| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8191672 | Physics Letters B | 2011 | 4 Pages |
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.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Charles H.-T. Wang, Paolo M. Bonifacio, Robert Bingham, J. Tito Mendonça,