Instability of regular electric black hole

被引：6

作者：

Sajadi, S. N. ^{[1
,2
]}

Poshteh, M. B. Jahani ^{[3
,4
]}

Hendi, S. H. ^{[1
,2
,5
]}

机构：

[1] Shiraz Univ, Sch Sci, Dept Phys, Shiraz 71454, Iran

[2] Shiraz Univ, Sch Sci, Biruni Observ, Shiraz 71454, Iran

[3] Inst Adv Studies Basic Sci IASBS, Dept Phys, Zanjan 4513766731, Iran

[4] Inst Res Fundamental Sci IPM, Sch Phys, POB 19395-5531, Tehran, Iran

[5] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada

来源：

NUCLEAR PHYSICS B | 2021年 / 972卷

关键词：

NONLINEAR ELECTRODYNAMICS; THERMODYNAMICS;

D O I：

10.1016/j.nuclphysb.2021.115567

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

A new spherically symmetric exact solution of Einstein gravity in the presence of a nonlinear electromagnetic field is introduced. It is shown that such a solution can be interpreted as an electrically charged regular black hole that behaves like Reissner-Nordstrom metric, asymptotically. An extension of the solution in the presence of cosmological constant is presented and thermodynamic properties of the solution are studied in the extended phase space thermodynamics. Then, thermal stability and possible phase transition are investigated and the van der Waals like behavior is observed. Finally, the relation between the photon sphere with a thermodynamic phase transition is studied. (C) 2021 Published by Elsevier B.V.

引用

页数：24

共 56 条

[1] Thermodynamics of Rotating Black Holes and Black Rings: Phase Transitions and Thermodynamic Volume [J].