Tail of Gravitational Radiation and Coulomb Final-State Interaction

Abstract

We present a simple intuitive derivation of the corrections to the intensity of gravitational radiation due to the so-called tail effect.

4 pages, latex

References in corpus (1)

• Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole

Cited by in corpus (4)

• The Effective Field Theorist's Approach to Gravitational Dynamics
• Gravitational radiative corrections from effective field theory
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Taming the post-Newtonian expansion: Simplifying the modes of the gravitational wave energy flux at infinity for a point particle in a circular orbit around a Schwarzschild black hole