Fluid accretion onto a spherical black hole: Relativistic description versus the Bondi model

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dc.contributor.authorMalec, Edward
dc.date.accessioned2017-08-29T09:14:25Z
dc.date.available2017-08-29T09:14:25Z
dc.date.issued1999
dc.description.abstractWe describe general relativistically a spherically symmetric stationary fluid accretion onto a black hole. Relativistic effects enhance mass accretion, in comparison to the Bondi model predictions, in the case when back reaction is neglected. That enhancement depends on the adiabatic index and the asymptotic gas temperature and it can magnify accretion by one order in the ultrarelativistic regime. (S0556-2821(99)01120-0).en
dc.description.statusPeer revieweden
dc.description.versionPublished Versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.articleid104043
dc.identifier.citationMalec, E. (1999) 'Fluid accretion onto a spherical black hole: Relativistic description versus the Bondi model', Physical Review D, 60(10), 104043 (8pp). doi: 10.1103/PhysRevD.60.104043en
dc.identifier.doi10.1103/PhysRevD.60.104043
dc.identifier.issn0556-2821
dc.identifier.issued10
dc.identifier.journaltitlePhysical Review Den
dc.identifier.urihttps://hdl.handle.net/10468/4579
dc.identifier.volume60
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.60.104043
dc.rights© 1999, American Physical Societyen
dc.subjectBondi modelen
dc.subjectNewtonianen
dc.subjectAdiabatic indexen
dc.subjectRelativistic descriptionen
dc.titleFluid accretion onto a spherical black hole: Relativistic description versus the Bondi modelen
dc.typeArticle (peer-reviewed)en
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