Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2018 |
Язык | русский |
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Игнатьев Юрий Геннадиевич, автор
Самигуллина Алсу Ринатовна, автор
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Библиографическое описание на языке оригинала |
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]
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Аннотация |
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. |
Ключевые слова |
standard cosmological model, averaging of invariant characteristics, mean value of the cosmological acceleration, stage of cosmological expansion, numerical gravitation |
Название журнала |
arXiv: General Relativity and Quantum Cosmology
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URL |
https://arxiv.org/abs/1808.05972 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=184128 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
dc.contributor.author |
Самигуллина Алсу Ринатовна |
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/?p_id=184128 |
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 |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|