Non-minimal coupling influence on the deviation from de Sitter cosmological expansion
arXiv:1711.06870 · doi:10.1140/epjc/s10052-018-6409-5
Abstract
We investigate the models of cosmological inflation in generalized scalar-tensor gravity, which we consider as a source of deviation from de Sitter dynamics in the case of GR. Within the framework of the proposed approach, the exact equations of cosmological dynamics and parameters of cosmological perturbations are obtained.
14 pages
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Cited by in corpus (6)
- Gauss-Bonnet term corrections in scalar field cosmology
- Reconstruction of GR cosmological solutions in modified gravity theories
- Exact and slow-roll solutions for exponential power-law inflation connected with f(R) gravity and observational constraints
- Generalized scalar-tensor theory of gravity reconstruction from physical potentials of a scalar field
- New method of exponential potentials reconstruction based on given scale factor in phantonical two-field models
- The scalar-torsion gravity corrections in the first-order inflationary models