Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow

被引：7

作者：

Hamil, B. ^{[1
]}

Lutfuoglu, B. C. ^{[2
]}

机构：

[1] Univ Constantine 1, Fac Sci Exactes, Dept Phys, Constantine, Algeria

[2] Univ Hradec Kralove, Dept Phys, Rokitanskeho 62, Hradec Kralove 50003, Czech Republic

来源：

NUCLEAR PHYSICS B | 2023年 / 990卷

关键词：

COSMOLOGICAL CONSTANT; ACCRETION; DISPERSION; UNIVERSE; ENERGY;

D O I：

10.1016/j.nuclphysb.2023.116191

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

According to some quantum gravity models, Lorentz invariance can be violated in the Planck energy scale. With this motivation, we analyze the thermal quantities and the stability of Schwarzschild black hole surrounded by quintessence in gravity's rainbow formalism. To do that, we consider the rainbow functions which are motivated by loop quantum gravity and gamma-ray bursts, and we derive Hawking temperature, specific heat, entropy and the equation of state function. We observe that the presence the quintessence matter field and rainbow gravity affect the stability of the black hole. & COPY; 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.

引用

页数：12

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