Tail of Gravitational Radiation and Coulomb Final-State Interaction

TL;DR

This paper provides an intuitive derivation of how tail effects modify the intensity of gravitational radiation, enhancing understanding of gravitational wave propagation.

Contribution

It introduces a straightforward derivation of tail corrections to gravitational radiation intensity, clarifying their physical origin.

Findings

Tail effects cause measurable corrections to gravitational wave signals.

The derivation offers a clearer physical interpretation of tail contributions.

Results improve modeling accuracy for gravitational wave detectors.

Abstract

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