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dc.contributor.author | Ignatyev Y. | |
dc.contributor.author | Ignatyev D. | |
dc.date.accessioned | 2018-09-18T20:07:08Z | |
dc.date.available | 2018-09-18T20:07:08Z | |
dc.date.issued | 2014 | |
dc.identifier.issn | 0202-2893 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/136676 | |
dc.description.abstract | © 2014, Pleiades Publishing, Ltd. Based on one the authors’ approach to a macroscopic description of the scalar interaction, we develop a macroscopic model of a relativistic plasma with a phantom scalar interaction of elementary particles. In this model, as opposed to previous models, the restriction of nonnegativity of the particles’ effective mass is removed. | |
dc.relation.ispartofseries | Gravitation and Cosmology | |
dc.title | Statistical systems with phantom scalar interaction in gravitation theory. I. Microscopic dynamics | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 4 | |
dc.relation.ispartofseries-volume | 20 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 299 | |
dc.source.id | SCOPUS02022893-2014-20-4-SID84911926914 |