弦云和暗物质晕对施瓦兹柴尔德黑洞周围粒子运动、阴影和表周期振荡的双重影响

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Rui-Yan Chen , Faisal Javed , G. Mustafa , S.K. Maurya , Saibal Ray
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引用次数: 0

摘要

在这项工作中,我们研究了具有三种不同暗物质晕和弦云参数的施瓦兹柴尔德黑洞周围的粒子动力学、阴影和准周期振荡。在弦云参数α的作用下考虑了粒子的运动,并对大质量和无质量粒子进行了研究。从有效势中得到了这些黑洞的光子轨道和内稳定圆轨道。利用三种不同的暗物质晕计算了黑洞阴影。与纯粹的施瓦兹柴尔德黑洞相比,在不同的弦云参数值下,这些黑洞的阴影半径会增大。此外,本次分析还讨论了准周期振荡。我们的研究探讨了轨道振荡和径向谐波振荡频率的径向剖面如何随弦云参数变化。本研究考察了测试粒子在黑洞赤道面稳定圆形轨道附近准周期振荡的主要特性。我们的研究结果表明,对受暗物质晕和弦云影响的黑洞进行观测测试也是可行的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dual effect of string cloud and dark matter halos on particle motions, shadows and epicyclic oscillations around Schwarzschild black holes
In this work, we study the particle dynamics, shadows and quasi-periodic oscillations around the Schwarzschild black hole with three different dark matter halos and string cloud parameters. The motion of particles is considered with the string cloud parameter α and investigated for massive and massless particles. The photon orbits and inner stable circular orbits of these black holes are obtained from the effective potential. The black hole shadows are calculated using three different dark matter halos. The shadow radius of these black holes increases compared to a pure Schwarzschild black hole for different values of the string cloud parameter. Further, quasi-periodic oscillations are also discussed in the current analysis. Our study examines how the radial profiles of orbital and radial harmonic oscillation frequencies change with the string cloud parameter. This study examines the major properties of test particle's quasi-periodic oscillations near stable circular orbits in the black hole equatorial plane. Our findings indicate that observational tests for black holes influenced by dark matter halos and cloud strings are also feasible and viable.
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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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