Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources
High Energy Astrophysical Phenomena
2016-11-15 v1 General Relativity and Quantum Cosmology
Abstract
We model two temperature viscous accretion flows in the sub-Keplerian, optically thin, regime around rotating black holes including important radiation effects self-consistently. The model successfully explains observed luminosities from ultra-luminous to under-luminous sources and predicts the spin parameter of black holes.
Keywords
Cite
@article{arxiv.1101.4626,
title = {Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources},
author = {Banibrata Mukhopadhyay},
journal= {arXiv preprint arXiv:1101.4626},
year = {2016}
}
Comments
4 pages including a figure; to appear in the proceedings of MG12, Marcel Grossman Meeting, Paris, France, 12-18 July 2009