Form of presentation | Conference proceedings in Russian journals and collections |
Year of publication | 2019 |
Язык | английский |
|
Ignatev Yuriy Gennadievich, author
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Bibliographic description in the original language |
Yu. G. Ignat'ev. The self-consistent field method and Einstein's macroscopic equations for the early Universe // 3rd Symposium of the BRICS Association on Gravity, Astrophysics and Cosmology. August, 29-September, 3 2019. Programm and Abstracts. Kazan. Kazanskiy universitet. 2019. – s. 40 |
Annotation |
3rd Symposium of the BRICS Association on Gravity, Astrophysics and Cosmology. August, 29-September, 3 2019. Programm and Abstracts. |
Keywords |
macroscopic gravity, self-consistent field, cosmological model, scalar fields, averaging of local fluctuations, asymptotic behavior, cosmological singularity |
The name of the journal |
3rd Symposium of the BRICS Association on Gravity, Astrophysics and Cosmology. August, 29-September, 3 2019. Programm and Abstracts.
|
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=206489&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.date.accessioned |
2019-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2019-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2019 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignat'ev. The self-consistent field method and Einstein's macroscopic equations for the early Universe // 3rd Symposium of the BRICS Association on Gravity, Astrophysics and Cosmology. August, 29-September, 3 2019. Programm and Abstracts. Kazan. Казанский университет. 2019. – с. 40 |
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=206489&p_lang=2 |
ru_RU |
dc.description.abstract |
3rd Symposium of the BRICS Association on Gravity, Astrophysics and Cosmology. August, 29-September, 3 2019. Programm and Abstracts. |
ru_RU |
dc.description.abstract |
Using the self-consistent field method, a complete theory of a macroscopic description of cosmological evolution is constructed, which includes a subsystem of linear equations of evolution of perturbations and nonlinear macroscopic equations of Einstein and a scalar field. Examples of the solution of this system are presented, illustrating the fundamental difference between the cosmological models of the early Universe built on homogeneous and locally fluctuating scalar fields. Corrections to the equation of state of the fluid are found,
based on the macroscopic Einstein equations which were obtained by averaging over microscopic
spherically symmetric metric fluctuations created by primordial black holes in a fluid medium.
It is shown that these corrections are effectively equivalent to addition to the system of a fluid
with the equation of state $p=-\varepsilon$. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
macroscopic gravity |
ru_RU |
dc.subject |
self-consistent field |
ru_RU |
dc.subject |
cosmological model |
ru_RU |
dc.subject |
scalar fields |
ru_RU |
dc.subject |
averaging of local fluctuations |
ru_RU |
dc.subject |
asymptotic behavior |
ru_RU |
dc.subject |
cosmological singularity |
ru_RU |
dc.title |
The self-consistent field method and Einstein's macroscopic equations for the early Universe |
ru_RU |
dc.type |
Conference proceedings in Russian journals and collections |
ru_RU |
|