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

Authors
  • Elizalde, E.
  • Nojiri, S.
  • Odintsov, S. D.
  • Saez-Gomez, D.
Type
Published Article
Publication Date
Aug 19, 2010
Submission Date
Jun 17, 2010
Identifiers
DOI: 10.1140/epjc/s10052-010-1455-7
Source
arXiv
License
Yellow
External links

Abstract

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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