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 |
|