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arXiv 2607.06321gr-qc
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非拓扑孤子巴丁玻色子星的偏振图像

Polarization images of non-topological soliton Bardeen boson stars

College of Physics and Optoelectronic Engineering, Chongqing Normal University(重庆师范大学物理与光电工程学院);Department of Mechanics, Chongqing Jiaotong University(重庆交通大学力学系);Center for Gravitational Wave Experiment, National Microgravity Laboratory, Institute of Mechanics, Chinese Academy of Sciences(中国科学院力学研究所微重力国家实验室引力波实验中心)

Xiao-Xiong Zeng, Chen-Yu Yang, Ke-Jian He, Li-Fang Li

AI总结:

研究通过求解方程,基于薄吸积盘模型探究非拓扑孤子巴丁玻色子星的偏振图像,分析初始标量场等关键参数影响,发现磁场几何形状等起关键作用,为比较玻色子星和黑洞提供定性依据。

摘要:

在本研究中,我们基于围绕这些致密天体的薄吸积盘模型,通过求解耦合的爱因斯坦非线性电动力学复标量场方程,研究非拓扑孤子巴丁玻色子星的偏振图像。我们关注包括初始标量场、磁荷、观测者倾角和磁场构型等关键参数对所得偏振特性的影响。结果表明,磁场几何形状,特别是径向\(B_r\)和角向\(B_\theta\)分量之间的相对强度,在确定偏振图案中起关键作用。此外,标量场振幅和磁荷的变化显著影响偏振的强度和空间分布。这些结果表明偏振形态对时空几何和磁场构型敏感,并为比较玻色子星与黑洞提供了定性基础。

英文摘要:

In this study, we investigate the polarized images of non-topological soliton Bardeen boson stars by solving the coupled Einstein nonlinear electrodynamics complex scalar field equations, based on the thin accretion disk model surrounding these compact objects. We focus on the influence of key parameters, including the initial scalar field, magnetic charge, observer inclination angle, and magnetic field configuration, on the resulting polarization characteristics. The results show that the geometry of the magnetic field, particularly the relative strength between the radial \(B_r\) and angular \(B_θ\) components, plays a crucial role in determining the polarization pattern. Additionally, variations in the scalar field amplitude and magnetic charge significantly affect both the intensity and spatial distribution of the polarization. These results show that the polarization morphology is sensitive to the spacetime geometry and magnetic field configuration, and provide a qualitative basis for comparing boson stars with black holes.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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