Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2017 |
Язык | русский |
|
Игнатьев Дмитрий Юрьевич, автор
Игнатьев Юрий Геннадиевич, автор
Самигуллина Алсу Ринатовна, автор
|
Библиографическое описание на языке оригинала |
Yu.G. Ignat'ev, D.Yu. Ignatyev, A.R. Samigullina. A macroscopic view to the standard cosmological model //arXiv:1705.05000[gr-qc]
|
Аннотация |
The averaging of the dynamic functions of the standard cosmological model (SCM) at its early stage with the dominance of the scalar field is carried out. It is shown that microscopic oscillations with Compton period provide the major contribution to the macroscopic energy density of the scalar field at large times at this stage. In this case, the effective equation of state of the scalar field oscillates between the inflationary and the extremely rigid ones, while the macroscopic equation of state is non-relativistic. |
Ключевые слова |
standard cosmological model, macroscopic averaging, fast
oscillations, numerical simulation, numerical gravitation. |
Название журнала |
ArXiv[gr-qc]
|
URL |
https://arxiv.org/abs/1705.05000 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=157420 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Игнатьев Дмитрий Юрьевич |
ru_RU |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
dc.contributor.author |
Самигуллина Алсу Ринатовна |
ru_RU |
dc.date.accessioned |
2017-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2017-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2017 |
ru_RU |
dc.identifier.citation |
Yu.G. Ignat'ev, D.Yu. Ignatyev, A.R. Samigullina. A macroscopic view to the standard cosmological model //arXiv:1705.05000[gr-qc]
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=157420 |
ru_RU |
dc.description.abstract |
ArXiv[gr-qc] |
ru_RU |
dc.description.abstract |
The averaging of the dynamic functions of the standard cosmological model (SCM) at its early stage with the dominance of the scalar field is carried out. It is shown that microscopic oscillations with Compton period provide the major contribution to the macroscopic energy density of the scalar field at large times at this stage. In this case, the effective equation of state of the scalar field oscillates between the inflationary and the extremely rigid ones, while the macroscopic equation of state is non-relativistic. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
standard cosmological model |
ru_RU |
dc.subject |
macroscopic averaging |
ru_RU |
dc.subject |
fast
oscillations |
ru_RU |
dc.subject |
numerical simulation |
ru_RU |
dc.subject |
numerical gravitation. |
ru_RU |
dc.title |
Yu.G. Ignat'ev, D.Yu. Ignatyev, A.R. Samigullina. A macroscopic view to the standard cosmological model //arXiv:1705.05000[gr-qc] |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|