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We study a nonlocally modified gravity model proposed by Deser and Woodardwhich gives an explanation for current cosmic acceleration. By deriving andsolving the equations governing the evolution of the structure in the Universe,we show that this model predicts a pattern of growth that differs from standardgeneral relativity (+dark energy) at the 10-30% level. These differences willbe easily probed by the next generation of galaxy surveys, so the model shouldbe tested shortly.

Structure formation in a nonlocally modified gravity model