Model of Decaying Dark Energy Based on the Kaluza–Klein Theory

dc.contributor.author	Zakirov U.
dc.date.accessioned	2018-04-05T07:09:32Z
dc.date.available	2018-04-05T07:09:32Z
dc.date.issued	2017
dc.identifier.issn	1064-8887
dc.identifier.uri	http://dspace.kpfu.ru/xmlui/handle/net/129816
dc.description.abstract	© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltrami’s geometry – manifolds of constant negative curvature, the Klein–Gordon problem has been solved, making it possible, under the assumption of a physical structure of the fifth dimension (presumably a rich form of matter), to model on the basis of the Kaluza–Klein theory the hypothesis of decaying dark energy configuring the rates of expansion of the Universe.
dc.relation.ispartofseries	Russian Physics Journal
dc.subject	Beltrami surface
dc.subject	dark energy
dc.subject	deceleration parameter
dc.subject	fifth dimension
dc.subject	scalar field
dc.subject	scalar potential
dc.title	Model of Decaying Dark Energy Based on the Kaluza–Klein Theory
dc.type	Article in Press
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	1
dc.source.id	SCOPUS10648887-2017-SID85026898406

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