erlich and C. Grojean</subfield>
<subfield code="p">312</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">604</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0012143</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">X. Calmet and H. Fritzsch</subfield>
<subfield code="r">hep-ph/0112110</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. Fritzsch</subfield>
<subfield code="r">hep-ph/0201198</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. R. Dvali and S. Pokorski</subfield>
<subfield code="p">126</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">379</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9601358</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Z. Chacko and R. N. Mohapatra</subfield>
<subfield code="p">2836</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">82</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9810315</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. P. Turneaure, C. M. Will, B. F. Farrell, E. M. Mattison and R. F. C. Vessot</subfield>
<subfield code="p">1705</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">27</subfield>
<subfield code="y">1983</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. D. Prestage, R. L. Tjoelker and L. Maleki</subfield>
<subfield code="p">3511</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">74</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. I. Shlyakhter</subfield>
<subfield code="p">340</subfield>
<subfield code="t">Nature</subfield>
<subfield code="v">264</subfield>
<subfield code="y">1976</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T. Damour and F. Dyson</subfield>
<subfield code="p">37</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">480</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9606486</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y. Fujii, A. Iwamoto, T. Fukahori, T. Ohnuki, M. Nakagawa, H. Hidaka, Y. Oura, P. Möller</subfield>
<subfield code="p">377</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">573</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9809549</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. W. Kolb, M. J. Perry and T. P. Walker</subfield>
<subfield code="p">869</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">33</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. A. Camp-bell and K. A. Olive</subfield>
<subfield code="p">429</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">345</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/9411272</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Bergström, S. Iguri and H. Rubinstein</subfield>
<subfield code="p">045005</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/9902157</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. P. Avelino et al</subfield>
<subfield code="p">103505</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">64</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/0102144</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Hannestad</subfield>
<subfield code="p">023515</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/9810102</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Kaplinghat, R. J. Scherrer and M. S. Turner</subfield>
<subfield code="p">023516</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/9810133</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. P. Avelino, C. J. Martins, G. Rocha and P. Viana</subfield>
<subfield code="p">123508</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">62</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">astro-ph/0008446</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. D. Hoyle, U. Schmidt, B. R. Heckel, E. G. Adelberger, J. H. Gundlach, D. J. Kap-ner and H. E. Swanson</subfield>
<subfield code="p">1418</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">86</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-ph/0011014</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. G. Adelberger [EOT-WASH Group Collaboration]</subfield>
<subfield code="r">hep-ex/0202008</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Coleman, Aspects of symmetry. (Cambridge Univ. Press, 1985.)</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-ph/0204143</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Domin, P</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Phenomenological Study of Solar-Neutrino Induced Double Beta Decay of Mo100</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">8 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">The detection of solar-neutrinos of different origin via induced beta beta process of Mo100 is investigated. The particular counting rates and energy distributions of emitted electrons are presented. A discussion in respect tosolar-neutrino detector consisting of 10 tones of Mo100 is included. Both the cases of the standard solar model and neutrino oscillation scenarios are analyzed. Moreover, new beta^- beta^+ and beta^-/EC channels of the double-betaprocess are introduced and possibilities of their experimental observation are addressed.</subfield>
<subfield code="b">8 PAGES LATEX 2 POSTSCRIPT FIGURES TALK PRESENTED BY P DOMIN ON THE WORKSHOP MEDEX'01 (PRAGUE JUNE 2001) TO APPEAR IN CZECH J PHYS 52 (2002)</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[1]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. M. Bilenky, C. Giunti and W. Grimus</subfield>
<subfield code="m">J. N. Bahcall, P. I. Krastev, and A. Yu. Smirnov</subfield>
<subfield code="p">096016</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">58</subfield>
<subfield code="y">1998</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-th/0204101</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="088" ind1="" ind2="">
<subfield code="a">CSULB-PA-02-2</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Nishino, H</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Axisymmetric Gravitational Solutions as Possible Classical Backgrounds around Closed String Mass Distributions</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">15 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">By studying singularities in stationary axisymmetric Kerr and Tomimatsu-Sato solutions with distortion parameter \d = 2, 3, ... in general relativity, we conclude that these singularities can be regarded as nothing other than closedstring-like circular mass distributions. We use two different regularizations to identify \d-function type singularities in the energy-momentum tensor for these solutions, realizing a regulator independent result. This result givessupporting evidence that these axisymmetric exact solutions may well be the classical solutions around closed string-like mass distributions, just like Schwarzschild solution corresponding to a point mass distribution. In otherwords, these axisymmetric exact solutions may well provide the classical backgrounds around closed strings.</subfield>
<subfield code="m">D. Kramer, H. Stephani, E. Herlt and M. MacCallum, `Exact Solutions of Einstein's Field Equations', Cambridge University Press (1980)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Arnowitt, S. Deser and C. Misner, in `Gravitation': `An Introduction to Current Re-search', ed. L. Witten (New York, Wiley, 1962)</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-th/0204102</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Bo-Yu, H</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Soliton on Noncommutative Orbifold $ T^2/Z_k $</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">13 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Following the construction of the projection operators on $ T^2 $ presented by Gopakumar, Headrick and Spradin, we construct the projection operators on the integral noncommutative orbifold $ T^2/G (G=Z_k,k=2, 3, 4, 6)$. Suchoperators are expressed by a function on this orbifold. So it provides a complete set of projection operators upon the moduli space $T^2 \times K/Z_k$. All these operators has the same trace 1/A ($A$ is an integer). Since theprojection operators correspond to solitons in noncommutative string field theory, we obtained the explicit expression of all the soliton solutions on $ T^2/Z_k $.</subfield>
<subfield code="m">G. Landi," An introduction to non-commutative space and their geometry"</subfield>
<subfield code="r">hep-th/9701078</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Varilly, "An introduction to non-commutative Geometry"</subfield>
<subfield code="r">physics/9709045</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Madore, "An introduction to non-commutative Differential Geometry and its physical Applications", Cambridge University press 2nd edition, 1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Connes, M. Douglas, A. Schwartz, Matrix theory compactification on Tori</subfield>
<subfield code="p">003</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">9802</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9711162</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. dougals, C. Hull</subfield>
<subfield code="p">008</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">9802</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9711165</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Nathan. Seiberg and Edward. Witten," String theory and non-commutative geometry"</subfield>
<subfield code="p">032</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">9909</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9908142</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V. Schomerus," D-branes and Deformation Quan-tization"</subfield>
<subfield code="p">030</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">9906</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. Witten, "Noncommutative Geometry and String Field Theory"</subfield>
<subfield code="p">253</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">268</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. B. Laughlin, "The quantum Hall Effect", edited by R. Prange and S. Girvin, p233</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">L. Susskind</subfield>
<subfield code="r">hep-th/0101029</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. P. Hu and S. C. Zhang</subfield>
<subfield code="r">cond-mat/0112432</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Gopakumar, M. Headrick, M. Spradin, "on Noncommutative Multi-solitons"</subfield>
<subfield code="r">hep-th/0103256</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. J. Martinec and G. Moore, "Noncommutative Solitons on Orbifolds"</subfield>
<subfield code="r">hep-th/0101199</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D. J. Gross and N. A. Nekrasov, " Solitons in noncommutative Gauge Theory"</subfield>
<subfield code="r">hep-th/0010090</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. R. Douglas and N. A. Nekrasov, "Noncommutative Field Theory"</subfield>
<subfield code="r">hep-th/0106048</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Gopakumar, S. Minwalla and A. Strominger, " Noncommutative Soliton"</subfield>
<subfield code="p">048</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">005</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/0003160</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Harvey, " Komaba Lectures on Noncommutative Solitons and D-branes</subfield>
<subfield code="r">hep-th/0102076</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. A. Harvey, P. Kraus and F.Larsen, J. High Energy Phys.0012 (200) 024</subfield>
<subfield code="r">hep-th/0010060</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Konechny and A. Schwarz, "Compactification of M(atrix) theory on noncommutative toroidal orbifolds"</subfield>
<subfield code="p">667</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">591</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9912185</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">" Moduli spaces of max-imally supersymmetric solutions on noncommutative tori and noncommutative orbifolds", J. High Energy Phys.0009, (2000) 005</subfield>
<subfield code="r">hep-th/0005167</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Walters, "Projective modules over noncommutative sphere", J. London Math. Soc. : 51 (1995) 589"Chern characters of Fourier modules", Can. J. Math. : 52 (2000) 633</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Rieffel, Pacific J. Math. : 93 (1981) 415</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. P. Boca</subfield>
<subfield code="p">325</subfield>
<subfield code="t">Commun. Math. Phys.</subfield>
<subfield code="v">202</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">H. Bacry, A. Grossman and J. Zak</subfield>
<subfield code="p">1118</subfield>
<subfield code="t">Phys. Rev., B</subfield>
<subfield code="v">12</subfield>
<subfield code="y">1975</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Zak, In Solid State Phys.edited by H. Ehrenreich, F. Seitz and D. Turnbull (Aca-demic,new York,1972), Vol. 27</subfield>
<subfield code="a">We review the status of hybrid baryons. The only known way to study hybrids rigorously is via excited adiabatic potentials. Hybrids can be modelled by both the bag and flux-tube models. The low-lying hybrid baryon is N 1/2^+ with amass of 1.5-1.8 GeV. Hybrid baryons can be produced in the glue-rich processes of diffractive gamma N and pi N production, Psi decays and p pbar annihilation.</subfield>
</datafield>
<datafield tag="595" ind1="" ind2="">
<subfield code="a">LANL EDS</subfield>
</datafield>
<datafield tag="650" ind1="1" ind2="7">
<subfield code="2">SzGeCERN</subfield>
<subfield code="a">Nuclear Physics</subfield>
</datafield>
<datafield tag="856" ind1="0" ind2="">
<subfield code="f">"Philip R. page" <prp@t16prp.lanl.gov></subfield>
<subfield code="b">INVITED PLENARY TALK PRESENTED AT THE ``9TH INTERNATIONAL CONFERENCE ON THE STRUCTURE OF BARYONS'' (BARYONS 2002) 3-8 MARCH NEWPORT NEWS VA USA 12 PAGES 7 ENCAPSULATED POSTSCRIPT FIGURES LATEX</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="S">
<subfield code="s">n</subfield>
<subfield code="w">200216</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">PREPRINT</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">nucl-th/0204032</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Amos, K</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">A simple functional form for proton-nucleus total reaction cross sections</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">13 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">A simple functional form has been found that gives a good representation of the total reaction cross sections for the scattering of protons from (15) nuclei spanning the mass range ${}^{9}$Be to ${}^{238}$U and for proton energiesranging from 20 to 300 MeV.</subfield>
<subfield code="a">Saturation of nuclear matter and radii of unstable nuclei</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="300" ind1="" ind2="">
<subfield code="a">26 p</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We examine relations among the parameters characterizing the phenomenological equation of state (EOS) of nearly symmetric, uniform nuclear matter near the saturation density by comparing macroscopic calculations of radii and massesof stable nuclei with the experimental data. The EOS parameters of interest here are the symmetry energy S_0, the symmetry energy density-derivative coefficient L and the incompressibility K_0 at the normal nuclear density. We find aconstraint on the relation between K_0 and L from the empirically allowed values of the slope of the saturation line (the line joining the saturation points of nuclear matter at finite neutron excess), together with a strongcorrelation between S_0 and L. In the light of the uncertainties in the values of K_0 and L, we macroscopically calculate radii of unstable nuclei as expected to be produced in future facilities. We find that the matter radii dependstrongly on L while being almost independent of K_0, a feature that will help to determine the L value via systematic measurements of nuclear size.</subfield>
<subfield code="m">C. Fuchs, A. Faessler, E. Zabrodin, Y.M. Zheng</subfield>
<subfield code="p">1974</subfield>
<subfield code="t">Phys. Rev. Lett.</subfield>
<subfield code="v">86</subfield>
<subfield code="y">2001</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Danielewicz, in: Proc. Int. Symp. on Non-Equilibrium and Nonlinear Dynamics in Nuclear and Other Finite Systems, Beijing, 2001</subfield>
<subfield code="m">K. Iida, K. Oyamatsu, unpublished</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J.P. Blaizot, J.F. Berger, J. Decharg´e, M. Girod</subfield>
<subfield code="p">435</subfield>
<subfield code="t">Nucl. Phys., A</subfield>
<subfield code="v">591</subfield>
<subfield code="y">1995</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">nucl-th/0204034</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Bozek, P</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Nuclear matter with off-shell propagation</subfield>
</datafield>
<datafield tag="260" ind1="" ind2="">
<subfield code="c">12 Apr 2002</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Symmetric nuclear matter is studied within the conserving, self-consistent T-matrix approximation. This approach involves off-shell propagation of nucleons in the ladder diagrams. The binding energy receives contributions from thebackground part of the spectral function, away form the quasiparticle peak. The Fermi energy at the saturation point fulfills the Hugenholz-Van Hove relation. In comparison to the Brueckner-Hartree-Fock approach, the binding energyis reduced and the equation of state is harder</subfield>
<subfield code="a">We consider the N=4 SU(N) Super Yang Mills theory on the Coulomb branch with gauge symmetry broken to S(U(N_1)*U(N_2)). By integrating the W particles, the effective action near the IR SU(N_i) conformal fixed points is seen to be adeformation of the Super Yang Mills theory by a non-renormalized, irrelevant, dimension 8 operator. The correction to the two-point function of the dilaton field dual operator near the IR is related to a three-point function ofchiral primary operators at the conformal fixed points and agrees with the classical gravity prediction, including the numerical factor.</subfield>
<subfield code="m">O. Aharony, S.S. Gubser, J. Maldacena, H. Ooguri and Y. Oz, Large N Field Theories, String Theory and Gravity</subfield>
<subfield code="p">183</subfield>
<subfield code="t">Phys. Rep.</subfield>
<subfield code="v">323</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9905111</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[5]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J.A. Minahan and N.P. Warner, Quark Potentials in the Higgs Phase of Large N Supersymmetric Yang-Mills Theories</subfield>
<subfield code="p">005</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">06</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9805104</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[6]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.R. Douglas and W. Taylor, Branes in the bulk of Anti-de Sitter space</subfield>
<subfield code="r">hep-th/9807225</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[7]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.A. Tseytlin and S. Yankielowicz, Free energy of N=4 super Yang-Mills in Higgs phase and non-extremal D3-brane interactions</subfield>
<subfield code="p">145</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">541</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9809032</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[8]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y. Wu, A Note on AdS/SYM Correspondence on the Coulomb Branch</subfield>
<subfield code="r">hep-th/9809055</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[9]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P. Kraus, F. Larsen, S. Trivedi, The Coulomb Branch of Gauge Theory from Rotating Branes</subfield>
<subfield code="p">003</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">03</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9811120</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[10]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I.R. Klebanov and E. Witten, AdS/CFT Correspondence and Symmetry Breaking</subfield>
<subfield code="p">89</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">556</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9905104</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">D.Z. Freedman, S.S. Gubser, K. Pilch and N.P. Warner, Continuous distributions of D3-branes and gauged supergravity</subfield>
<subfield code="r">hep-th/9906194</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Brandhuber and K. Sfetsos, Wilson loops from multicentre and rotating branes, mass gaps and phase structure in gauge theories</subfield>
<subfield code="r">hep-th/9906201</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. Chepelev and R. Roiban, A note on correlation functions in AdS5/SY M4 corre-spondence on the Coulomb branch</subfield>
<subfield code="p">74</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">462</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9906224</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.B. Giddings and S.F. Ross, D3-brane shells to black branes on the Coulomb branch</subfield>
<subfield code="p">024036</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">61</subfield>
<subfield code="y">2000</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9907204</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Cvetic, S.S. Gubser, H. Lu and C.N. Pope, Symmetric Potentials of Gauged Su-pergravities in Diverse Dimensions and Coulomb Branch of Gauge Theories</subfield>
<subfield code="r">hep-th/9909121</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R.C.Rashkov and K.S.Viswanathan, Correlation functions in the Coulomb branch of N=4 SYM from AdS/CFT correspondence</subfield>
<subfield code="r">hep-th/9911160</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.S. Costa, Absorption by Double-Centered D3-Branes and the Coulomb Branch of N = 4 SYM Theory</subfield>
<subfield code="r">hep-th/9912073</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[18]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Y.S. Myung, G. Kang and H.W. Lee, Greybody factor for D3-branes in B field</subfield>
<subfield code="r">hep-th/9911193</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S-wave absorption of scalars by noncommutative D3-branes</subfield>
<subfield code="r">hep-th/9912288</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[19]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. Manvelyan, H.J.W. Mueller-Kirsten, J.-Q. Liang, Y. Zhang, Absorption Cross Sec-tion of Scalar Field in Supergravity Background</subfield>
<subfield code="r">hep-th/0001179</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[20]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.S. Gubser and I.R. Klebanov, Absorption by Branes and Schwinger Terms in the World Volume Theory</subfield>
<subfield code="p">41</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">413</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9708005</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[21]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Intriligator, Maximally Supersymmetric RG Flows and AdS Duality</subfield>
<subfield code="r">hep-th/9909082</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[22]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.S. Gubser, A. Hashimoto, I.R. Klebanov and M. Krasnitz, Scalar Absorption and the Breaking of the World Volume Conformal Invariance</subfield>
<subfield code="p">393</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">526</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9803023</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[23]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S. Lee, S. Minwalla, M. Rangamani and N. Seiberg, Three-Point Functions of Chiral Operators in D=4, N = 4 SYM at Large N</subfield>
<subfield code="m">E. D'Hoker, D.Z. Freedman and W. Skiba, Field Theory Tests for Correlators in the AdS/CFT Correspondence</subfield>
<subfield code="p">045008</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">59</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9807098</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[25]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">F. Gonzalez-Rey, B. Kulik and I.Y. Park, Non-renormalization of two and three Point Correlators of N=4 SYM in N=1 Superspace</subfield>
<subfield code="p">164</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">455</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9903094</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[26]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Intriligator, Bonus Symmetries of N=4 Super-Yang-Mills Correlation Functions via AdS Duality</subfield>
<subfield code="p">575</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">551</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9811047</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">K. Intriligator and W. Skiba, Bonus Symmetry and the Operator Product Expansion of N=4 Super-Yang-Mills</subfield>
<subfield code="p">165</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">559</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9905020</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[27]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Eden, P.S. Howe and P.C. West, Nilpotent invariants in N=4 SYM</subfield>
<subfield code="p">19</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">463</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9905085</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">P.S. Howe, C. Schubert, E. Sokatchev and P.C. West, Explicit construction of nilpotent covariants in N=4 SYM</subfield>
<subfield code="r">hep-th/9910011</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[28]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Petkou and K. Skenderis, A non-renormalization theorem for conformal anomalies</subfield>
<subfield code="p">100</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">561</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9906030</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[29]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.R. Douglas, D. Kabat, P. Pouliot and S.H. Shenker, D-branes and Short Distances in String Theory</subfield>
<subfield code="p">85</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">485</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9608024</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[30]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">G. Lifschytz and S.D. Mathur, Supersymmetry and Membrane Interactions in M(atrix) Theory</subfield>
<subfield code="p">621</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">507</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9612087</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[31]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">J. Maldacena, Probing Near Extremal Black Holes with D-branes</subfield>
<subfield code="p">3736</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">57</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9705053</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Branes probing black holes</subfield>
<subfield code="p">17</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">68</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9709099</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[32]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">I. Chepelev and A.A. Tseytlin, Interactions of type IIB D-branes from D-instanton ma-trix model</subfield>
<subfield code="p">629</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">511</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9705120</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">Long-distance interactions of branes: correspondence between supergravity and super Yang-Mills descriptions</subfield>
<subfield code="p">73</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">515</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9709087</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.A. Tseytlin, Interactions Between Branes and Matrix Theories</subfield>
<subfield code="p">99</subfield>
<subfield code="t">Nucl. Phys. B, Proc. Suppl.</subfield>
<subfield code="v">68</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9709123</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[33]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M. Dine and N. Seiberg, Comments on Higher Derivative Operators in Some SUSY Field Theories</subfield>
<subfield code="p">239</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">409</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9705057</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[34]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A.A. Tseytlin, On non-abelian generalisation of Born-Infeld action in string theory</subfield>
<subfield code="p">41</subfield>
<subfield code="t">Nucl. Phys., B</subfield>
<subfield code="v">501</subfield>
<subfield code="y">1997</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9701125</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[35]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.S. Gubser and A. Hashimoto, Exact absorption probabilities for the D3-brane, Com-mun. Math. Phys. : 203 (1999) 325</subfield>
<subfield code="r">hep-th/9805140</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[36]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">S.S. Gubser, Non-conformal examples of AdS/CFT</subfield>
<subfield code="a">AdS/CFT For Non-Boundary Manifolds</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">In its Euclidean formulation, the AdS/CFT correspondence begins as a study of Yang-Mills conformal field theories on the sphere, S^4. It has been successfully extended, however, to S^1 X S^3 and to the torus T^4. It is natural tohope that it can be made to work for any manifold on which it is possible to define a stable Yang-Mills conformal field theory. We consider a possible classification of such manifolds, and show how to deal with the most obviousobjection : the existence of manifolds which cannot be represented as boundaries. We confirm Witten's suggestion that this can be done with the help of a brane in the bulk.</subfield>
<subfield code="a">We construct explicit form of the anomalous effective action, in arbitrary even dimension, for Abelian vector and axial gauge fields coupled to Dirac fermions. It turns out to be a surprisingly simple extension of 2D Schwinger modeleffective action.</subfield>
<subfield code="m">S.E.Treiman, R. Jackiw, D.J.Gross " Lectures on Current Algebra and its Applications ", Princeton UP, Princeton NJ, (1972)</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">T.Berger " Fermions in two (1+1)-dimensional anomalous gauge theories: the chiral Schwinger model and the chiral quantum gravity " Hamburg U</subfield>
<subfield code="m">R.Jackiw " Topological Investigations of Quantized Gauge Theories " in Relativity, Groups and Topology eds. B.deWitt and R.Stora (Elsevier, Amsterdam 1984)</subfield>
<subfield code="a">Restrictions on Gauge Groups in Noncommutative Gauge Theory</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">We show that the gauge groups SU(N), SO(N) and Sp(N) cannot be realized on a flat noncommutative manifold, while it is possible for U(N).</subfield>
<subfield code="m">J.Polchinski, TASI Lectures on D-branes</subfield>
<subfield code="r">hep-th/9611050</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[2]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">M.R.Douglas and C.Hull, D-branes and the Noncommuta-tive torus</subfield>
<subfield code="p">8</subfield>
<subfield code="t">J. High Energy Phys.</subfield>
<subfield code="v">2</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="r">hep-th/9711165</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[3]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">V.Schomerus, D-branes and Deformation Quantization</subfield>
<subfield code="r">hep-th/9903205</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[4]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">N.Seiberg and E.Witten, String Theory and Noncommu-tative Geometry</subfield>
<subfield code="r">hep-th/9908142</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">2</subfield>
</datafield>
</record>
<record>
<datafield tag="037" ind1="" ind2="">
<subfield code="a">hep-th/0003295</subfield>
</datafield>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">eng</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Wang, B</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Quasinormal modes of Reissner-Nordstrom Anti-de Sitter Black Holes</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">Complex frequencies associated with quasinormal modes for large Reissner-Nordstr$\ddot{o}$m Anti-de Sitter black holes have been computed. These frequencies have close relation to the black hole charge and do not linearly scale withthe black hole temperature as in Schwarzschild Anti-de Sitter case. In terms of AdS/CFT correspondence, we found that the bigger the black hole charge is, the quicker for the approach to thermal equilibrium in the CFT. The propertiesof quasinormal modes for $l>0$ have also been studied.</subfield>
<subfield code="m">S. S. Gubser, I. R. Klebanov and A. M. Polyakov</subfield>
<subfield code="p">105</subfield>
<subfield code="t">Phys. Lett., B</subfield>
<subfield code="v">428</subfield>
<subfield code="y">1998</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[11]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Chamblin, R. Emparan, C. V. Johnson and R. C. Myers</subfield>
<subfield code="p">064018</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">60</subfield>
<subfield code="y">1999</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[12]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. W. Leaver</subfield>
<subfield code="p">1238</subfield>
<subfield code="t">J. Math. Phys.</subfield>
<subfield code="v">27</subfield>
<subfield code="y">1986</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[13]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">E. W. Leaver</subfield>
<subfield code="p">2986</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">41</subfield>
<subfield code="y">1990</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[14]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">C. O. Lousto</subfield>
<subfield code="p">1733</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">51</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[15]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">O. Kaburaki</subfield>
<subfield code="p">316</subfield>
<subfield code="t">Phys. Lett., A</subfield>
<subfield code="v">217</subfield>
<subfield code="y">1996</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[16]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">R. K. Su, R. G. Cai and P. K. N. Yu</subfield>
<subfield code="p">2932</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">50</subfield>
<subfield code="y">1994</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">3473</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">48</subfield>
<subfield code="y">1993</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="p">6186</subfield>
<subfield code="t">Phys. Rev., D</subfield>
<subfield code="v">52</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">B. Wang, J. M. Zhu</subfield>
<subfield code="p">1269</subfield>
<subfield code="t">Mod. Phys. Lett., A</subfield>
<subfield code="v">10</subfield>
<subfield code="y">1995</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="o">[17]</subfield>
</datafield>
<datafield tag="999" ind1="C" ind2="5">
<subfield code="m">A. Chamblin, R. Emparan, C. V. Johnson and R. C. Myers, Phys. Rev., D60: 104026 (1999) 5070 90 110 130 150 r+ 130 230 330 50 70 90 110 130 150 r+</subfield>
</datafield>
</record>
<record>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">rus</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Пушкин, А С</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Медный всадник</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">
На берегу пустынных волн,<br>
Стоял он, дум великих полн,<br>
И вдаль глядел. Пред ним широко<br>
Река неслася; бедный чёлн<br>
По ней стремился одиноко.<br>
По мшистым, топким берегам<br>
Чернели избы здесь и там,<br>
Приют убогого чухонца;<br>
И лес, неведомый лучам<br>
В тумане спрятанного солнца,<br>
Кругом шумел.<br>
</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="0">
<subfield code="y">1833</subfield>
</datafield>
<datafield tag="909" ind1="C" ind2="1">
<subfield code="c">1990-01-27</subfield>
<subfield code="l">00</subfield>
<subfield code="m">2002-04-12</subfield>
<subfield code="o">BATCH</subfield>
</datafield>
<datafield tag="980" ind1="" ind2="">
<subfield code="a">POETRY</subfield>
</datafield>
</record>
<record>
<datafield tag="041" ind1="" ind2="">
<subfield code="a">gre</subfield>
</datafield>
<datafield tag="100" ind1="" ind2="">
<subfield code="a">Καβάφης, Κ Π</subfield>
</datafield>
<datafield tag="245" ind1="" ind2="">
<subfield code="a">Ιθάκη</subfield>
</datafield>
<datafield tag="520" ind1="" ind2="">
<subfield code="a">
Σα βγεις στον πηγαιμό για την Ιθάκη,<br>
να εύχεσαι νάναι μακρύς ο δρόμος,<br>
γεμάτος περιπέτειες, γεμάτος γνώσεις.<br>
Τους Λαιστρυγόνας και τους Κύκλωπας,<br>
τον θυμωμένο Ποσειδώνα μη φοβάσαι,<br>
τέτοια στον δρόμο σου ποτέ σου δεν θα βρείς,<br>
αν μέν' η σκέψις σου υψηλή, αν εκλεκτή<br>
συγκίνησις το πνεύμα και το σώμα σου αγγίζει.<br>
Τους Λαιστρυγόνας και τους Κύκλωπας,<br>
τον άγριο Ποσειδώνα δεν θα συναντήσεις,<br>
αν δεν τους κουβανείς μες στην ψυχή σου,<br>
αν η ψυχή σου δεν τους στήνει εμπρός σου.<br>
<br>
Να εύχεσαι νάναι μακρύς ο δρόμος.<br>
Πολλά τα καλοκαιρινά πρωϊά να είναι<br>
που με τι ευχαρίστησι, με τι χαρά<br>
θα μπαίνεις σε λιμένας πρωτοειδωμένους·<br>
να σταματήσεις σ' εμπορεία Φοινικικά,<br>
και τες καλές πραγμάτειες ν' αποκτήσεις,<br>
σεντέφια και κοράλλια, κεχριμπάρια κ' έβενους,<br>
και ηδονικά μυρωδικά κάθε λογής,<br>
όσο μπορείς πιο άφθονα ηδονικά μυρωδικά·<br>
σε πόλεις Αιγυπτιακές πολλές να πας,<br>
να μάθεις και να μάθεις απ' τους σπουδασμένους.<br>
<br>
Πάντα στον νου σου νάχεις την Ιθάκη.<br>
Το φθάσιμον εκεί είν' ο προορισμός σου.<br>
Αλλά μη βιάζεις το ταξίδι διόλου.<br>
Καλλίτερα χρόνια πολλά να διαρκέσει·<br>
και γέρος πια ν' αράξεις στο νησί,<br>
πλούσιος με όσα κέρδισες στον δρόμο,<br>
μη προσδοκώντας πλούτη να σε δώσει η Ιθάκη.<br>
<br>
Η Ιθάκη σ' έδωσε το ωραίο ταξίδι.<br>
Χωρίς αυτήν δεν θάβγαινες στον δρόμο.<br>
Αλλο δεν έχει να σε δώσει πια.<br>
<br>
Κι αν πτωχική την βρεις, η Ιθάκη δεν σε γέλασε.<br>