1. On Thermodynamic Stability of Black Holes. Part I: Classical stability
- Author
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Avramov, V., Dimov, H., Radomirov, M., Rashkov, R. C., and Vetsov, T.
- Subjects
High Energy Physics - Theory ,High Energy Physics - Theory (hep-th) ,FOS: Physical sciences ,General Relativity and Quantum Cosmology (gr-qc) ,General Relativity and Quantum Cosmology - Abstract
We revisit the thermodynamic stability of the standard black hole solutions by presenting the intrinsic necessary and sufficient conditions for stable global and local thermodynamic equilibrium. The criteria for such equilibria are quite generic and well-established in classical thermodynamics, but they have not been fully utilized in black hole physics. The global thermodynamic analysis is based on two equivalent criteria: the Hessian eigenvalue method in energy representation and the Sylvester criterion for positive definiteness of quadratic forms. The study of local thermodynamic stability is realized through the calculation of the admissible black hole heat capacities and their positiveness. The existence of critical points and phase transitions of the black hole is determined by the divergences of the corresponding heat capacities. This paper is the first in the line of intended works on thermodynamic stability of black holes in modified theories of gravity and holography., Comment: 27 pages, no figures, no tables
- Published
- 2023
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