Two binary stars gravitational waves - homotopy perturbation method

Published 22 Mar 2012 in astro-ph.SR and astro-ph.CO | (1203.5123v2)

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.

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