Form of presentation | Articles in international journals and collections |
Year of publication | 2017 |
Язык | русский |
|
Ignatev Dmitriy Yurevich, author
Ignatev Yuriy Gennadievich, author
Samigullina Alsu Rinatovna, author
|
Bibliographic description in the original language |
Yu.G. Ignat'ev, D.Yu. Ignatyev, A.R. Samigullina. A macroscopic view to the standard cosmological model //arXiv:1705.05000[gr-qc]
|
Annotation |
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. |
Keywords |
standard cosmological model, macroscopic averaging, fast
oscillations, numerical simulation, numerical gravitation. |
The name of the journal |
ArXiv[gr-qc]
|
URL |
https://arxiv.org/abs/1705.05000 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=157420&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Dmitriy Yurevich |
ru_RU |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.contributor.author |
Samigullina Alsu Rinatovna |
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/eng/?p_id=157420&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|