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Brane f(R)f(\cal R) gravity

Abstract

We consider a brane world scenario in which the bulk action is assumed to have the form of a generic function of the Ricci scalar f(R)f(\mathcal{R}) and derive the resulting Einstein field equations on the brane. In a constant curvature bulk a conserved geometric quantity appears in the field equations which can be associated with matter. We present cosmological and spherically symmetric solutions by assuming specific forms for f(R)f(\mathcal{R}) and show that the former can explain an accelerated expanding universe while the latter may account for galaxy rotation curves.Comment: 8 pages, 2 figures, to appear in EP

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