The role of topological photon spheres in constraining the parameters of black holes

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Jafar Sadeghi, Mohammad Ali S. Afshar
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引用次数: 0

Abstract

In this paper, we investigate the topological photon sphere from two distinct perspectives. In the first view, we examine the existence and characteristics of topological photon (anti-photon) spheres for black holes with different structures, such as Einstein–Young–Mills non-minimal, AdS black holes surrounded by Chaplygin-like dark fluid, and Bardeen-like black holes in Einstein–Gauss–Bonnet gravity. Furthermore, we delve into the deeper perspective of the necessity of photon spheres for super-compact gravitational structures such as black holes. By leveraging this necessity, we propose a classification of the parameter space of black hole models based on the existence and positioning of photon spheres. This approach enables the determination of parameter ranges that delineate whether a solution represents a black hole or a naked singularity. In essence, the paper illustrates the utility of the photon sphere as a notable test for establishing the permissible and non-permissible parameter ranges within specific theories of black hole solutions.

拓扑光子球在约束黑洞参数方面的作用
本文从两个不同的角度研究拓扑光子球。第一个角度,我们研究了不同结构黑洞的拓扑光子(反光子)球的存在和特征,如爱因斯坦-杨-米尔斯非最小黑洞、被查普里金类暗流体包围的 AdS 黑洞,以及爱因斯坦-高斯-波奈引力中的巴丁类黑洞。此外,我们还从更深的角度探讨了光子球对于黑洞等超紧密引力结构的必要性。利用这种必要性,我们提出了一种基于光子球的存在和定位的黑洞模型参数空间分类方法。这种方法可以确定参数范围,从而划定一个解决方案代表的是黑洞还是裸奇点。从本质上讲,本文说明了光子球作为一种显著的检验方法的实用性,可用于确定特定黑洞解理论中允许和不允许的参数范围。
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
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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