Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT correspondence

被引：53

作者：

Sakti, Muhammad F. A. R. ^{[1
]}

Suroso, Agus ^{[1
,2
]}

Zen, Freddy P. ^{[1
,2
]}

机构：

[1] Inst Teknol Bandung, THEPI Div, Theoret Phys Lab, Jl Ganesha 10, Bandung 40132, Indonesia

[2] Inst Teknol Bandung, ICTMP, Jl Ganesha 10, Bandung 40132, Indonesia

来源：

ANNALS OF PHYSICS | 2020年 / 413卷

关键词：

Demianski-Newman-Janis algorithm; Rastall gravity; Thermodynamics; Kerr/CFT correspondence; NONZERO DIVERGENCE; THERMODYNAMICS; SPACE;

D O I：

10.1016/j.aop.2019.168062

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We present a new twisted rotating black hole solution by performing Demianski-Newman-Janis algorithm to the electrically and dyonically charged black hole with quintessence in Rastall theory of gravity. Using our black hole solution, we argue that Rastall gravity is not equivalent with Einstein gravity. For further explanation, the black hole properties such as the horizon and ergosphere are studied for which there are some different properties for those theories. Some thermodynamic properties of the black hole solution are also discussed. At the end, considering the Kerr/CFT correspondence is valid for our black hole solution, the central charge from the CFT of this extremal solution is derived. (C) 2019 Elsevier Inc. All rights reserved.

引用

页数：20

共 120 条

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