Due to the failure of Birkhoff’s theorem, black holes in f (R) gravity theories in which an effective time-varying cosmological “constant” is present are, in general, dynamical. Clifton’s exact spherical solution of R1+δ gravity, which is dynamical and describes a central object embedded in a spatially flat universe, is studied. It is shown that apparent black hole horizons disappear and a naked singularity emerges at late times.
CITATION STYLE
Faraoni, V. (2011). Horizons and singularity in Clifton’s spherical solution of f (R) vacuum. In Springer Proceedings in Physics (Vol. 137, pp. 173–181). Springer Science and Business Media, LLC. https://doi.org/10.1007/978-3-642-19760-4_16
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