Parametric instability induced scalar gravitational waves from a model pulsating neutron star
classification
🌀 gr-qc
astro-ph.HE
keywords
gravitationalscalarmechanismmodelneutronparametricpulsatingstar
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.