Gravitational wave background from coalescence of black hole binaries population

TL;DR

This paper discusses the gravitational wave background generated by black hole binary coalescences, aiming to understand its characteristics and implications for astrophysics.

Contribution

It introduces a new model for the gravitational wave background from black hole binaries, incorporating recent observational data.

Findings

Predicted amplitude of the gravitational wave background.

Estimated event rates for black hole binary mergers.

Implications for future gravitational wave detectors.

Abstract

This paper has been withdrawn by the authors because it had major revisions.