dc.contributor.author |
Ivanov G. |
|
dc.date.accessioned |
2018-09-14T20:58:11Z |
|
dc.date.available |
2018-09-14T20:58:11Z |
|
dc.date.issued |
1986 |
|
dc.identifier.issn |
0038-5697 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/132918 |
|
dc.description.abstract |
The structure of the Boltzmann and Vlasov Kinetic equations is considered for spatially uniform cosmological models taking into account the Einstein equations. A successive approximation technique is proposed for solving Boltzmann's equation at the intensely anisotropic vacuum stage of expansion for the type I Bianci cosmological model. It is shown that during the hadron stage the collisional gas can be found in a highly nonequilibrium state. © 1986 Plenum Publishing Corporation. |
|
dc.relation.ispartofseries |
Soviet Physics Journal |
|
dc.title |
Boltzmann and Vlasov kinetic equations in anisotropic cosmological models |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
5 |
|
dc.relation.ispartofseries-volume |
29 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
360 |
|
dc.source.id |
SCOPUS00385697-1986-29-5-SID0022710630 |
|