dc.contributor.author | K. K. Yerzhanov | |
dc.contributor.author | P. Yu. Tsyba | |
dc.contributor.author | Sh. R. Myrzakul | |
dc.contributor.author | I. I. Kulnazarov | |
dc.contributor.author | R. Myrzakulov | |
dc.date.accessioned | 2013-04-18T04:52:43Z | |
dc.date.available | 2013-04-18T04:52:43Z | |
dc.date.issued | 2013-04-18 | |
dc.identifier.uri | http://dspace.enu.kz/handle/data/6840 | |
dc.description | http://www.enu.kz | ru_RU |
dc.description.abstract | In the present work we analyze the g-essence model for the particular Lagrangian: L = R + 2[αXn + ǫY − V (ψ, ¯ ψ)]. The g-essence models were proposed recently as an alternative and as a generalization to the scalar k-essence. We have presented the 3 types solutions of the g-essence model. We reconstructed the corresponding potentials and the dynamics of the scalar and fermionic fields according the evolution of the scale factor. The obtained results shows that the g-essence model can describes the decelerated and accelerated expansion phases of the univers | ru_RU |
dc.language.iso | en | ru_RU |
dc.subject | analyze | ru_RU |
dc.subject | essence | ru_RU |
dc.subject | Solutions | ru_RU |
dc.subject | reconstructed | ru_RU |
dc.title | Accelerated expansion of the Universe driven by G-essence | ru_RU |
dc.type | Article | ru_RU |