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Charged AdS black holes and catastrophic holography

Andrew ChamblinRoberto EmparanClifford V. JohnsonRobert C. Myers

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.

Black Holes and Theoretical PhysicsCosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesPhysicsCritical phenomenaPhase spaceTheoretical physicsBlack hole thermodynamicsClassical mechanicsSpace (punctuation)Field (mathematics)Black hole (networking)Einstein

Funding

  • National Science Foundation
  • University of Kentucky
  • McGill University
  • Natural Sciences and Engineering Research Council of Canada
  • Engineering and Physical Sciences Research Council
  • Pembroke College, University of Cambridge
Citations
1,356
FWCI
22.35
field-weighted impact
References
51
Percentile
99%
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Black holes in higher dimensional space-times
Annals of Physics · 1986 · 2,042 citations
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Communications in Mathematical Physics · 1983 · 2,881 citations
The world as a hologram
Journal of Mathematical Physics · 1995 · 3,768 citations
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