<small><strong>Abstract: </strong>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.</small><br/>
<br/><br/><strong>Published in: </strong><a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.%20Lett.%2C%20B&volume=481&year=2000&page=79">Phys. Lett., B :481 2000 79-88</a>
<br/><br/><strong>Cited by:</strong> try citation search for <a href="http://pcdh23.cern.ch/search?f=reference&p=hep-th/0003295">hep-th/0003295</a>
</p>
<blockquote><strong>References:</strong><ul><li><small>[1]</small> <small>K. D. Kokkotas, B. G. Schmidt</small> <small> [<a href="http://pcdh23.cern.ch/search?f=reportnumber&p=gr-qc/9909058">gr-qc/9909058</a>] </small> <br/><small>and references therein</small> <li><small>[2]</small> <small>W. Krivan</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=60&year=1999&page=101501">Phys. Rev., D: 60 (1999) 101501</a> </small> <br/><li><small>[3]</small> <small>S. Hod</small> <small> [<a href="http://pcdh23.cern.ch/search?f=reportnumber&p=gr-qc/9902072">gr-qc/9902072</a>] </small> <br/><li><small>[4]</small> <small>P. R. Brady, C. M. Chambers, W. G. Laarakkers and E. Poisson</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=60&year=1999&page=064003">Phys. Rev., D: 60 (1999) 064003</a> </small> <br/><li><small>[5]</small> <small>P. R. Brady, C. M. Chambers, W. Krivan and P. Laguna</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=55&year=1997&page=7538">Phys. Rev., D: 55 (1997) 7538</a> </small> <br/><li><small>[6]</small> <small>G. T. Horowitz and V. E. Hubeny</small> <small> [<a href="http://pcdh23.cern.ch/search?f=reportnumber&p=hep-th/9909056">hep-th/9909056</a>] </small> <br/><small>G. T. Horowitz</small> <small> [<a href="http://pcdh23.cern.ch/search?f=reportnumber&p=hep-th/9910082">hep-th/9910082</a>] </small> <br/><li><small>[7]</small> <small>E. S. C. Ching, P. T. Leung, W. M. Suen and K. Young</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=52&year=1995&page=2118">Phys. Rev., D: 52 (1995) 2118</a> </small> <br/><li><small>[8]</small> <small>J. M. Maldacena</small> <small> Adv. Theor. Math. Phys.21998231 </small> <br/><li><small>[9]</small> <small>E. Witten</small> <small> Adv. Theor. Math. Phys.21998253 </small> <br/><li><small>[10]</small> <small>S. S. Gubser, I. R. Klebanov and A. M. Polyakov</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Lett.,+B&volume=428&year=1998&page=105">Phys. Lett., B: 428 (1998) 105</a> </small> <br/><li><small>[11]</small> <small>A. Chamblin, R. Emparan, C. V. Johnson and R. C. Myers</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=60&year=1999&page=064018">Phys. Rev., D: 60 (1999) 064018</a> </small> <br/><li><small>[12]</small> <small>E. W. Leaver</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=J.+Math.+Phys.&volume=27&year=1986&page=1238">J. Math. Phys.: 27 (1986) 1238</a> </small> <br/><li><small>[13]</small> <small>E. W. Leaver</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=41&year=1990&page=2986">Phys. Rev., D: 41 (1990) 2986</a> </small> <br/><li><small>[14]</small> <small>C. O. Lousto</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=51&year=1995&page=1733">Phys. Rev., D: 51 (1995) 1733</a> </small> <br/><li><small>[15]</small> <small>O. Kaburaki</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Lett.,+A&volume=217&year=1996&page=316">Phys. Lett., A: 217 (1996) 316</a> </small> <br/><li><small>[16]</small> <small>R. K. Su, R. G. Cai and P. K. N. Yu</small> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=50&year=1994&page=2932">Phys. Rev., D: 50 (1994) 2932</a> </small> <br/> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=48&year=1993&page=3473">Phys. Rev., D: 48 (1993) 3473</a> </small> <br/> <small> <a href="http://weblib.cern.ch/cgi-bin/ejournals?publication=Phys.+Rev.,+D&volume=52&year=1995&page=6186">Phys. Rev., D: 52 (1995) 6186</a> </small> <br/><small>B. Wang, J. M. Zhu</small> <small> Mod. Phys. Lett., A1019951269 </small> <br/><li><small>[17]</small> <small>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+</small> </ul><p><small><i><b>Warning</b>: references are automatically extracted and standardized from the PDF document and may therefore contain errors. If you think they are incorrect or incomplete, look at the fulltext document itself.<br></i></small></blockquote>
Caption</td></tr></table> <small>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.</small></p><p><table><tr><td class="blocknote">
Légende</td></tr></table><small>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.</small></p>
<p><table><tr><td class="blocknote">See also:</td></tr></table><small><a href="http://www.cern.ch/CERN/Announcements/1998/WebNext.html">"Internet, Web, What's next?" 26 June 1998</a><br/><a href="http://Bulletin.cern.ch/9828/art2/Text_E.html">CERN Bulletin no 28/98 (6 July 1998) (English)</a><br/><a href="http://Bulletin.cern.ch/9828/art2/Text_F.html">CERN Bulletin no 28/98 (6 juillet 1998) (French)</a><br/><a href="http://www.w3.org/People/Berners-Lee/">Biography</a></small></p>
<article><front><journal-meta><journal-title>J. High Energy Phys.</journal-title><abbrev-journal-title>J. High Energy Phys.</abbrev-journal-title><issn>1126-6708</issn></journal-meta><article-meta><title-group><article-title>AdS/CFT For Non-Boundary Manifolds</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>McInnes</surname><given-names>B</given-names></name></contrib></contrib-group><pub-date pub-type="pub"><year>2000</year></pub-date><volume>05</volume><fpage></fpage><lpage></lpage><self-uri xlink:href="http://pcdh23.cern.ch/record/70" xmlns:xlink="http://www.w3.org/1999/xlink/"/><self-uri xlink:href="http://documents.cern.ch/cgi-bin/setlink?base=preprint&categ=hep-th&id=0003291" xmlns:xlink="http://www.w3.org/1999/xlink/" /></article-meta><abstract>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.</abstract></front><article-type>research-article</article-type><ref></ref></article>
</articles>'''
deftest_nlm_output(self):
"""bibformat - NLM output"""
pageurl=weburl+'/record/70?of=xn'
result=test_web_page_content(pageurl,
expected_text=self.record_70_xn)
self.assertEqual([],result)
classBibFormatBriefHTMLTest(unittest.TestCase):
"""Check output produced by BibFormat for brief HTML ouput for