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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 |