Parametric instability induced scalar gravitational waves from a model
pulsating neutron star [PDF]
Charles H. -T. Wang, Paolo M. Bonifacio, Robert Bingham, J. Tito MendoncaWe 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.View original: http://arxiv.org/abs/0905.0706
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