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
Full text not available in this repository. (Request a copy from the Strathclyde author)Official URL: http://dx.doi.org/10.1016/j.physletb.2011.09.111
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.
| Item type: | Article |
|---|---|
| ID code: | 36053 |
| Keywords: | scalar-tensor gravity, scalar waves, pulsating stars, general relativity, parametric instability, scalar gravitational waves, model, Physics |
| Subjects: | Science > Physics |
| Department: | Faculty of Science > Physics |
| Related URLs: | |
| Depositing user: | Pure Administrator |
| Date Deposited: | 22 Nov 2011 14:15 |
| Last modified: | 04 Oct 2012 14:07 |
| URI: | http://strathprints.strath.ac.uk/id/eprint/36053 |
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