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

Abstract

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

13 pages, no figures, to be published in Phys. Rev. D

References in corpus (5)

• Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order
• Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections
• Binary inspiral, gravitational radiation, and cosmology
• Second-post-Newtonian generation of gravitational radiation
• Gravitational Lensing of Gravitational Waves from Merging Neutron Star Binaries

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