Dynamics in nonlocal linear models in the Friedmann-Robertson-Walker metric

Abstract

A general class of cosmological models driven by a nonlocal scalar field inspired by the string field theory is studied. Using the fact that the considering linear nonlocal model is equivalent to an infinite number of local models we have found an exact special solution of the nonlocal Friedmann equations. This solution describes a monotonically increasing Universe with the phantom dark energy.

18 pages, 3 figures, a few misprints in Section 5 have been corrected

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