Abstract
The diffraction effects on gravitational waves propagating through a stellar cluster are analyzed in the relevant approximation of Fresnel diffraction limit. We find that a gravitational wave scintillation effect - similar to the radio source scintillation effect - comes out naturally, implying that the gravitational wave intensity changes in a characteristic way as the observer moves.
| Original language | English |
|---|---|
| Pages (from-to) | 1937-1945 |
| Number of pages | 9 |
| Journal | International Journal of Modern Physics D |
| Volume | 15 |
| Issue number | 11 |
| DOIs | |
| State | Published - Nov 2006 |
Keywords
- Gravitational waves
ASJC Scopus subject areas
- Mathematical Physics
- Astronomy and Astrophysics
- Space and Planetary Science