Kinetic theory of the generation of magnetic fields in the radiation-dominated stage of expansion of the universe

dc.contributor.author	Zakharov A.
dc.contributor.author	Anikanov V.
dc.date.accessioned	2018-09-17T21:49:12Z
dc.date.available	2018-09-17T21:49:12Z
dc.date.issued	1992
dc.identifier.issn	0038-5697
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/135474
dc.description.abstract	The system of linearized Einstein and Maxwell equations and a kinetic equation with model collision integral for the cosmological plasma are used to calculate the magnetic field generated by solenoidal perturbations in the radiation-dominated stage of expansion of the universe. The magnetic field is generated by two effects - the Harrison effect and a new effect due to kinetic processes. The second effect contributes to the magnetic field if solenoidal gravitational perturbations exist from the very beginning of the radiation-dominated stage. © 1992 Plenum Publishing Corporation.
dc.relation.ispartofseries	Soviet Physics Journal
dc.title	Kinetic theory of the generation of magnetic fields in the radiation-dominated stage of expansion of the universe
dc.type	Article
dc.relation.ispartofseries-issue	1
dc.relation.ispartofseries-volume	35
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	98
dc.source.id	SCOPUS00385697-1992-35-1-SID34249841352

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