self.record_74_hd_title='''<center><big><big><strong>Quasinormal modes of Reissner-Nordstrom Anti-de Sitter Black Holes</strong></big></big></center>'''
self.record_74_hd_abstract='''<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 />'''
self.record_74_hd_pubinfo='''<strong>Published in: </strong><a href="https://cds.cern.ch/ejournals.py?publication=Phys.%20Lett.%2C%20B&volume=481&year=2000&page=79">Phys. Lett., B :481 2000 79-88</a>'''
self.record_74_hd_citations='''<strong>Cited by:</strong> try citation search for <a href="%(siteurl)s/search?f=reference&p=hep-th/0003295&ln=%(lang)s">hep-th/0003295</a>'''% \
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self.record_74_hd_references='''<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> </li>'''
Caption</span><br /> <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><span class="blocknote">
Légende</span><br /><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>'''
<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>