Показать сокращенную информацию
dc.contributor.author | Zimdahl W. | |
dc.contributor.author | Balakin A. | |
dc.date.accessioned | 2018-09-17T20:04:00Z | |
dc.date.available | 2018-09-17T20:04:00Z | |
dc.date.issued | 1999 | |
dc.identifier.issn | 0001-7701 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/132982 | |
dc.description.abstract | We show that a relativistic gas may be at "global" equilibrium in the expanding universe for any equation of state 0 < p ≤ ρ/3, provided that the gas particles move under the influence of a self-interacting, effective one-particle force in between elastic binary collisions. In the force-free limit we recover the equilibrium conditions for ultrarelativistic matter which imply the existence of a conformal timelike Killing vector. | |
dc.relation.ispartofseries | General Relativity and Gravitation | |
dc.subject | Acting gas | |
dc.subject | Boltzmann equation | |
dc.subject | Conformal symmetry | |
dc.subject | Self-inter | |
dc.title | Thermodynamic equilibrium in the expanding universe | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 9 | |
dc.relation.ispartofseries-volume | 31 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 1395 | |
dc.source.id | SCOPUS00017701-1999-31-9-SID0033246793 |