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

Hideki Asada and Toshifumi Futamase
Phys. Rev. D 56, R6062(R) – Published 15 November 1997
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Abstract

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.

  • Received 13 August 1997

DOI:https://doi.org/10.1103/PhysRevD.56.R6062

©1997 American Physical Society

Authors & Affiliations

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

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Vol. 56, Iss. 10 — 15 November 1997

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