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In this paper it has been shown that the neutrino bulk viscous stresses cangive rise to the late time acceleration of the universe. It is found that anumber of spatially flat FRW models with a negative deceleration parameter canbe constructed using neutrino viscosity and one of them mimics a $\Lambda$CDMmodel. This does not require any exotic dark energy component or anymodification of gravity.

Can neutrino viscosity drive the late time cosmic acceleration?