Thermodynamic properties of Reissner—Nordström—de Sitter quintessence black holes

Abstract

The mass, electric charge, and temperature of black holes in the Reissner-Nordström-de Sitter quintessence (RN-dSQ) spacetime are obtained. The heat capacities of the RN-dSQ black holes for certain electric charges and masses are analyzed. The electrostatic energy and dark energy in the RN-dSQ black holes are also calculated.

Black hole solutions surrounded by perfect fluid in Rastall theory

“…Phase transition, quasinormal modes and Hawking radiation of Schwarzschild black hole in the quintessence field are studied in [59,60,61]. Also, One may refer to [62,63,64,65,66,67] for more detail in thermodynamical analysis of the Schwarzschild, Reissner-Nordström and Reissner-Nordström-AdS black holes in a quintessence background.…”

Geometric structure and thermodynamic properties of ZPS black hole

“…史瓦西(Schwarzschild)黑洞描述无物质分布的 球对称黑洞时空, 它的质量隐藏于黑洞的内部. 一 类静态球对称黑洞的度规取多项式的形式, 时空能 量-动量张量的四个分量满足T t t = T r r 和T θ θ = T φ φ [1][2][3] . 这 类 球 对 称 时 空 解 包 括 史 瓦 西 黑 洞、 德 西 特(de Sitter)黑 洞(正 真 空 能)、 反 德 西 特(anti-de Sitter)黑 洞(负 真 空 能)和RN 黑 洞(静 电 能)等 时 空 解. Hay-ward时空可考虑为史瓦西黑洞时空的一个推广 [4] .…”

Thermal properties of regular black hole with electric charge in Einstein gravity coupled to nonlinear electrodynamics*

“…Letting f = 0, one obtains the energy enclosed by the horizon of the NED black hole as E H = (1/2)r H . The first law of thermodynamics for the NED black hole reads [36][37][38]…”