Charged AdS black holes and catastrophic holography

We compute the properties of a class of charged black holes in antide Sitter space-time, in diverse dimensions. These black holes are solutions of consistent Einstein-Maxwell truncations of gauged supergravities, which are shown to arise from the inclusion of rotation in the transverse space. We unc...

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Detalles Bibliográficos
Autores: Chamblin, A., Emparan García de Salazar, Roberto A., Johnson, Clifford V. (Clifford Victor), 1968-, Myers, Robert Charles
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:1999
País:España
Institución:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repositorio:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/12366
Acceso en línea:https://hdl.handle.net/2445/12366
Access Level:acceso abierto
Palabra clave:Relativitat general (Física)
Teoria quàntica de camps
Forats negres (Astronomia)
Supergravetat
Partícules (Física nuclear)
General relativity (Physics)
Quantum field theory
Black holes (Astronomy)
Supergravity
Particles (Nuclear physics)
Descripción
Sumario:We compute the properties of a class of charged black holes in antide Sitter space-time, in diverse dimensions. These black holes are solutions of consistent Einstein-Maxwell truncations of gauged supergravities, which are shown to arise from the inclusion of rotation in the transverse space. We uncover rich thermodynamic phase structures for these systems, which display classic critical phenomena, including structures isomorphic to the van der WaalsMaxwell liquid-gas system. In that case, the phases are controlled by the universal cusp and swallowtail shapes familiar from catastrophe theory. All of the thermodynamics is consistent with field theory interpretations via holography, where the dual field theories can sometimes be found on the world volumes of coincident rotating branes.