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dc.contributor.author | Balakin A. | |
dc.contributor.author | Bochkarev V. | |
dc.contributor.author | Tarasova N. | |
dc.date.accessioned | 2018-09-18T20:22:34Z | |
dc.date.available | 2018-09-18T20:22:34Z | |
dc.date.issued | 2012 | |
dc.identifier.issn | 1434-6044 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/139230 | |
dc.description.abstract | We establish an extended version of the Einstein-Maxwell-axion model by introducing into the Lagrangian cross-terms, which contain the gradient four-vector of the pseudoscalar (axion) field in convolution with the Maxwell tensor. The gradient model of the axion-photon coupling is applied to cosmology: we analyze the Bianchi-I type Universe with an initial magnetic field, electric field induced by the axion-photon interaction, cosmological constant and dark matter, which is described in terms of the pseudoscalar (axion) field. Analytical, qualitative and numerical results are presented in detail for two distinguished epochs: first, for the early Universe with magnetic field domination; second, for the stage of late-time accelerated expansion. © Springer-Verlag / Società Italiana di Fisica 2012. | |
dc.relation.ispartofseries | European Physical Journal C | |
dc.title | Gradient models of the axion-photon coupling | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 2 | |
dc.relation.ispartofseries-volume | 72 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 1 | |
dc.source.id | SCOPUS14346044-2012-72-2-SID84856801880 |