Form of presentation | Articles in international journals and collections |
Year of publication | 2018 |
Язык | русский |
|
Ignatev Yuriy Gennadievich, author
Samigullina Alsu Rinatovna, author
|
Bibliographic description in the original language |
Yurii Ignat'ev, A. R. Samigullina. Averaging of the Equations of the Standard Cosmological Model over Rapid Oscillations: Influence of the cosmological term on the mean value of the effective barotropic coefficient // arXiv:1808.05972 [gr-qc]
|
Annotation |
With the help of an applied software package written by the authors, we have averaged the effective total barotropic coefficient κ=(−λ+p)/(λ+ϵ) of the classical scalar field and the cosmological term and have shown that during cosmological evolution for sufficiently large values of the cosmological constant the Universe transitions from the inflationary stage to a nonrelativistic stage, and then, after a plateau, it transitions to a later inflationary stage. |
Keywords |
standard cosmological model, averaging of invariant characteristics, mean value of the cosmological acceleration, stage of cosmological expansion, numerical gravitation |
The name of the journal |
arXiv: General Relativity and Quantum Cosmology
|
URL |
https://arxiv.org/abs/1808.05972 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=184128&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.contributor.author |
Samigullina Alsu Rinatovna |
ru_RU |
dc.date.accessioned |
2018-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2018-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2018 |
ru_RU |
dc.identifier.citation |
Yurii Ignat'ev, A. R. Samigullina. Averaging of the Equations of the Standard Cosmological Model over Rapid Oscillations: Influence of the cosmological term on the mean value of the effective barotropic coefficient // arXiv:1808.05972 [gr-qc]
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=184128&p_lang=2 |
ru_RU |
dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
ru_RU |
dc.description.abstract |
With the help of an applied software package written by the authors, we have averaged the effective total barotropic coefficient κ=(−λ+p)/(λ+ϵ) of the classical scalar field and the cosmological term and have shown that during cosmological evolution for sufficiently large values of the cosmological constant the Universe transitions from the inflationary stage to a nonrelativistic stage, and then, after a plateau, it transitions to a later inflationary stage. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
standard cosmological model |
ru_RU |
dc.subject |
averaging of invariant characteristics |
ru_RU |
dc.subject |
mean value of the cosmological acceleration |
ru_RU |
dc.subject |
stage of cosmological expansion |
ru_RU |
dc.subject |
numerical gravitation |
ru_RU |
dc.title |
Yurii Ignat'ev, A. R. Samigullina. Averaging of the Equations of the Standard Cosmological Model over Rapid Oscillations: Influence of the cosmological term on the mean value of the effective barotropic coefficient // arXiv:1808.05972 [gr-qc] |
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|