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2007

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

Nojiri, Shin'ichi, Odintsov, Sergei D., Tretyakov, Petr V.

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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.

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

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S. Nojiri and S. D. Odintsov, arXiv:0707.1941[hep-th]
Original
1941
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Phys. Rev. D 68
2003
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Phys. Lett. B 599
2004
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G. Allemandi, A. Borowiec, M. Francaviglia, and S. D. Odintsov, Phys. Rev. D 72
2005
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S. Mukohyama and L. Randall, Phys. Rev. Lett. 92
2005
Earlier work this paper cites.

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W. Hu and I. Sawicki, arXiv:0705.1158[astro-ph]
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S. Appleby and R. A. Battye, arXiv:0705.3199[astro-ph]; L. Pogosian and A. Silvestri, arXiv:0709.0296[astro-ph]; S. Tsujikawa, arXiv:0709.1391[astro-ph]
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V. Faraoni, arXiv:0710.1291[gr-qc]
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O. Bertolami and J. Paramos, arXiv:0709.3988[astro-ph]
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S. Nojiri and S. D. Odintsov, arXiv:0710.1738[hep-th]
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S. Nojiri and S. D. Odintsov, arXiv:0708.0924[hep-th]
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Then

S. Nojiri and S. D. Odintsov, Phys. Lett. B 652
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2007
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G. Cognola, E. Elizalde, S. Nojiri, S. D. Odintsov, and S. Zerbini, Phys. Rev. D 73
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2007
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S. Nojiri, S. D. Odintsov, and P. Tretyakov, Phys. Lett. B 651
Original
2007
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S. Deser and R. Woodard, Phys. Rev. Lett. 99
2007
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V. Faraoni and S. Nadeau, Phys. Rev. D 75
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2007
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