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.
|ジャーナル||Physical Review D - Particles, Fields, Gravitation and Cosmology|
|出版ステータス||Published - 1997|
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