The Dynamical Instability of Static, Spherically Symmetric Solutions in Nonsymmetric Gravitational Theories
arXiv:gr-qc/9801085 · doi:10.1023/A:1018865125354
Abstract
We consider the dynamical stability of a class of static, spherically-symmetric solutions of the nonsymmetric gravitational theory. We numerically reproduce the Wyman solution and generate new solutions for the case where the theory has a nontrivial fundamental length scale μ^{-1}. By considering spherically symmetric perturbations of these solutions we show that the Wyman solutions are generically unstable.
13 pages, uses amslatex, graphicx and subfigure packages