Document Type

Article

Publication Date

11-21-2003

Abstract

We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to construct stable finite-difference schemes for numerical relativity, in particular for their use in black-hole excision. As an application, we present 3D simulations of a scalar field propagating in a Schwarzschild black-hole background.

Publication Source (Journal or Book title)

Classical and Quantum Gravity

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