Asymptotically null slices in numerical relativity
Asymptotically null slices in numerical relativity
The work in this thesis concerns numerical evolution of the equations of General Relativity. The motivation is towards astrophysics through the choice of coordinates adapted to outgoing gravitational waves far from the strong-field region of a given spacetime. These asymptotically null coordinates allow a large region of spacetime to be evolved at a negligible computational cost.
The behaviour of various gauge conditions (coordinate choices) can be studied without the resorting to the Einstein equations, but instead evolving coordinates on a known background. This “pure-gauge” approach is used to find gauge conditions suitable for evolving asymptotically null initial data.
Breakthroughs in numerical relativity have relied on a constraint damping technique. In the work that follows constraint damping is used to evolve asymptotically null initial data with various formulations of the Einstein equations.
Characteristic analysis of a given formulation allows for the construction of maximally dissipative and constraint preserving boundary conditions; such conditions are implemented and studied numerically on both flat and asymptotically null slices.
University of Southampton
Hilditch, David Matthew
d01d9bff-3c21-4ad3-8756-29e6f2f5f2f5
2007
Hilditch, David Matthew
d01d9bff-3c21-4ad3-8756-29e6f2f5f2f5
Hilditch, David Matthew
(2007)
Asymptotically null slices in numerical relativity.
University of Southampton, Doctoral Thesis.
Record type:
Thesis
(Doctoral)
Abstract
The work in this thesis concerns numerical evolution of the equations of General Relativity. The motivation is towards astrophysics through the choice of coordinates adapted to outgoing gravitational waves far from the strong-field region of a given spacetime. These asymptotically null coordinates allow a large region of spacetime to be evolved at a negligible computational cost.
The behaviour of various gauge conditions (coordinate choices) can be studied without the resorting to the Einstein equations, but instead evolving coordinates on a known background. This “pure-gauge” approach is used to find gauge conditions suitable for evolving asymptotically null initial data.
Breakthroughs in numerical relativity have relied on a constraint damping technique. In the work that follows constraint damping is used to evolve asymptotically null initial data with various formulations of the Einstein equations.
Characteristic analysis of a given formulation allows for the construction of maximally dissipative and constraint preserving boundary conditions; such conditions are implemented and studied numerically on both flat and asymptotically null slices.
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Published date: 2007
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Local EPrints ID: 466980
URI: http://eprints.soton.ac.uk/id/eprint/466980
PURE UUID: f9b5e76d-053c-4c7f-8c1b-a893fd653a5d
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Date deposited: 05 Jul 2022 08:05
Last modified: 16 Mar 2024 20:54
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David Matthew Hilditch
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