Phys. Rev. D 56, R6062–R6066 (1997)

Propagation of gravitational waves from slow motion sources in a Coulomb-type potential

Abstract

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Citing Articles (4)

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Hideki Asada
Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-01, Japan

Toshifumi Futamase
Astronomical Institute, Graduate School of Science, Tohoku University, Sendai 980-77, Japan

Received 13 August 1997; published in the issue dated 15 November 1997

We consider the propagation of gravitational waves generated by slow motion sources in a Coulomb-type potential due to the mass of the source. Then, the formula for a gravitational waveform including the tail is obtained in a straightforward manner by using the spherical Coulomb function. We discuss its relation with the formula in the previous work.

URL:

http://link.aps.org/doi/10.1103/PhysRevD.56.R6062

DOI:

10.1103/PhysRevD.56.R6062

PACS:

04.25.Nx, 04.30.Nk

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Phys. Rev. D 56, R6062–R6066 (1997)

Propagation of gravitational waves from slow motion sources in a Coulomb-type potential