Parametric instability in scalar gravitational fields
arXiv:1309.4260 · doi:10.1142/S0217732312300236
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.
15 pages
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