Complete Cosmological Evolution Model of a Classical Scalar Field with a Higgs Potential. II. Numerical Simulation

dc.contributor.author	Ignat’ev Y.G.
dc.contributor.author	Samigullina A.R.
dc.date.accessioned	2022-02-09T20:35:44Z
dc.date.available	2022-02-09T20:35:44Z
dc.date.issued	2021
dc.identifier.issn	1064-8887
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/169281
dc.description.abstract	A complete cosmological evolution model of the classical scalar field with a Higgs potential is studied and simulated on a computer without the assumption that the Hubble constant is nonnegative. It is shown that with most initial conditions, the cosmological model goes from the expansion stage to the compression stage. Thus, cosmological models based on the classical Higgs field are unstable to finite perturbations.
dc.relation.ispartofseries	Russian Physics Journal
dc.subject	cosmological models
dc.subject	Einstein–Higgs hypersurface
dc.subject	global behavior
dc.subject	Higgs fields
dc.title	Complete Cosmological Evolution Model of a Classical Scalar Field with a Higgs Potential. II. Numerical Simulation
dc.type	Article
dc.relation.ispartofseries-issue	5
dc.relation.ispartofseries-volume	64
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	931
dc.source.id	SCOPUS10648887-2021-64-5-SID85115995143

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.