Quasinormal modes of the Hayward black hole surrounded by quintessence: Scalar, electromagnetic and gravitational perturbations

被引：5
|
作者：
Pedraza, Omar [1 ]
Lopez, L. A. [1 ]
Arceo, R. [2 ]
Cabrera-Munguia, I [3 ]
机构：
[1] UAEH, Area Acad Matemat & Fis, Carretera Pachuca Tulancingo Km 4-5, Mineral De La Reforma 42184, Hidalgo, Mexico
[2] Univ Autonoma Chiapas, Fac Ciencias Fis & Matemat, Tuxtla Gutierrez 29050, Chiapas, Mexico
[3] Univ Autonoma Ciudad Juarez, Dept Fis & Matemat, Ciudad Juarez 32310, Chihuahua, Mexico
来源：
MODERN PHYSICS LETTERS A | 2022年 / 37卷 / 09期
关键词：
Quasinormal modes; quintessence; WKB approximation; COSMOLOGICAL CONSTANT; DARK ENERGY; GEODESICS;
D O I：
10.1142/S0217732322500572
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, we study the quasinormal modes for scalar, electromagnetic, and gravitational axial perturbations in the Hayward regular black hole surrounded by quintessence (HBH-omega(q)). Using the third-order WKB approximation, we can determine the dependence of the quasinormal modes on the parameters of the regular black hole and the parameters on the test fields. We also determine the greybody factor, giving transmission and reflection coefficients of the scattered wave through the effective potentials in the WKB approximation using numerical analysis.
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页数：23
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