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Spherical symmetry in $f(R)$-gravity

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arxiv 0709.0891 v2 pith:W5XQEO7Z submitted 2007-09-06 gr-qc astro-ph

classification gr-qcastro-ph
keywords solutionsconstantexactgravityobtainricciscalarspherical
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abstract

Spherical symmetry in $f(R)$ gravity is discussed in details considering also the relations with the weak field limit. Exact solutions are obtained for constant Ricci curvature scalar and for Ricci scalar depending on the radial coordinate. In particular, we discuss how to obtain results which can be consistently compared with General Relativity giving the well known post-Newtonian and post-Minkowskian limits. Furthermore, we implement a perturbation approach to obtain solutions up to the first order starting from spherically symmetric backgrounds. Exact solutions are given for several classes of $f(R)$ theories in both $R =$ constant and $R = R(r)$.

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Cited by 1 Pith paper

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  1. Propagating degrees of freedom on maximally-symmetric backgrounds in $f(R)$ theories of gravity

    gr-qc 2024-12 accept novelty 7.0 of 10

    For all degenerate f(R) models, the linearized spectrum on maximally symmetric backgrounds is empty: no graviton and no scalaron.

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