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Thermal dynamic phase transition of Reissner-Nordström Anti-de Sitter black holes on free energy landscape
Abstract
A bstract: We explore the thermodynamics and the underlying kinetics of the van der Waals type phase transition of Reissner-Nordström anti-de Sitter (RNAdS) black holes based on the free energy landscape. We show that the thermodynamic stabilities of the three branches of the RNAdS black holes are determined by the underlying free energy landscape topography. We suggest that the large (small) RNAdS black hole can have the probability to switch to the small (large) black hole due to the thermal fluctuation. Such a state switching process under the thermal fluctuation is taken as a stochastic process and the associated kinetics can be described by the probabilistic Fokker-Planck equation. We obtained the time dependent solutions for the probabilistic evolution by numerically solving Fokker-Planck equation with the reflecting boundary conditions. We also investigated the first passage process which describes how fast a system undergoes a stochastic process for the first time. The distributions of the first passage time switching from small (large) to large (small) black hole and the corresponding mean first passage time as well as its fluctuations at different temperatures are studied in detail. We conclude that the mean first passage time and its fluctuations are related to the free energy landscape topography through barrier heights and temperatures.
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When the transition is spatially homogeneous, the dynamics of the RNAdS black hole phase transition has been studied based on the underlying free energy landscape.
“When the transition is spatial homogeneous, the dynamics of the RNAdS black hole phase transition has been studied based on the underlying free energy landscape [10,11].”
From Vacuum decay and bubble nucleation in the anti-de Sitter black holes (2022) · cites this paper as [10]
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Particle creation by black holes
Hawking, S. W. (1975) · Communications In Mathematical Physics · doi:10.1007/bf02345020 · Cited by 13,106 · cited 1×
“nergy landscape8 4 Kinetics and its uctuations of black hole state switching dynamics11 5 Conclusion17 1 Introduction Hawking’s original derivation of blackbody radiation from a collapsing black hole [1] revealed the thermal nature of black holes. This discovery established a close relationship between gravity, thermo…”
BackgroundAnti-de Sitter space, thermal phase transition, and confinement in gauge theories
Witten, E. (1998) · Advances in Theoretical and Mathematical Physics · doi:10.4310/atmp.1998.v2.n3.a3 · Cited by 3,915
Thermodynamics of black holes in anti-de Sitter space
Hawking, S. W., & Page, D. N. (1983) · Communications in Mathematical Physics · doi:10.1007/bf01208266 · Cited by 3,045
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Cited by
Sorted by citations
Vacuum decay and bubble nucleation in the anti-de Sitter black holes
Li, R., & Wang, J. (2022) · Journal of High Energy Physics · doi:10.1007/jhep09(2022)151 · Cited by 2
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Metadata
- Authors
- Li, R., Zhang, K., & Wang, J.
- Venue
- Journal of High Energy Physics
- Published
- 2020-10
- Volume
- 2020
- Issue
- 10
- ISSN
- 1029-8479
- Cited by
- 74
- References
- 3
- Language
- en
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