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Matter and Electromagnetic Fields in Strong Gravity

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High Order Methods for the Neutron Star Inspiral Problem

Mark Miller

NASA Jet Propulsion Laboratory


Abstract:   High order numerical methods are necessary for obtaining simulations of sufficient accuracy for gravitational wave template calculations. I will describe and present results from my implementation of a high order multigrid solver (initial data), a high order spacetime solver, and high order relativistic shock capturing solver, applied to the neutron star inspiral problem.

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