Abstract

We discuss a possible mechanism to screen a cosmological constant in non-local gravity. We find that in a simple model of of non-local gravity with the Lagrangian of the form, R+f(□−1R)−2ΛR+f(\Box^{-1}R)-2Λ where f(X)f(X) is a quadratic function of XX, there is a flat spacetime solution despite the presence of the cosmological constant ΛΛ. Unfortunately, however, we also find that this solution contains a ghost in general. Then we discuss the condition to avoid a ghost and find that one can avoid it only for a finite range of `time'. Nevertheless our result suggests the possibility of solving the cosmological constant problem in the context of non-local gravity.

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