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dc.contributor.authorТихомиров, Виктор Васильевич-
dc.contributor.authorЮралевич, Светлана Эдвардовна-
dc.date.accessioned2018-12-13T09:43:12Z-
dc.date.available2018-12-13T09:43:12Z-
dc.date.issued2003-
dc.identifier.citationВестник Белорусского государственного университета. Сер. 1, Физика. Математика. Информатика. – 2003. - № 1. – С. 27-33.ru
dc.identifier.issn0321-0367-
dc.identifier.urihttp://elib.bsu.by/handle/123456789/210814-
dc.description.abstractPrimordial black holes (PBHs) of masses M≥5*1014 g are able to absorb white dwarfs (WD), giving rise to formation of black holes of WD masses. The WD absorption is accompanied by up to 1052 erg neutrino bursts which can be readily detected by modern neutrino detectors. We calculate time characteristics of such a burst in this paper.ru
dc.language.isoruru
dc.publisherМинск : БГУru
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.subjectЭБ БГУ::ЕСТЕСТВЕННЫЕ И ТОЧНЫЕ НАУКИ::Физикаru
dc.subjectЭБ БГУ::ЕСТЕСТВЕННЫЕ И ТОЧНЫЕ НАУКИ::Астрономияru
dc.titleНейтринная вспышка белого карлика, поглощаемого первичной черной дыройru
dc.typearticleru
Appears in Collections:2003, №1 (январь)

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