Study of thermodynamic properties for charged power law black holes in Eddington-inspired Born-Infeld theory

F. S. Hariono, B. N. Jayawiguna, H. S. Ramadhan
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Abstract

We study thermodynamic properties of static spherically-symmetric and electrically-charged black hole in Eddington-inspired Born-Infeld (EiBi) Theory. We consider Maxwell electrodynamics with power law for the matter fields. Corrected black hole entropy is needed when we evaluate in EiBI theory of gravity [1] and we can derived the black hole mass. Specific heat CQ is derive√d from entropy and Hawking temperature. Results show that mostly of the black holes exist except when q=18(−3−41), κ = 1 and Q = 0.1. Black holes are unstable at first for a few values of Q, but CQ increases exponentially afterwards and becomes positive.
Eddington-inspired Born-Infeld理论中带电幂律黑洞热力学性质的研究
利用Eddington-inspired Born-Infeld (EiBi)理论研究了静态球对称带电黑洞的热力学性质。我们考虑麦克斯韦电动力学与幂律的物质场。在EiBI引力理论[1]中进行计算时,需要对黑洞熵进行修正,才能推导出黑洞质量。比热CQ由熵和霍金温度导出。结果表明,除了q=18(−3−41)、κ =1和q= 0.1外,大多数黑洞都存在。黑洞一开始在几个Q值下是不稳定的,但之后CQ呈指数增长并变为正值。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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