<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-17T07:32:23Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/12368" metadataPrefix="qdc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/12368</identifier><datestamp>2025-12-04T20:47:03Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478822</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>Holography, thermodynamics and fluctuations of charged AdS black holes</dc:title>
   <dc:creator>Chamblin, A.</dc:creator>
   <dc:creator>Emparan García de Salazar, Roberto A.</dc:creator>
   <dc:creator>Johnson, Clifford V. (Clifford Victor), 1968-</dc:creator>
   <dc:creator>Myers, Robert Charles</dc:creator>
   <dc:subject>Relativitat general (Física)</dc:subject>
   <dc:subject>Supergravetat</dc:subject>
   <dc:subject>Forats negres (Astronomia)</dc:subject>
   <dc:subject>General relativity (Physics)</dc:subject>
   <dc:subject>Supergravity</dc:subject>
   <dc:subject>Black holes (Astronomy)</dc:subject>
   <dcterms:abstract>rg model with A3 potential. The holographically dual field theories provide the description of the microscopic degrees of freedom which underlie all of the thermodynamics, as can be seen by examining the form of the microscopic fluctuations.</dcterms:abstract>
   <dcterms:issued>2010-05-06T09:25:16Z</dcterms:issued>
   <dcterms:issued>2010-05-06T09:25:16Z</dcterms:issued>
   <dcterms:issued>1999</dcterms:issued>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:relation>Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.60.104026</dc:relation>
   <dc:relation>Physical Review D, 1999, vol. 60, núm. 10, p. 104026-1-104026-20</dc:relation>
   <dc:relation>http://dx.doi.org/10.1103/PhysRevD.60.104026</dc:relation>
   <dc:rights>(c) The American Physical Society, 1999</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:publisher>The American Physical Society</dc:publisher>
   <dc:source>Articles publicats en revistes (Física de la Matèria Condensada)</dc:source>
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