Schwarzschild-type black holes in Starobinsky-Bel-Robinson gravity

被引：13
|
作者：
Delgado, Ruben Campos [1 ]
Ketov, Sergei V. [2 ,3 ,4 ]
机构：
[1] Phys Inst Univ Bonn, Bethe Ctr Theoret Phys, Nussallee 12, D-53115 Bonn, Germany
[2] Tokyo Metropolitan Univ, Dept Phys, 1-1 Minami Ohsawa, Hachioji, Tokyo 1920397, Japan
[3] Tomsk State Univ, Interdisciplinary Res Lab, 36 Lenin Ave, Tomsk 634050, Russia
[4] Univ Tokyo Inst Adv Study, Kavli Inst Phys & Math Universe, Kashiwa 2778583, Japan
来源：
PHYSICS LETTERS B | 2023年 / 838卷
关键词：
Modified gravity; Black holes; ENTROPY;
D O I：
10.1016/j.physletb.2023.137690
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study physical properties of a Schwarzschild-type black hole in the framework of the recently proposed Starobinsky-Bel-Robinson (SBR) modified theory of gravity, working perturbatively in the coupling constant. In particular, we compute the temperature, entropy, pressure and lifetime of a Schwarzschild-type black hole.(c) 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons .org /licenses /by /4 .0/). Funded by SCOAP3.
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页数：4
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