Recovery of consistency in thermodynamics of regular black holes in Einstein's gravity coupled with nonlinear electrodynamics
arXiv:2306.12709 · doi:10.1016/j.nuclphysb.2024.116491
Abstract
As one of candidate theories in the construction of regular black holes, Einstein's gravity coupled with nonlinear electrodynamics has been a topic of great concerns. Owing to the coupling between Einstein's gravity and nonlinear electromagnetic fields, we need to reconsider the first law of thermodynamics, which will lead to a new thermodynamic phase space. In such a phase space, the equation of state accurately describes the complete phase transition process of regular black holes. The Maxwell equal area law strictly holds when the phase transition occurs, and the entropy obeys the Bekenstein-Hawking area formula, which is compatible with the situation in Einstein's gravity.
v1: 18 pages, 7 figures; v2: 20 pages, clarifications and references added, final version to appear in Nuclear Physics B
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Cited by in corpus (4)
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- On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows
- Signal of phase transition hidden in quasinormal modes of regular AdS black holes
- Thermodynamic phase transition and winding number for the third-order Lovelock black hole