Some observable physical properties of the higher dimensional dS/AdS black holes in Einstein-bumblebee gravity theory

被引:20
|
作者
Uniyal, Akhil [1 ]
Kanzi, Sara [2 ]
Sakalli, Izzet [3 ]
机构
[1] Indian Inst Technol, Dept Phys, Gauhati 781039, India
[2] Final Int Univ, Fac Engn, Via Mersin 10, TR-99370 Kyrenia, Northern Cyprus, Turkiye
[3] Eastern Mediterranean Univ, Phys Dept, Via Mersin 10, TR-99628 Famagusta, North Cyprus, Turkiye
来源
EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 07期
关键词
QUASI-NORMAL MODES; TELESCOPE RESULTS. I; GREYBODY RADIATION; LORENTZ VIOLATION; WKB APPROACH; SHADOW; ASTROPHYSICS; SPACETIME; BREAKING; SYMMETRY;
D O I
10.1140/epjc/s10052-023-11846-8
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
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS)/anti de-Sitter (AdS) black hole spacetimes derived from the Einstein-bumblebee gravity theory within the Lorentz symmetry breaking (LSB) framework. We specifically apply the semi-analytical WKB method and the time domain approach to study the scalar and Dirac perturbations of the black hole. In-depth researches are done on the effects of the LSB and dimensionality on the bosonic/fermionic greybody factors, quasinormal modes, and shadow of the higher dimensional bumblebee black hole. The results obtained are discussed, tabulated, and illustrated graphically.
引用
收藏
页数:19
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