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   <dc:title>Microstates of a neutral black hole in M theory</dc:title>
   <dc:creator>Emparan García de Salazar, Roberto A.</dc:creator>
   <dc:creator>Horowitz, Gary T.</dc:creator>
   <dc:subject>Teoria de camps (Física)</dc:subject>
   <dc:subject>Relativitat general (Física)</dc:subject>
   <dc:subject>Models de corda</dc:subject>
   <dc:subject>General theory of fields and particles</dc:subject>
   <dc:subject>General relativity and gravitation</dc:subject>
   <dc:subject>String models</dc:subject>
   <dcterms:abstract>We consider vacuum solutions in M theory of the form of a five-dimensional Kaluza-Klein black hole cross T6. In a certain limit, these include the five-dimensional neutral rotating black hole (cross T6). From a type-IIA standpoint, these solutions carry D0 and D6 charges. We show that there is a simple D-brane description which precisely reproduces the Hawking-Bekenstein entropy in the extremal limit, even though supersymmetry is completely broken.</dcterms:abstract>
   <dcterms:issued>2010-07-05T10:10:16Z</dcterms:issued>
   <dcterms:issued>2010-07-05T10:10:16Z</dcterms:issued>
   <dcterms:issued>2006</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 proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevLett.97.141601</dc:relation>
   <dc:relation>Physical Review Letters, 2006, vol. 97, núm. 14, p. 141601-1-141601-4</dc:relation>
   <dc:relation>http://dx.doi.org/10.1103/PhysRevLett.97.141601</dc:relation>
   <dc:rights>(c) American Physical Society, 2006</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:publisher>American Physical Society</dc:publisher>
   <dc:source>Articles publicats en revistes (Física de la Matèria Condensada)</dc:source>
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