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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 |