Thermal analysis with emission energy of perturbed black hole in f (Q) gravity

被引：71

作者：

Javed, Faisal ^{[1
]}

Mustafa, G. ^{[1
]}

Mumtaz, Saadia ^{[2
]}

Atamurotov, Farruh ^{[3
,4
,5
,6
]}

机构：

[1] Zhejiang Normal Univ, Dept Phys, Jinhua 321004, Peoples R China

[2] Univ Punjab, Inst Chem Engn & Technol, Quaid E Azam Campus, Lahore 54590, Pakistan

[3] New Uzbekistan Univ, Mustaqillik Ave 54, Tashkent 100007, Uzbekistan

[4] Akfa Univ, Milliy Bog St 264, Tashkent 111221, Uzbekistan

[5] Inha Univ Tashkent, Ziyolilar 9, Tashkent 100170, Uzbekistan

[6] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan

来源：

NUCLEAR PHYSICS B | 2023年 / 990卷

关键词：

QUASI-NORMAL MODES; HAWKING RADIATION; CORRECTED THERMODYNAMICS; PHASE-TRANSITION; FLUCTUATIONS; GEOMETRY; ENTROPY; FIELD;

D O I：

10.1016/j.nuclphysb.2023.116180

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：

In the present paper, we investigate the thermodynamics of a new perturbed black hole solution in symmetric teleparallel gravity. Our main focus is on the solution for a nonlinear model like Q + & alpha; Q2. We study new features of null geodesics and quasi-normal modes that occur for the current perturbed black hole solution. We inspect the critical behavior of thermal fluctuation and phase transitions in the background of a considered black hole solution and get the Davies points. To complete this study, we also explore the interesting aspects of the emission energy and quantum fluctuations. We highlight that our results are in good agreement with the thermodynamics of the previous black hole solutions and assumptions presented in the literature. & 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：19

共 84 条

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