Form of presentation | Articles in international journals and collections |
Year of publication | 2020 |
Язык | английский |
|
Ignatev Yuriy Gennadievich, author
|
Bibliographic description in the original language |
Yu. G. Ignat'ev. The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe // arXiv:2004.14865 [gr-qc]
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Annotation |
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. |
Keywords |
macroscopic gravitation, self-consistent field, cosmological model, scalar fields, averaging oflocal fluctuations, asymptotical behavior, cosmological singularity |
The name of the journal |
arXiv: General Relativity and Quantum Cosmology
|
URL |
https://arxiv.org/pdf/2004.14865.pdf |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=231060&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
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/eng/?p_id=231060&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|