arXiv Analytics

Sign in

arXiv:gr-qc/0601124AbstractReferencesReviewsResources

A minimization problem for the lapse and the initial-boundary value problem for Einstein's field equations

Gabriel Nagy, Olivier Sarbach

Published 2006-01-28Version 1

We discuss the initial-boundary value problem of General Relativity. Previous considerations for a toy model problem in electrodynamics motivate the introduction of a variational principle for the lapse with several attractive properties. In particular, it is argued that the resulting elliptic gauge condition for the lapse together with a suitable condition for the shift and constraint-preserving boundary conditions controlling the Weyl scalar Psi_0 are expected to yield a well posed initial-boundary value problem for metric formulations of Einstein's field equations which are commonly used in numerical relativity. To present a simple and explicit example we consider the 3+1 decomposition introduced by York of the field equations on a cubic domain with two periodic directions and prove in the weak field limit that our gauge condition for the lapse and our boundary conditions lead to a well posed problem. The method discussed here is quite general and should also yield well posed problems for different ways of writing the evolution equations, including first order symmetric hyperbolic or mixed first-order second-order formulations. Well posed initial-boundary value formulations for the linearization about arbitrary stationary configurations will be presented elsewhere.

Comments: 34 pages, no figures
Journal: Class.Quant.Grav. 23 (2006) S477-S504
Categories: gr-qc
Related articles: Most relevant | Search more
arXiv:1203.2154 [gr-qc] (Published 2012-03-09, updated 2012-04-24)
Boundary Conditions for the Gravitational Field
arXiv:1306.6204 [gr-qc] (Published 2013-06-26, updated 2014-05-22)
Conformally covariant systems of wave equations and their equivalence to Einstein's field equations
arXiv:gr-qc/0412006 (Published 2004-12-02, updated 2005-06-10)
Linearized solutions of the Einstein equations within a Bondi-Sachs framework, and implications for boundary conditions in numerical simulations