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.
Original language | English |
---|---|
Pages (from-to) | 148-151 |
Number of pages | 4 |
Journal | Physics Letters B |
Volume | 705 |
Issue number | 1-2 |
DOIs | |
Publication status | Published - 3 Nov 2011 |
Keywords
- scalar-tensor gravity
- scalar waves
- pulsating stars
- general relativity
- dynamical analysis