Clifton's spherical solution in f(R) vacuo harbours a naked singularity
classification
🌀 gr-qc
astro-ph.COhep-th
keywords
singularitycliftonharboursnakedsolutionsphericalasymptoticallydelta
read the original abstract
Clifton's exact solution of f(R)=R^(1+\delta) gravity describing a dynamical spherical metric which is asymptotically Friedmann-Lemaitre-Robertson-Walker is studied. It is shown that it harbours a strong spacetime singularity and that this singularity is naked at late times.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.