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

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

2009-05-06

arxiv.org/abs/0905.0706v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, 1 figure

Scientific paper

We identify a new dynamical mechanism for a strong scalar gravitational field
effect. To illustrate this mechanism, we analytically and numerically
investigate the parametric excitation and emission of scalar gravitational
waves by a radially pulsating model neutron star.

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