Determinant-Gravity: Cosmological implications

Abstract

We analyze the action ∫ d4x || B gμ+ C Rμ|| as a possible alternative or addition to the Einstein gravity. Choosing a particular form of B(R)= R we can restore the Einstein gravity and, if B=m2, we obtain the cosmological constant term. Taking B = m2 + B1 R and expanding the action in 1/m2, we obtain as a leading term the Einstein Lagrangian with a cosmological constant proportional to m4 and a series of higher order operators. In general case of non-vanishing B and C new cosmological solutions for the Robertson-Walker metric are obtained.

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