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Stability of cosmological solutions in F(R) Horava-Lifshitz gravity · Around

2010

Stability of cosmological solutions in F(R) Horava-Lifshitz gravity

Sáez-Gómez, Diego

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At the present paper, it is studied cosmological solutions and its stability in the frame of F(R) Horava-Lifshitz gravity.

The perturbations around general spatially flat FRW solutions are analyzed and it is showed that the stability of those solutions will depend on the kind of theory, i.e.
on the form of the action F(R), as well as on the parameters contained in any Horava-Lifshitz theory due to the breaking of Lorentz invariance.
The (in)stability of a given cosmic solution can restrict the models and gives new observational predictions, and can give a natural explanation on the end of inflation and radiation/matter phases.

Built on

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S. Nojiri, S. D. Odintsov, arXiv:1011.0544 [gr-qc], arXiv:1008.4275 [hep-th], eConf C0602061
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2007
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S. Nojiri and S. D. Odintsov, Phys. Rev. D 77
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2008
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E. Elizalde and D. Sáez-Gómez, Phys. Rev. D 80
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2009
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G. Cognola, E. Elizalde, S. D. Odintsov, P. Tretyakov, and S Zerbini, Phys. Rev. D 79
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2009
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Nojiri S., Odintsov S.D., Sáez-Gómez D., Phys. Lett. B 681
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E. Elizalde, S. Nojiri, S. D. Odintsov and D. Sáez-Gómez, Unifying inflation with dark energy in modfied F(R) Hořava-Lifshitz gravity

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M. Chaichian, M. Oksanen, A. Tureanu, arXiv:1006.3235 [hep-th]

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