Ricci dark energy in Chern-Simons modified gravity

Published 27 Jun 2013 in hep-th and gr-qc | (1306.6638v1)

Abstract: In this work, we have considered the Ricci dark energy model, where the energy density of the universe is proportional to the Ricci scalar curvature, in the dynamic Chern-Simons modified gravity. We show that in this context the evolution of the scale factor is similar to that displayed by the modified Chaplygin gas.

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