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Modelling Extreme-Mass-Ratio Inspirals using Pseudospectral Methods (1001.4697v1)

Published 26 Jan 2010 in gr-qc, astro-ph.GA, and astro-ph.HE

Abstract: We introduce a new time-domain method for computing the self-force acting on a scalar particle in a Schwarzschild geometry. The principal feature of our method consists in the division of the spatial domain into several subdomains and locating the particle at the interface betweem two them. In this way, we avoid the need of resolving a small length scale associated with the presence of a particle in the computational domain and, at the same time, we avoid numerical problems due to the low differentiability of solutions of equations with point-like singular behaviour.

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