Parametric instability induced scalar gravitational waves from a model pulsating neutron star
General Relativity and Quantum Cosmology
2013-01-04 v2 High Energy Astrophysical Phenomena
Abstract
We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.
Cite
@article{arxiv.0905.0706,
title = {Parametric instability induced scalar gravitational waves from a model pulsating neutron star},
author = {Charles H. -T. Wang and Paolo M. Bonifacio and Robert Bingham and J. Tito Mendonca},
journal= {arXiv preprint arXiv:0905.0706},
year = {2013}
}
Comments
4 pages, published version