Form of presentation | Articles in international journals and collections |
Year of publication | 2021 |
Язык | английский |
|
Popov Arkadiy Aleksandrovich, author
Rubin Sergey Georgievich, author
|
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Petriakova Polina , author
|
Bibliographic description in the original language |
P. Petriakova Sub-Planckian Scale and Limits for f(R) Models / Petriakova, P.; Popov, A.; Rubin, S. // Symmetry. - 2021. - V.13. - P.313. https://doi.org/10.3390/sym13020313 |
Annotation |
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. |
Keywords |
f(R) gravity, cosmology, Planck energies |
The name of the journal |
Symmetry
|
On-line resource for training course |
http://dspace.kpfu.ru/xmlui/bitstream/handle/net/160648/symmetry_13_00313.pdf?sequence=1&isAllowed=y
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URL |
https://www.mdpi.com/2073-8994/13/2/313 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=248735&p_lang=2 |
Resource files | |
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Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Popov Arkadiy Aleksandrovich |
ru_RU |
dc.contributor.author |
Rubin Sergey Georgievich |
ru_RU |
dc.contributor.author |
Petriakova Polina |
ru_RU |
dc.date.accessioned |
2021-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2021-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2021 |
ru_RU |
dc.identifier.citation |
P. Petriakova Sub-Planckian Scale and Limits for f(R) Models / Petriakova, P.; Popov, A.; Rubin, S. // Symmetry. - 2021. - V.13. - P.313. https://doi.org/10.3390/sym13020313 |
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=248735&p_lang=2 |
ru_RU |
dc.description.abstract |
Symmetry |
ru_RU |
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. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
f(R) gravity |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
Planck energies |
ru_RU |
dc.title |
Sub-Planckian Scale and Limits for f(R) Models |
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|