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arXiv · 0905.0706

Parametric instability induced scalar gravitational waves from a model pulsating neutron star

Charles H. -T. Wang·Paolo M. Bonifacio·Robert Bingham·J. Tito Mendonca
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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.

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Charles H. -T. Wang, Paolo M. Bonifacio, Robert Bingham, J. Tito Mendonca. 2009-05-06. Parametric instability induced scalar gravitational waves from a model pulsating neutron star. https://doi.org/10.1016/j.physletb.2011.09.111

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