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Cosmological parameters of f(R) gravity with kinetic scalar curvature
Author(s) -
S. V. Chervon,
И. В. Фомин,
T. I. Mayorova,
Alexandra Khapaeva
Publication year - 2020
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1557/1/012016
Subject(s) - physics , curvature , scalar field , scalar curvature , scalar (mathematics) , f(r) gravity , inflation (cosmology) , mathematical physics , kinetic energy , kinetic term , theoretical physics , parametric statistics , classical mechanics , geometry , quantum mechanics , mathematics , quantum gravity , statistics , quantum
We study modified f ( R ) gravity theory with kinetic scalar curvature reducible to chiral cosmological model of a special type. New method of cosmological parameters calculation based on reduction of two-fields model to standard one with single scalar field is proposed. Parametric correspondence to observational data is shown for massive scalar field, power-law and intermediate inflation.

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