Effects of rotation and deformation on the orbits of a Kerr-like spacetime

IF 3.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Diego Solano-Alfaro and Francisco Frutos-Alfaro
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引用次数: 0

Abstract

This study employs an approximate Kerr-like metric with a mass quadrupole perturbation to investigate the equatorial circular motion around deformed, rotating compact objects. The numerical results reveal how the quadrupole modifies the photon sphere and the innermost stable circular orbit, with implications for accretion dynamics near systems such as neutron stars. A stability analysis shows that certain symmetries are preserved in the effective potential, yielding equivalent behavior for co-rotating and counter-rotating particles. Comparisons with the Hartle–Thorne spacetime highlight the influence of higher-order multipole moments. Additionally, under the Black Widow pulsar equation of state, the metric suggests that inspiraling particles may temporarily form a transient, disk-like structure near the pulsar. This would allow interactions between co-rotating and counter-rotating matter. More research is needed to characterize this phenomenon and explore its observational signatures.
旋转和变形对类克尔时空轨道的影响
本研究采用近似kerr -类度量和质量四极摄动来研究围绕变形、旋转致密物体的赤道圆周运动。数值结果揭示了四极子如何改变光子球和最内层稳定的圆形轨道,并对中子星等系统附近的吸积动力学有启示。稳定性分析表明,有效势保持一定的对称性,使同旋转和反旋转粒子的行为等效。与Hartle-Thorne时空的比较突出了高阶多极矩的影响。此外,在黑寡妇脉冲星状态方程下,度规表明,吸入粒子可能在脉冲星附近暂时形成一个瞬态的盘状结构。这将允许同旋转和反旋转物质之间的相互作用。需要更多的研究来描述这一现象并探索其观测特征。
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
Classical and Quantum Gravity
Classical and Quantum Gravity 物理-天文与天体物理
CiteScore
7.00
自引率
8.60%
发文量
301
审稿时长
2-4 weeks
期刊介绍: Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.
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