dc.contributor.author |
Balakin A. |
|
dc.contributor.author |
Dehnen H. |
|
dc.contributor.author |
Zayats A. |
|
dc.date.accessioned |
2018-09-18T20:07:15Z |
|
dc.date.available |
2018-09-18T20:07:15Z |
|
dc.date.issued |
2008 |
|
dc.identifier.issn |
0218-2718 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/136698 |
|
dc.description.abstract |
We establish a nonminimal Einstein-Yang-Mills-Higgs model, which contains six coupling parameters. The first three parameters relate to the nonminimal coupling of a non-Abelian gauge field and a gravity field, the next two parameters describe the so-called derivative nonminimal coupling of a scalar multiplet with a gravity field, and the sixth parameter introduces the standard coupling of a scalar field with a Ricci scalar. The formulated six-parameter nonminimal Einstein-Yang-Mills-Higgs model is applied to cosmology. We show that there exists a unique exact cosmological solution of the de Sitter type for a special choice of the coupling parameters. The nonminimally extended Yang-Mills and Higgs equations are satisfied for arbitrary gauge and scalar fields, when the coupling parameters are specifically related to the curvature constant of the isotropic space-time. Based on this special exact solution, we discuss the problem of a hidden anisotropy of the Yang-Mills field, and give an explicit example, when the nonminimal coupling effectively screens the anisotropy induced by the Yang-Mills field and thus restores the isotropy of the model. © 2008 World Scientific Publishing Company. |
|
dc.relation.ispartofseries |
International Journal of Modern Physics D |
|
dc.subject |
Isotropic cosmological model |
|
dc.subject |
Nonminimal interaction |
|
dc.subject |
Yang-Mills-Higgs theory |
|
dc.title |
Nonminimal isotropic cosmological model with yang-mills and higgs fields |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
8 |
|
dc.relation.ispartofseries-volume |
17 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
1255 |
|
dc.source.id |
SCOPUS02182718-2008-17-8-SID51049089706 |
|