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Charged AdS black holes and catastrophic holography
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Allowing for the cosmological constant to be a dynamical pressure gives the thermodynamics of anti-de Sitter black holes a richer structure than their asymptotically flat counterparts; behaving as Van der Waals fluids, polymers, and allowing for the construction of black hole heat engines.
“Glossing over the details, allowing for the cosmological constant to be a dynamical pressure has the thermodynamics of anti-de Sitter black holes, in particular, acquire a richer structure than their asymptotically flat counterparts; behaving as Van der Waals fluids [145,146], polymers [147], and allowing for the construction of black hole heat engines [148].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [145]
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Emparan, R., Johnson, C. V., & Myers, R. C. (1999) · Physical Review D · doi:10.1103/physrevd.60.104001 · Cited by 703
Self-citationThe statistical mechanics of near-extremal black holes
Iliesiu, L. V., & Turiaci, G. J. (2021) · Journal of High Energy Physics · doi:10.1007/jhep05(2021)145 · Cited by 190
Quasinormal modes of Reissner-Nordström Anti-de Sitter black holes
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Conserved charges in general relativity
Aoki, S., Onogi, T., & Yokoyama, S. (2021) · International Journal of Modern Physics A · doi:10.1142/s0217751x21500986 · Cited by 34
Three-Dimensional Quantum Black Holes: A Primer
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Metadata
- Authors
- Chamblin, A., Emparan, R., Johnson, C. V., & Myers, R. C.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1999-08-24
- Volume
- 60
- Issue
- 6
- ISSN
- 0556-2821
- 1089-4918
- Cited by
- 1,016
- References
- 6
- Language
- en
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