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Cosmological perfect-fluids in f(R) gravity

1 Pith paper cite this work, alongside 151 external citations. Polarity classification is still indexing.

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abstract

We show that an n-dimensional generalized Robertson-Walker (GRW) space-time with divergence-free conformal curvature tensor exhibits a perfect fluid stress-energy tensor for any f(R) gravity model. Furthermore we prove that a conformally flat GRW space-time is still a perfect fluid in both f(R) and quadratic gravity where other curvature invariants are considered.

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