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Matter and Electromagnetic Fields in Strong Gravity
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Matter and Electromagnetic Fields in Strong Gravity
CSIC Building (#406),
Seminar Room 4122.
Directions: home.cscamm.umd.edu/directions
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High Order Methods for the Neutron Star Inspiral Problem
Mark Miller
NASA Jet Propulsion Laboratory
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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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