Transport coefficients and equations of hydrodynamics for the radiation-dominated cosmological plasma

dc.contributor.author	Zakharov A.
dc.contributor.author	Malanichev I.
dc.date.accessioned	2018-09-14T20:59:42Z
dc.date.available	2018-09-14T20:59:42Z
dc.date.issued	1990
dc.identifier.issn	0038-5697
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/132929
dc.description.abstract	Using relativistic kinetic theory, the hydrodynamics equations are obtained for a mixture of electrons, protons, and photons, which interact by Compton scattering and Coulomb collisions. We assume that the electrons and protons are nonrelativistic, and their concentrations are much lower than that of the photons. The obtained equations are applicable for a description of cosmological plasma in the temperature range of 4·103 K < T ≪ 6·109 K. © 1990 Plenum Publishing Corporation.
dc.relation.ispartofseries	Soviet Physics Journal
dc.title	Transport coefficients and equations of hydrodynamics for the radiation-dominated cosmological plasma
dc.type	Article
dc.relation.ispartofseries-issue	5
dc.relation.ispartofseries-volume	33
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	412
dc.source.id	SCOPUS00385697-1990-33-5-SID34249929574

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.