Stability analysis of black holes in massive gravity: a unified treatment
arXiv:1401.6871 · doi:10.1103/PhysRevD.89.081502
Abstract
We consider the analytic solutions of massive (bi)gravity which can be written in a simple form using advanced Eddington-Finkelstein coordinates. We analyse the stability of these solutions against radial perturbations. First we recover the previously obtained result on the instability of the bidiagonal bi-Schwarzschild solutions. In the non-bidiagonal case (which contains, in particular, the Schwarzschild solution with Minkowski fiducial metric) we show that generically there are physical spherically symmetric perturbations, but no unstable modes.
4 pages; v2: matches the published version
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Cited by in corpus (37)
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