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The Dynamical Instability of Static, Spherically Symmetric Solutions in Nonsymmetric Gravitational Theories

M. A. Clayton·L. Demopoulos·J. Legare
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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.

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M. A. Clayton, L. Demopoulos, J. Legare. 1998-01-26. The Dynamical Instability of Static, Spherically Symmetric Solutions in Nonsymmetric Gravitational Theories. https://doi.org/10.1023/a%3A1018865125354

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