Friday, January 4, 2013

0905.0706 (Charles H. -T. Wang et al.)

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

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