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

被引：1

作者：

Macedo, M. H. ^{[1
]}

Furtado, J. ^{[2
,3
]}

Alencar, G. ^{[1
]}

Landim, R. R. ^{[1
]}

机构：

[1] Univ Fed Ceara UFC, Dept Fis, Campus Pici,CP 6030, BR-60455760 Fortaleza, CE, Brazil

[2] Univ Fed Cariri UFCA, Av Tenente Raimundo Rocha,Cidade Univ, BR-63048080 Juazeiro Do Norte, Ceara, Brazil

[3] Gazi Univ, Fac Sci, Dept Phys, TR-06500 Ankara, Turkiye

来源：

ANNALS OF PHYSICS | 2024年 / 471卷

关键词：

Regular black holes; Thermodynamics; Quasinormal modes; Dymnikova black hole; Higher dimensions; STABILITY; REMNANTS; TENSOR;

D O I：

10.1016/j.aop.2024.169833

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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.

引用

页数：9

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