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Non-minimal coupling influence on the deviation from de Sitter cosmological expansion

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arxiv 1711.06870 v3 pith:UNSU4E2U submitted 2017-11-18 gr-qc

Igor V. Fomin , Sergey V. Chervon This is my paper · ORCID
classification gr-qc
keywords cosmologicaldeviationdynamicssitterapproachcaseconsidercoupling
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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.

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  1. Corrections to inflationary models induced by non-minimal coupling between scalar field and curvature

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Power-law non-minimal coupling F=(H/λ)^{2n} deforms inflationary potentials, shifts r and n_S while preserving n_T=-r/8 and GR-like reheating, enabling r(1-n_S) classification of models against Planck/ACT data.

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