Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations

Many evolution problems in physics are described by partial differential equations on an infinite domain; therefore, one is interested in the solutions to such problems for a given initial dataset. A prominent example is the binary black-hole problem within Einstein's theory of gravitation, in...

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Main Authors: Olivier Sarbach, Manuel Tiglio
Format: Article
Language:English
Published: SpringerOpen 2012-08-01
Series:Living Reviews in Relativity
Subjects:
Online Access:http://www.livingreviews.org/lrr-2012-9
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spelling doaj-e605d96cc7854a499ac6a7c77ed987812020-11-25T00:54:43ZengSpringerOpenLiving Reviews in Relativity1433-83512012-08-01159Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field EquationsOlivier SarbachManuel TiglioMany evolution problems in physics are described by partial differential equations on an infinite domain; therefore, one is interested in the solutions to such problems for a given initial dataset. A prominent example is the binary black-hole problem within Einstein's theory of gravitation, in which one computes the gravitational radiation emitted from the inspiral of the two black holes, merger and ringdown. Powerful mathematical tools can be used to establish qualitative statements about the solutions, such as their existence, uniqueness, continuous dependence on the initial data, or their asymptotic behavior over large time scales. However, one is often interested in computing the solution itself, and unless the partial differential equation is very simple, or the initial data possesses a high degree of symmetry, this computation requires approximation by numerical discretization. When solving such discrete problems on a machine, one is faced with a finite limit to computational resources, which leads to the replacement of the infinite continuum domain with a finite computer grid. This, in turn, leads to a discrete initial-boundary value problem. The hope is to recover, with high accuracy, the exact solution in the limit where the grid spacing converges to zero with the boundary being pushed to infinity. The goal of this article is to review some of the theory necessary to understand the continuum and discrete initial boundary-value problems arising from hyperbolic partial differential equations and to discuss its applications to numerical relativity; in particular, we present well-posed initial and initial-boundary value formulations of Einstein's equations, and we discuss multi-domain high-order finite difference and spectral methods to solve them.http://www.livingreviews.org/lrr-2012-9Boundary value problemsPartial differential equations
collection DOAJ
language English
format Article
sources DOAJ
author Olivier Sarbach
Manuel Tiglio
spellingShingle Olivier Sarbach
Manuel Tiglio
Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
Living Reviews in Relativity
Boundary value problems
Partial differential equations
author_facet Olivier Sarbach
Manuel Tiglio
author_sort Olivier Sarbach
title Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
title_short Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
title_full Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
title_fullStr Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
title_full_unstemmed Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations
title_sort continuum and discrete initial-boundary value problems and einstein's field equations
publisher SpringerOpen
series Living Reviews in Relativity
issn 1433-8351
publishDate 2012-08-01
description Many evolution problems in physics are described by partial differential equations on an infinite domain; therefore, one is interested in the solutions to such problems for a given initial dataset. A prominent example is the binary black-hole problem within Einstein's theory of gravitation, in which one computes the gravitational radiation emitted from the inspiral of the two black holes, merger and ringdown. Powerful mathematical tools can be used to establish qualitative statements about the solutions, such as their existence, uniqueness, continuous dependence on the initial data, or their asymptotic behavior over large time scales. However, one is often interested in computing the solution itself, and unless the partial differential equation is very simple, or the initial data possesses a high degree of symmetry, this computation requires approximation by numerical discretization. When solving such discrete problems on a machine, one is faced with a finite limit to computational resources, which leads to the replacement of the infinite continuum domain with a finite computer grid. This, in turn, leads to a discrete initial-boundary value problem. The hope is to recover, with high accuracy, the exact solution in the limit where the grid spacing converges to zero with the boundary being pushed to infinity. The goal of this article is to review some of the theory necessary to understand the continuum and discrete initial boundary-value problems arising from hyperbolic partial differential equations and to discuss its applications to numerical relativity; in particular, we present well-posed initial and initial-boundary value formulations of Einstein's equations, and we discuss multi-domain high-order finite difference and spectral methods to solve them.
topic Boundary value problems
Partial differential equations
url http://www.livingreviews.org/lrr-2012-9
work_keys_str_mv AT oliviersarbach continuumanddiscreteinitialboundaryvalueproblemsandeinsteinsfieldequations
AT manueltiglio continuumanddiscreteinitialboundaryvalueproblemsandeinsteinsfieldequations
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