Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2016 |
Язык | русский |
|
Игнатьев Юрий Геннадиевич, автор
|
Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev. Macroscopic Einstein Equations for a Cosmological Model
with a λ Term //Gravitation and Cosmology, 2016, Vol. 22, No. 3, pp. 264–269.
|
Аннотация |
By averaging the Einstein equations over transverse gravitational perturbations we obtain a closed set of two ordinary differential equations describing the macroscopic cosmological evolution of the isotropic spatially flat Universe filled with gravitational radiation. We have found an asymptotic solution of the evolution equation for the gravitational perturbation amplitude. Substituting this solution to the Einstein equations averaged over gravitational perturbations, we obtain a single nonlinear ordinary differential second-order evolution equation with respect to the macroscopic scale factor. We have also found a solution of the evolution equation for the scale factor in the WKB approximation which analytically
describes the process of transformation from the ultrarelativistic mode of cosmological expansion to an inflationary one. |
Ключевые слова |
gravitation, cosmology, averaging, local fluctuations of metric, macroscopic Einsten Equations |
Название журнала |
Gravitation and Cosmology
|
URL |
http://link.springer.com/article/10.1134/S0202289316030075 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=133907 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
dc.date.accessioned |
2016-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2016-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2016 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignat'ev. Macroscopic Einstein Equations for a Cosmological Model
with a λ Term //Gravitation and Cosmology, 2016, Vol. 22, No. 3, pp. 264–269.
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=133907 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.abstract |
By averaging the Einstein equations over transverse gravitational perturbations we obtain a closed set of two ordinary differential equations describing the macroscopic cosmological evolution of the isotropic spatially flat Universe filled with gravitational radiation. We have found an asymptotic solution of the evolution equation for the gravitational perturbation amplitude. Substituting this solution to the Einstein equations averaged over gravitational perturbations, we obtain a single nonlinear ordinary differential second-order evolution equation with respect to the macroscopic scale factor. We have also found a solution of the evolution equation for the scale factor in the WKB approximation which analytically
describes the process of transformation from the ultrarelativistic mode of cosmological expansion to an inflationary one. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
gravitation |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
averaging |
ru_RU |
dc.subject |
local fluctuations of metric |
ru_RU |
dc.subject |
macroscopic Einsten Equations |
ru_RU |
dc.title |
Macroscopic Einstein Equations for a Cosmological Model
with a λ Term |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|