Two binary stars gravitational waves - homotopy perturbation method
classification
🌌 astro-ph.SR
astro-ph.CO
keywords
homotopymethodperturbationphysicsanalysisaroundbinaryblack
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.