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 |
Yu. G. Ignat'ev, D. Yu. Ignatyev, and A. R. Samigullina A Macroscopic View of the Standard Cosmological Model //Gravitation and Cosmology, 2018, Vol. 24, No. 2, pp. 148–153 |
Аннотация |
Averaging of the dynamic functions of the standard cosmological model (SCM) at its early stage with the dominance of a scalar field is carried out. It is shown that microscopic oscillations with Compton period provide a 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, obtained by averaging over fast oscillations of the scalar field, is nonrelativistic. |
Ключевые слова |
standart cosmologycal model, numeric gravitation, averaging |
Название журнала |
Gravitation and Cosmology
|
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=178802 |
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 |
Yu. G. Ignat'ev, D. Yu. Ignatyev, and A. R. Samigullina A Macroscopic View of the Standard Cosmological Model //Gravitation and Cosmology, 2018, Vol. 24, No. 2, pp. 148–153 |
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=178802 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.abstract |
Averaging of the dynamic functions of the standard cosmological model (SCM) at its early stage with the dominance of a scalar field is carried out. It is shown that microscopic oscillations with Compton period provide a 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, obtained by averaging over fast oscillations of the scalar field, is nonrelativistic. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
standart cosmologycal model |
ru_RU |
dc.subject |
numeric gravitation |
ru_RU |
dc.subject |
averaging |
ru_RU |
dc.title |
Yu. G. Ignat'ev, D. Yu. Ignatyev, and A. R. Samigullina A Macroscopic View of the Standard Cosmological Model //Gravitation and Cosmology, 2018, Vol. 24, No. 2, pp. 148–153 |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|