Abstract
In this paper, we present the formation mechanisms of the accretion disk, shock cones and waves on the disk around the rotating black holes in the High Mass X-ray Binaries (HMXBs) solving the general relativistic hydrodynamic equation using the high resolution shock capturing scheme. We show how the disk and shock cones change depending on the initial conditions, Mach number, adiabatic index and the disk radius. Different physical conditions create different disk structures and these structures cause the varying physical mechanisms around the black holes. The shock cones around the black holes trap the oscillation modes. These trapped oscillation modes cause the quasiperiodic oscillation on the accretion disk. The different formations of disk help us to understand the properties of the black holes and mechanisms in the high mass X-ray binaries
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Süleyman Demirel Üniversitesi Fen Bilimleri Enstitüsü Dergisi
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
