Screening the Cosmological Constant in non-local gravity

2012

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Abstract: (Grobid)
In this paper, we consider a class of model of non-local gravity with a largebare cosmological constant, Λ, and study its cosmological solutions. In theabsence of matter, we find a power-law expanding universe solution a ∝ t n withn < 1, that is, a universe with decelarated expansion without any fine-tuning ofthe parameter. So the effect of the cosmological constant is effectivelyscreened in this solution. Also it is found that the solution is ghost-free fora very wide range of parameters. Thus our solution opens up new possibilitiesfor solution to the cosmological constant problem.