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

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

1998-01-26

arxiv.org/abs/gr-qc/9801085v1

Gen.Rel.Grav.30:1501-1520,1998

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, uses amslatex, graphicx and subfigure packages

Scientific paper

10.1023/A:1018865125354

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 \mu^{-1}. By considering spherically symmetric perturbations of these solutions we show that the Wyman solutions are generically unstable.

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