Thermodynamic stability and holographic heat engine efficiency of a Kerr-Newmann-NUT-Kiselev-AdS black hole in Rastall gravity

被引：2

作者：

Karmakar, Sourav ^{[1
]}

Roy, Tanusree ^{[2
]}

Debnath, Ujjal ^{[2
]}

机构：

[1] Jadavpur Univ, Dept Instrumentat & Elect, Salt Lake Bypass,LB Block,Sect III, Kolkata 700098, India

[2] Indian Inst Engn Sci & Technol, Dept Math, Howrah 711103, India

来源：

ANNALS OF PHYSICS | 2023年 / 457卷

关键词：

Rastall gravity; KN-NUT-Kiselev-AdS black hole; Perfect fluid matter; Dark energy; Holographic heat engine; PARAMETER-ESTIMATION; ENERGY; QUINTESSENCE; MATTER;

D O I：

10.1016/j.aop.2023.169425

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Einstein's general relativity was modified to the Rastall grav-ity by generalizing the energy-momentum conservation law to T & mu;& nu; ;& mu; & lambda;R & nu; and for this change in the covariant conservation = of T & mu;& nu; the thermodynamic characteristics also show some inter-esting properties. Here we discuss the thermodynamics, phase transition, stability and heat engine construction of a Kerr- Newman-NUT-Kiselev-AdS black hole in 4D Rastall gravity. We consider the space to be surrounded by dark energy, a specific perfect fluid matter. The dark energy has significant effects on the thermodynamic variables of the black hole. Here, the energy condition constraints the Rastall parameter (& lambda;). We finally find that the equation-of-state is related to the Rastall parameter (& lambda;) even when it is reduced to the critical point. The cosmological constant leads us to consider the black hole as a heat engine and determine the efficiency of the Carnot cycle for the black hole. In conclusion, we discuss possible methodologies for constraining the black hole parameters from astrophysical observations. & COPY; 2023 Published by Elsevier Inc.

引用

页数：18

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