Back reaction of the gravitational radiation on the metric of spacetime

dc.contributor.author	Grib A.
dc.contributor.author	Pavlov Y.
dc.date.accessioned	2019-01-22T20:36:06Z
dc.date.available	2019-01-22T20:36:06Z
dc.date.issued	2018
dc.identifier.issn	0218-2718
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/147910
dc.description.abstract	© 2018 World Scientific Publishing Company. The problem of back reaction of the gravitational radiation of the two merging black holes on the metric of the spacetime is investigated. It is shown for some models that large energy density of the gravitational waves close to the merger can lead to the disappearance of the visible accretion disc of the merged pair of black holes.
dc.relation.ispartofseries	International Journal of Modern Physics D
dc.subject	accretion disc
dc.subject	Gravitational waves
dc.subject	merging black holes
dc.title	Back reaction of the gravitational radiation on the metric of spacetime
dc.type	Article
dc.relation.ispartofseries-issue	7
dc.relation.ispartofseries-volume	27
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS02182718-2018-27-7-SID85042760894

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