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

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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

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