Relativistic cross sections of tidal disruption events

In this contribution I introduce and discuss the so-called cross sections of tidal disruption and partial mass stripping of stars after a tidal encounter with a rotating supermassive black hole. The presented approach is fully relativistic. Possible applications and generalisations of the discussed...

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Main Author: Ivanov P.B.
Format: Article
Language:English
Published: EDP Sciences 2012-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20123901002
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spelling doaj-c53362a49ac64b35997fa4d722e4170c2021-08-02T16:12:00ZengEDP SciencesEPJ Web of Conferences2100-014X2012-12-01390100210.1051/epjconf/20123901002Relativistic cross sections of tidal disruption eventsIvanov P.B.In this contribution I introduce and discuss the so-called cross sections of tidal disruption and partial mass stripping of stars after a tidal encounter with a rotating supermassive black hole. The presented approach is fully relativistic. Possible applications and generalisations of the discussed results are also shortly reviewed. http://dx.doi.org/10.1051/epjconf/20123901002
collection DOAJ
language English
format Article
sources DOAJ
author Ivanov P.B.
spellingShingle Ivanov P.B.
Relativistic cross sections of tidal disruption events
EPJ Web of Conferences
author_facet Ivanov P.B.
author_sort Ivanov P.B.
title Relativistic cross sections of tidal disruption events
title_short Relativistic cross sections of tidal disruption events
title_full Relativistic cross sections of tidal disruption events
title_fullStr Relativistic cross sections of tidal disruption events
title_full_unstemmed Relativistic cross sections of tidal disruption events
title_sort relativistic cross sections of tidal disruption events
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2012-12-01
description In this contribution I introduce and discuss the so-called cross sections of tidal disruption and partial mass stripping of stars after a tidal encounter with a rotating supermassive black hole. The presented approach is fully relativistic. Possible applications and generalisations of the discussed results are also shortly reviewed.
url http://dx.doi.org/10.1051/epjconf/20123901002
work_keys_str_mv AT ivanovpb relativisticcrosssectionsoftidaldisruptionevents
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