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

Wang, Charles H.-T. and Bonifacio, Paolo M. and Bingham, Robert and Mendonça, J. Tito (2011) Parametric instability induced scalar gravitational waves from a model pulsating neutron star. Modern Physics Letters B, 705 (1-2). pp. 148-151. ISSN 0217-9849 (https://doi.org/10.1016/j.physletb.2011.09.111)

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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.

ORCID iDs

Wang, Charles H.-T., Bonifacio, Paolo M., Bingham, Robert ORCID logoORCID: https://orcid.org/0000-0002-9843-7635 and Mendonça, J. Tito;