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Accelerating cosmology in modified gravity with scalar field
Authors:Yulia?A.?Shaido  author-information"  >  author-information__contact u-icon-before"  >  mailto:Shaido@ngs.ru"   title="  Shaido@ngs.ru"   itemprop="  email"   data-track="  click"   data-track-action="  Email author"   data-track-label="  "  >Email author,Akio?Sugamoto
Affiliation:(1) Laboratory for Fundamental Studies, Tomsk State Pedagogical University, 634041 Tomsk, Russia;(2) Department of Physics and Chemistry, Graduate School of Humanities and Sciences, Ochanomizu University, Japan;(3) Department of Physics, Faculty of Science, Ochanomizu University, 1-1 Otsuka 2, Bunkyo-ku, Tokyo 112-8610, Japan
Abstract:The modified gravity with 1/R term (R being the scalar curvature) and the Einstein-Hilbert term is studied by incorporating the phantom scalar field. A number of cosmological solutions are derived in the presence of the phantom field in the perfect fluid background. It is shown: the current inflation obtained in the modified gravity is affected by the existence of the phantom field.
Keywords:Nonlinear gravity  Cosmology
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