Supersonic and subsonic flows in general relativistic radiation hydrodynamics

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dc.creatorMalec, Edward
dc.creatorKarkowski, Janusz
dc.creatorRoszkowski, Krzysztof
dc.creatorSwierczynski, Zdobyslaw
dc.date2008-04-24
dc.date2009-01-26
dc.date.accessioned2026-07-07T12:34:12Z
dc.date.available2026-07-07T12:34:12Z
dc.descriptionWe analyze stationary accretion of selfgravitating gas onto a compact center within general-relativistic radiation hydrodynamics. Spherical symmetry and thin gas approximation are assumed. Numerical investigation shows that transonic flows exist for small redshifts and they cease to exist for high redshifts and high luminosities. There exist two branches of flows (subsonic or supersonic) that originate at a bifurcation point and that embrace the set of subsonic solutions. The morphology of the set of subsonic solutions is essentially independent of redshifts and flows that belong to their boundary provide estimates of the gas abundance of subsonic solutions. It appears that prescribed boundary data guarantee uniqueness only of the bifurcation point, and that the latter has maximal luminosity.
dc.description8 figures
dc.identifierhttps://arxiv.org/abs/0804.3898
dc.identifierhttp://arxiv.org/abs/0804.3898
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217341
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSupersonic and subsonic flows in general relativistic radiation hydrodynamics
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