Two binary stars gravitational waves - homotopy perturbation method

TL;DR

This paper applies the homotopy perturbation method to solve the wave equation around a black hole, aiming to bridge theoretical and experimental physics in gravitational wave research.

Contribution

It introduces the homotopy perturbation method for analyzing wave equations in black hole environments, offering a new numerical approach.

Findings

Effective solution of wave equations around black holes.

Potential implications for gravitational wave detection.

Bridges gap between theory and experiment in physics.

Abstract

Homotopy perturbation is one of the newest methods for numerical analysis of deferential equations. We have used for solving wave equation around a black hole. Our conclusions have this method far reaching consequences for comparison of theoritical physics and experimental physics.