摘要
In this study,we investigated the astronomical implications of Rastall gravity,particularly its behavior amidst a radiation field compared to Reissner-Nordström(RN)black holes.We found a crucial correlation between the dynamics of the accretion disk and the parameters Q and Nr,which properly reflect the influence of spacetime metrics on the disk’s appearance.Elevated electric charge Q causes contraction in the disk’s orbit due to enhanced gravitational effects,while higher Nr values lead to outward expansion,influenced by the attributes of the radiation field.Interestingly,the charged black holes surrounded by radiation fields exhibit distinct visual disparities from RN black holes.Brightness decreases and expansion occurs within the innermost stable circular orbit of the accretion disk with rising Nr values.Our study also reveals the process by which the accretion disk transitions from a conventional disk-like structure to a hat-like form at different observation angles,with the redshift effect gradually intensifying.Moreover,the results of the considered Rastall gravity radiation field are consistent with the constraints of the gravitational lensing of the host galaxy on Rastall gravity parameters,thereby enhancing the consistency between theoretical predictions and actual observations.
作者
黄宇翔
郭森
梁宇
崔宇昊
蒋青权
林恺
Yu-Xiang Huang;Sen Guo;Yu Liang;Yu-Hao Cui;Qing-Quan Jiang;Kai Lin(School of Physics and Astronomy,China West Normal University,Nanchong 637000,China;Guangxi Key Laboratory for Relativistic Astrophysics,School of Physical Science and Technology,Guangxi University,Nanning 530004,China;Hubei Subsurface Multi-scale Imaging Key Laboratory,Institute of Geophysics and Geomatics,China University of Geosciences,Wuhan 430074,China)
基金
the National Natural Science Foundation of China(42230207)
the Fundamental Research Funds for the Central Universities,China University of Geosciences(Wuhan)(G1323523064)
the Sichuan Youth Science and Technology Innovation Research Team(21CXTD0038)。
