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A Dark Energy Model in Lyra Manifold

Published 1 Apr 2012 in gr-qc | (1204.0774v2)

Abstract: We consider, in normal-gauge Lyra's geometry, evolution of a homogeneous isotropic universe in a gravitational model involving only the standard matter in interaction with a displacement vector field $\phi_{\mu}$. Considering both constant and time-dependent displacement vector field we show that the observed cosmic acceleration could be explained without considering an alien energy component with a negative pressure.

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