Strange Quark Matter as Dark Matter

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Please use this identifier to cite or link to this item: https://elib.bsu.by/handle/123456789/254361

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DC Field	Value	Language
dc.contributor.author	Terazawa, H.	-
dc.date.accessioned	2021-01-21T09:25:42Z	-
dc.date.available	2021-01-21T09:25:42Z	-
dc.date.issued	2019	-
dc.identifier.citation	Nonlinear Phenomena in Complex Systems. - 2019. - Vol. 22, N 4. - P. 311-317	ru
dc.identifier.issn	1561-4085	-
dc.identifier.uri	https://elib.bsu.by/handle/123456789/254361	-
dc.description.abstract	New forms of matter such as super-hypernuclei (strange quark matter) and superhypernuclear stars (strange quark stars) as candidates for dark matter are discussed in some detail, based on the so-called “Bodmer–Terazawa–Witten hypothesis” assuming that they are stable absolutely or quasi-stable (decaying only weakly).	ru
dc.language.iso	en	ru
dc.publisher	Minsk : Education and Upbringing	ru
dc.rights	info:eu-repo/semantics/restrictedAccess	en
dc.subject	ЭБ БГУ::ЕСТЕСТВЕННЫЕ И ТОЧНЫЕ НАУКИ::Физика	ru
dc.title	Strange Quark Matter as Dark Matter	ru
dc.type	article	en
dc.rights.license	CC BY 4.0	ru
Appears in Collections:	2019. Volume 22. Number 4

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