Sub-Planckian Scale and Limits for f(R) Models

Petriakova Polina; Rubin Sergey Georgievich; Popov Arkadiy Aleksandrovich

dc.contributor	Казанский федеральный университет
dc.contributor.author	Petriakova Polina
dc.contributor.author	Popov Arkadiy Aleksandrovich
dc.contributor.author	Rubin Sergey Georgievich
dc.date.accessioned	2021-02-15T11:40:05Z
dc.date.available	2021-02-15T11:40:05Z
dc.date.issued	2021
dc.identifier.citation	Petriakova P. Sub-Planckian Scale and Limits for f(R) Models / P. Petriakova, A. Popov, S. Rubin // Symmetry. - 2021. - V.13. - Id.313. - doi: 10.3390/sym13020313.
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/160648
dc.description.abstract	We study the universe evolution starting from the sub-Planckian scale to present times. The requirement for an exponential expansion of the space with the observed metric as a final stage leads to significant restrictions on the parameter values of a function f(R). An initial metric of the universe should be maximally symmetric with the positive curvature.
dc.language.iso	en
dc.relation.ispartofseries	Symmetry
dc.rights	открытый доступ
dc.subject	f(R) gravity
dc.subject	cosmology
dc.subject	Planck energies
dc.subject.other	Математика
dc.title	Sub-Planckian Scale and Limits for f(R) Models
dc.type	Article
dc.contributor.org	Институт математики и механики им.Н.И.Лобачевского
dc.description.pages	313(1)-313(7)
dc.relation.ispartofseries-issue	2
dc.relation.ispartofseries-volume	13
dc.pub-id	248735
dc.identifier.doi	10.3390/sym13020313