| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2020 |
| Язык | английский |
|
Игнатьев Юрий Геннадиевич, автор
|
| Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev. The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe // arXiv:2004.14865 [gr-qc]
|
| Аннотация |
The complete theory of cosmological evolution's macroscopic description is constructed with a help of self-consistent field. The theory includes a subsystem of linear equations of perturbations' evolution and nonlinear macroscopic Einstein equations and equations of a scalar field. We provide examples of system's solution which show the principal difference of the cosmological models of the early Universe built on homogenous and locally fluctuating scalar fields. {\bf Keywords}: macroscopic gravitation, self-consistent field, cosmological model, scalar fields, averaging of local fluctuations, asymptotical behavior, cosmological singularity. |
| Ключевые слова |
macroscopic gravitation, self-consistent field, cosmological model, scalar fields, averaging oflocal fluctuations, asymptotical behavior, cosmological singularity |
| Название журнала |
arXiv: General Relativity and Quantum Cosmology
|
| URL |
https://arxiv.org/pdf/2004.14865.pdf |
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=231060 |
Полная запись метаданных  |
| Поле DC |
Значение |
Язык |
| dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
| dc.date.accessioned |
2020-01-01T00:00:00Z |
ru_RU |
| dc.date.available |
2020-01-01T00:00:00Z |
ru_RU |
| dc.date.issued |
2020 |
ru_RU |
| dc.identifier.citation |
Yu. G. Ignat'ev. The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe // arXiv:2004.14865 [gr-qc]
|
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=231060 |
ru_RU |
| dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
ru_RU |
| dc.description.abstract |
The complete theory of cosmological evolution's macroscopic description is constructed with a help of self-consistent field. The theory includes a subsystem of linear equations of perturbations' evolution and nonlinear macroscopic Einstein equations and equations of a scalar field. We provide examples of system's solution which show the principal difference of the cosmological models of the early Universe built on homogenous and locally fluctuating scalar fields. {\bf Keywords}: macroscopic gravitation, self-consistent field, cosmological model, scalar fields, averaging of local fluctuations, asymptotical behavior, cosmological singularity. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
macroscopic gravitation |
ru_RU |
| dc.subject |
self-consistent field |
ru_RU |
| dc.subject |
cosmological model |
ru_RU |
| dc.subject |
scalar fields |
ru_RU |
| dc.subject |
averaging oflocal fluctuations |
ru_RU |
| dc.subject |
asymptotical behavior |
ru_RU |
| dc.subject |
cosmological singularity |
ru_RU |
| dc.title |
The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe |
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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