Astronomy and Astrophysics – Astrophysics
Scientific paper
1992-12-23
Phys.Rev.Lett.70:1572-1575,1993
Astronomy and Astrophysics
Astrophysics
RevTeX, 11pp, UU-HEP-92/11
Scientific paper
10.1103/PhysRevLett.70.1572
We consider a compact source of gravitational waves of frequency $\omega$, in or near a massive spherically symmetric distribution of matter or a black hole. Recent calculations have led to apparently contradictory results for the influence of the massive body on the propagation of the waves. We show here that the results are in fact consistent and in agreement with the ``standard'' viewpoint in which the high frequency compact source produces the radiation as if in a flat background, and the background curvature affects the propagation of these waves.
Kundu Prasun
Price Richard H.
Pullin Jorge
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