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

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dc.contributor.author Malec, Edward
dc.date.accessioned 2017-08-29T09:14:25Z
dc.date.available 2017-08-29T09:14:25Z
dc.date.issued 1999
dc.identifier.citation Malec, 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.60.104043 en
dc.identifier.volume 60
dc.identifier.issued 10
dc.identifier.issn 0556-2821
dc.identifier.uri http://hdl.handle.net/10468/4579
dc.identifier.doi 10.1103/PhysRevD.60.104043
dc.description.abstract We 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.format.mimetype application/pdf en
dc.language.iso en en
dc.publisher American Physical Society en
dc.relation.uri https://journals.aps.org/prd/abstract/10.1103/PhysRevD.60.104043
dc.rights © 1999, American Physical Society en
dc.subject Bondi model en
dc.subject Newtonian en
dc.subject Adiabatic index en
dc.subject Relativistic description en
dc.title Fluid accretion onto a spherical black hole: Relativistic description versus the Bondi model en
dc.type Article (peer-reviewed) en
dc.internal.authorcontactother Edward Malec, Physics, University College Cork, Cork, Ireland. +353-21-490-3000. en
dc.internal.availability Full text available en
dc.description.version Published Version en
dc.internal.wokid WOS:000083862300070
dc.description.status Peer reviewed en
dc.identifier.journaltitle Physical Review D en
dc.identifier.articleid 104043


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