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      Simultaneous expansion and rotation of shear-free universes in modified gravity

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          Abstract

          We show in a fully covariant way that, there exist a class of \(f(R)\) models for which a shear-free, almost FLRW universe can expand and rotate at the same time .

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          On Shear-free perturbations of f(R) gravity

          Recently it was shown that if the matter congruence of a general relativistic perfect fluid flow in an almost FLRW universe is shear-free, then it must be either expansion or rotation-free. Here we generalize this result for a general f(R) theory of gravity and show there exist scenarios where this result can be avoided. This suggests that there are situations where linearized forth-order gravity shares properties with Newtonian theory not valid in General Relativity.
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            Author and article information

            Journal
            17 February 2012
            Article
            10.1063/1.4734421
            1202.3864
            4324fd60-0ff1-4565-ac43-75b6230e33d9

            http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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            4 pages, no figures. Contribution submitted to the proceedings of the Spanish Relativity Meeting ERE2011, September 2011, Madrid, Spain
            gr-qc hep-th

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