To theory of asymptotically stable accelerating universe in Riemann-Cartan spacetime

dc.contributor.author	Garkun A.
dc.contributor.author	Kudin V.
dc.contributor.author	Minkevich A.
dc.date.accessioned	2018-09-18T20:36:02Z
dc.date.available	2018-09-18T20:36:02Z
dc.date.issued	2014
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/141561
dc.description.abstract	© 2014 IOP Publishing Ltd and Sissa Medialab srl. Homogeneous isotropic cosmological models built in the framework of the Poincaré gauge theory of gravity based on general expression of gravitational Lagrangian with indefinite parameters are analyzed. Special points of cosmological solutions for flat cosmological models at asymptotics and conditions of their stability in dependence of indefinite parameters are found. Procedure of numerical integration of the system of gravitational equations at asymptotics is considered. Numerical solution for accelerating Universe without dark energy is obtained.
dc.subject	Dark energy theory
dc.subject	Gravity
dc.subject	Modified gravity
dc.title	To theory of asymptotically stable accelerating universe in Riemann-Cartan spacetime
dc.type	Article
dc.relation.ispartofseries-issue	12
dc.relation.ispartofseries-volume	2014
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS-2014-2014-12-SID84918496736

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