Hayward black holes in Einstein-Gauss-Bonnet gravity

被引:38
作者
Kumar, Arun [1 ]
Singh, Dharm Veer [2 ]
Ghosh, Sushant G. [1 ,3 ,4 ]
机构
[1] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
[2] GIA Univ, Inst Appl Sci & Humanities, Dept Phys, Mathura 281406, India
[3] Jamia Millia Islamia, Multidisciplinary Ctr Adv Res & Studies MCARS, New Delhi 110025, India
[4] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Private Bag X54001, ZA-4000 Durban, South Africa
关键词
Hayward; Black holes; Regular; THERMODYNAMICS; DESITTER; REMNANTS; TENSOR; SPACE;
D O I
10.1016/j.aop.2020.168214
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Hayward metric is a spherically symmetric charged regular black holes, a modification of the Reisnner-Nordstrom black holes of Einstein's equations coupled to nonlinear electrodynamics. We consider Einstein-Gauss-Bonnet gravity (EGB) coupled to nonlinear electrodynamics to present an exact five dimension (5D) Hayward black holes with a regular center, having inner (Cauchy) and outer (event) horizons which go over to Boulware-Desser black holes when the charge is switched off (e = 0). The presence of charge e leads the modification in thermodynamical quantities, and it has also been shown that the Hawking-Page like phase transition can be achieved. The specific heat shows divergence at the horizon radius r = r(C) (critical radius), where the temperature has a maximum. Our result in the limit, e -> 0, reduces vis-a-vis to the 5D Boulware-Desser solutions. (C) 2020 Elsevier Inc. All rights reserved.
引用
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页数:13
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