与非线性电动力学耦合的 f(R,T) 引力中的带磁正规黑洞

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Takol Tangphati , Menglong Youk , Supakchai Ponglertsakul
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引用次数: 0

摘要

我们在与非线性电动力学拉格朗日耦合的f(R,T)引力中构建了近似平坦、静态球对称、中心规则的黑洞。我们得到了巴丁黑洞和海沃德黑洞的广义度量函数。我们讨论了这些解的空能、弱能和强能条件。通过适当选择参数,所有能量条件在黑洞外事件视界外都成立。此外,还研究了大质量标量扰动的准正态模式。准正态频率是通过六阶 Wentzel-Kramers-Brillouin (WKB) 与 Padé 近似计算的。发现频率的所有虚部都是负的。最后,我们还提供了一个埃可纳极限分析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetically charged regular black holes in f(R,T) gravity coupled to nonlinear electrodynamics

We construct asymptotically flat, static spherically symmetric black holes with regular centre in f(R,T) gravity coupled to nonlinear electrodynamics Lagrangian. We obtain generalized metric function of the Bardeen and Hayward black holes. The null, weak and strong energy conditions of these solutions are discussed. All the energy conditions hold outside the black hole's outer event horizon by appropriated choices of parameters. Quasinormal mode of massive scalar perturbation is also investigated. Quasinormal frequencies are computed via the sixth order Wentzel-Kramers-Brillouin (WKB) with Padé approximation. All the imaginary parts of the frequencies are found to be negative. Finally, we provide an analysis in the eikonal limit.

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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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