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 |
|