Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources

Banibrata Mukhopadhyay

doi:10.1142/9789814374552_0110

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arXiv · 1101.4626

Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources

Banibrata Mukhopadhyay

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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.

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Banibrata Mukhopadhyay. 2011-01-24. Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources. https://doi.org/10.1142/9789814374552_0110

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