Regular black holes in isothermal cavity
arXiv:2012.03349 · doi:10.1016/j.physletb.2021.136426
Abstract
We examine the thermodynamic behavior of a static neutral regular (non-singular) black hole enclosed in a finite isothermal cavity. The cavity enclosure helps us investigate black hole systems in a canonical or a grand canonical ensemble. Here we demonstrate the derivation of the reduced action for the general metric of a regular black hole in a cavity by considering a canonical ensemble. The new expression of the action contains quantum corrections at short distances and concludes to the action of a singular black hole in a cavity at large distances. We apply this formalism to the noncommutative Schwarzschild black hole, in order to study the phase structure of the system. We conclude to a possible small/large stable regular black hole transition inside the cavity that exists neither at the system of a classical Schwarzschild black hole in a cavity, nor at the asymptotically flat regular black hole without the cavity. This phase transition seems to be similar with the liquid/gas transition of a Van der Waals gas.
arXiv comment10 pages, 4 figures, version appeared in Physics Letters B
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- Quantum corrections to the thermodynamics and phase transition of a black hole surrounded by a cavity in the extended phase space
- Schwarzschild black hole surrounded by a cavity and phase transition in the non-commutative gauge theory of gravity
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