Abstract
We describe the recent results obtained on the problem of accretion of dark matter by supermassive black holes, based on the evolution of matter fields on a black hole space-time. We mention the results for the models where dark matter is assumed to be an ideal gas, both with and without pressure, and the model that considers the dark matter is a scalar field. Up to now the analyses focus only on the radial accretion.
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 callDisclaimer: 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.
