Thermodynamics of regular black hole

2007/08/31 by Yun Soo Myung, Yong-Wan Kim, Young-Jai Park · 1 citation
Physics and Astronomy · #gr-qc

paper · pdf · doi:10.1007/s10714-008-0690-9

20 pages, 6 figures, version to appear in GRG

arxiv created 2008/09/21 · arxiv updated 2009/12/01

Abstract

We investigate thermodynamics for a magnetically charged regular black hole (MCRBH), which comes from the action of general relativity and nonlinear electromagnetics, comparing with the Reissner-Norström (RN) black hole in both four and two dimensions after dimensional reduction. We find that there is no thermodynamic difference between the regular and RN black holes for a fixed charge Q in both dimensions. This means that the condition for either singularity or regularity at the origin of coordinate does not affect the thermodynamics of black hole. Furthermore, we describe the near-horizon AdS₂ thermodynamics of the MCRBH with the connection of the Jackiw-Teitelboim theory. We also identify the near-horizon entropy as the statistical entropy by using the AdS₂/CFT₁ correspondence.

Cited by

• De Sitter cores from nonlocal quantum field theories

Related

• Thermodynamic geometry of the RN-AdS black hole and non-local observables
• A note on non-linear electrodynamics, regular black holes and the entropy function
• Thermodynamics of a class of regular black holes with a generalized uncertainty principle
• Magnetically charged regular black hole in a model of nonlinear electrodynamics
• Regular black holes and reductions of thermodynamic phase spaces