Thermodynamics and quasinormal modes of the Dymnikova black hole in higher dimensions

IF 3 3区物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY

Annals of Physics Pub Date : 2024-11-01 DOI:10.1016/j.aop.2024.169833

M.H. Macêdo , J. Furtado , G. Alencar , R.R. Landim

引用次数: 0

Abstract

In this study, we investigate the thermodynamic properties and quasinormal modes of Dymnikova black holes within the context of higher dimensions in Einstein’s general theory of relativity. We calculate the thermodynamic parameters, including the Hawking temperature and heat capacity, which allowed us to investigate the black hole’s stability. Lastly the quasinormal modes with the WKB formula were calculated.

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高维度迪姆尼科娃黑洞的热力学和准正常模式

在这项研究中，我们在爱因斯坦广义相对论的更高维度背景下研究了迪米尼科娃黑洞的热力学性质和类常态模式。我们计算了霍金温度和热容量等热力学参数，从而研究了黑洞的稳定性。最后，我们用 WKB 公式计算了准正常模式。

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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来源期刊

Annals of Physics 物理-物理：综合

CiteScore

5.30

自引率

3.30%

发文量

211

审稿时长

47 days

期刊介绍： Annals of Physics presents original work in all areas of basic theoretic physics research. Ideas are developed and fully explored, and thorough treatment is given to first principles and ultimate applications. Annals of Physics emphasizes clarity and intelligibility in the articles it publishes, thus making them as accessible as possible. Readers familiar with recent developments in the field are provided with sufficient detail and background to follow the arguments and understand their significance. The Editors of the journal cover all fields of theoretical physics. Articles published in the journal are typically longer than 20 pages.