2024/01/16 by Tripathi, Ashutosh, Mall, Gitika, Abdikamalov, Askar
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE)
paper · doi:10.48550/arxiv.2401.08545
General Relativity predicts the spacetime metric around an astrophysical black hole to be described by Kerr solution which is a massive rotating black hole without any residual charge. In a previous paper, we analyzed the NuSTAR observations of six X-ray binaries to obtain constraints on deformation parameter α13 using a state-of-the-art relativistic model. In this work, we continue analyzing NuSTAR observations of four more X-ray Binaries; two of which are X-ray Transients very close to the supermassive black hole at the center of our galaxy. The other two sources have complicated absorption which is accounted by time-resolved and flux-resolved spectroscopy. The constraints obtained are consistent with the Kerr hypothesis and are comparable with those obtained in previous studies and those from gravitational events.