The Dynamical Instability of Static, Spherically Symmetric Solutions in Nonsymmetric Gravitational Theories
General Relativity and Quantum Cosmology
2010-11-19 v1
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 \mu^{-1}. By considering spherically symmetric perturbations of these solutions we show that the Wyman solutions are generically unstable.
Keywords
Cite
@article{arxiv.gr-qc/9801085,
title = {The Dynamical Instability of Static, Spherically Symmetric Solutions in Nonsymmetric Gravitational Theories},
author = {M. A. Clayton and L. Demopoulos and J. Legare},
journal= {arXiv preprint arXiv:gr-qc/9801085},
year = {2010}
}
Comments
13 pages, uses amslatex, graphicx and subfigure packages