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      Charged AdS Black Holes and Catastrophic Holography

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          Abstract

          We compute the properties of a class of charged black holes in anti-de 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 Waals-Maxwell 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.

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          Black holes in higher dimensional space-times

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            Particle emission rates from a black hole. II. Massless particles from a rotating hole

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              Author and article information

              Journal
              23 February 1999
              1999-03-09
              Article
              10.1103/PhysRevD.60.064018
              hep-th/9902170
              b61299d9-3e97-49f3-89a4-ad605f90c522
              History
              Custom metadata
              DAMTP-1999-29, EHU-FT/9902, DTP-99/9, UK/99-02, McGill/99-07
              Phys.Rev. D60 (1999) 064018
              19 pages, revtex, psfig, 6 multicomponent figures, typos, references and a few remarks have been repaired, and added
              hep-th

              High energy & Particle physics
              High energy & Particle physics

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