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Paper detail

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

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.

preprint1998arXivOpen access
M. A. ClaytonL. DemopoulosJ. Legare
gr-qc
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M. A. ClaytonL. DemopoulosJ. Legare

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