Parametric instability in scalar gravitational fields
General Relativity and Quantum Cosmology
2013-09-18 v1
Abstract
We present a brief review on a new dynamical mechanism for a strong field effect in scalar tensor theory. Starting with a summary of the essential features of the theory and subsequent work by several authors, we analytically investigate the parametric excitation of a scalar gravitational field in a spherically symmetric radially pulsating neutron star.
Cite
@article{arxiv.1309.4260,
title = {Parametric instability in scalar gravitational fields},
author = {T. B. Davies and C. H. -T. Wang and R. Bingham and J. T. Mendonca},
journal= {arXiv preprint arXiv:1309.4260},
year = {2013}
}
Comments
15 pages