Unifying inflation with dark energy in modified F(R) Horava-Lifshitz gravity

Details Unifying inflation with dark energy in modified F(R) Horava-Lifshitz gravity Unifying inflation with dark energy in modified F(R) Horava-Lifshitz gravity

2010-06-17

arxiv.org/abs/1006.3387v3

Eur.Phys.J.C70:351-361,2010

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX 12 pages, typos are corrected

Scientific paper

10.1140/epjc/s10052-010-1455-7

We study FRW cosmology for a non-linear modified F(R) Horava-Lifshitz gravity which has a viable convenient counterpart. A unified description of early-time inflation and late-time acceleration is possible in this theory, but the cosmological dynamic details are generically different from the ones of the convenient viable F(R) model. Remarkably, for some specific choice of parameters they do coincide. The emergence of finite-time future singularities is investigated in detail. It is shown that these singularities can be cured by adding an extra, higher-derivative term, which turns out to be qualitatively different when compared with the corresponding one of the convenient F(R) theory.

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