Kinetics of small disturbances in an isotropic universe I. Derivation of the equations for the disturbances

Zakharov A.

dc.contributor.author	Zakharov A.
dc.date.accessioned	2018-09-14T20:55:55Z
dc.date.available	2018-09-14T20:55:55Z
dc.date.issued	1978
dc.identifier.issn	0038-5697
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/132870
dc.description.abstract	Gravitational disturbances in an isotropic cosmological model are considered within the bounds of relativistic kinetic theory. It is assumed that the collision frequency of the particles of the medium is much smaller than the frequency of the disturbances being studied. Equations are obtained for scalar, vector, and tensor disturbances in the case where the undisturbed solution describes a flat, isotropic cosmological model. © 1978 Plenum Publishing Corporation.
dc.relation.ispartofseries	Soviet Physics Journal
dc.title	Kinetics of small disturbances in an isotropic universe I. Derivation of the equations for the disturbances
dc.type	Article
dc.relation.ispartofseries-issue	3
dc.relation.ispartofseries-volume	21
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	289
dc.source.id	SCOPUS00385697-1978-21-3-SID33744702522