From inflation to dark energy in the non-minimal modified gravity

Abstract

We consider the modified gravity non-minimally coupled with matter Lagrangian for the description of early-time and late-time universe. Such $F(R)$ ($F(G)$) gravity in the absence of non-minimal coupling is viable theory which passes the local tests and reproduces the $\Lambda$CDM era. For qualitatively similar choice of non-minimal gravitational coupling function it is shown that the unified description of early-time inflation and late-time cosmic acceleration is possible. It is interesting that matter (scalar) which supports the inflationary era is gravitationally screened at late times. Hence, it may be effectively invisible at current universe.

LaTeX file, 10 pages, based on the talk given by S.D. Odintsov at ICGA8 conference, Nara, Japan

Cited by in corpus (5)

• Construction of cosmologically viable f(G) gravity models
• Initial and final de Sitter universes from modified $f(R)$ gravity
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• Delicate f(R) gravity models with disappearing cosmological constant and observational constraints on the model parameters
• Cosmic acceleration and crossing of $\omega =-1$ in non-minimal modified Gauss-Bonnet gravity