Instabilities and anti-evaporation of Reissner-Nordstrom black holes in modified F(R) gravity

被引:69
|
作者
Nojiri, Shin'ichi [1 ,2 ]
Odintsov, Sergei D. [3 ,4 ,5 ,6 ,7 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan
[3] ICREA, Bellaterra 08193, Barcelona, Spain
[4] Inst Ciencies Espai IEEC CSIC, Bellaterra 08193, Barcelona, Spain
[5] Tomsk State Pedag Univ, Tomsk 634061, Russia
[6] Natl Res Tomsk State Univ, Tomsk 634050, Russia
[7] King Abdulaziz Univ, Jeddah 21413, Saudi Arabia
关键词
SPHERICALLY SYMMETRIC-SOLUTIONS; SCALARS;
D O I
10.1016/j.physletb.2014.06.070
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the instabilities and related anti-evaporation of the extremal Reissner-Nordstrom (RN) black hole in F(R) gravity. It is remarkable that the effective electric charge can be generated for some solutions of F(R) gravity without electromagnetic field. The anti-evaporation effect occurs but it emerges only in the strong coupling limit of the effective gravitational coupling. The instabilities of RN black hole are also investigated when the electromagnetic sector is added to the action of F(R) gravity. We show the anti-evaporation occurs in the Maxwell-F(R) gravity with the arbitrary gravitational coupling constant although it does not occur in the Maxwell-Einstein gravity. Furthermore, general spherically-symmetric solution of F(R) gravity in the Einstein frame is obtained. (C) 2014 Published by Elsevier B.V.
引用
收藏
页码:376 / 382
页数:7
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