An asymptotic approximation of the Fokker-Planck model of evolution of superthermal ultrarelativistic particles in the presence of interaction scaling

dc.contributor.author	Ignat'ev Y.
dc.contributor.author	Ziatdinov P.
dc.date.accessioned	2018-09-18T20:16:28Z
dc.date.available	2018-09-18T20:16:28Z
dc.date.issued	2009
dc.identifier.issn	1064-8887
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/138194
dc.description.abstract	The evolution of a superthermal relict plasma component is studied using a nonequilibrium model of the Universe [1] and a kinetic equation of the Fokker-Planck type [2]. Given is the evidence of two maxima in the distribution of superthermal particles. The first maximum can further evolve into an equilibrium distribution, whereas the second one can result in a high-energy tail of superthermal relict particles. © 2009 Springer Science+Business Media, Inc.
dc.relation.ispartofseries	Russian Physics Journal
dc.subject	Cosmology
dc.subject	Gravitation theory
dc.subject	Relativistic kinetics
dc.subject	Scaling
dc.title	An asymptotic approximation of the Fokker-Planck model of evolution of superthermal ultrarelativistic particles in the presence of interaction scaling
dc.type	Article
dc.relation.ispartofseries-issue	2
dc.relation.ispartofseries-volume	52
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	210
dc.source.id	SCOPUS10648887-2009-52-2-SID71449113215

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