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 |
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 |
Annotation |
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. |
Keywords |
standart cosmologycal model, numeric gravitation, averaging |
The name of the journal |
Gravitation and Cosmology
|
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=178802&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 |
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/eng/?p_id=178802&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|