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The Polish doughnuts revisited I. The angular momentum distribution and equipressure surfaces

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arxiv 0812.2467 v2 pith:ONVUSZDW submitted 2008-12-12 astro-ph

classification astro-ph
keywords angularequipressuremomentumsurfacesdisksdistributionthoseaccretion
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We construct a new family of analytic models of black hole accretion disks in dynamical equilibria. Our construction is based on assuming distributions of angular momentum and entropy. For a particular choice of the distribution of angular momentum, we calculate the shapes of equipressure surfaces. The equipressure surfaces we find are similar to those in thick, slim and thin disks, and to those in ADAFs.

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  1. Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH

    astro-ph.HE 2019-09 conditional novelty 6.0 of 10

    Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to...

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