Simulations of gravitational collapse in null coordinates. III. : Hyperbolicity
Simulations of gravitational collapse in null coordinates. III. : Hyperbolicity
We investigate the well-posedness of the characteristic initial-boundary value problem for the Einstein equations in Bondi-like coordinates (including Bondi, double-null and affine). We propose a definition of strong hyperbolicity of a system of partial differential equations of any order, and show that the Einstein equations in Bondi-like coordinates in their second-order form used in numerical relativity do not meet it, in agreement with results of Giannakopoulos et al. for specific first-order reductions. In the principal part, frozen coefficient approximation that one uses to examine hyperbolicity, we explicitly construct the general solution to identify the solutions that obstruct strong hyperbolicity. Independently, we present a first-order symmetric hyperbolic formulation of the Einstein equations in Bondi gauge, linearized about Schwarzschild, thus completing work by Frittelli. This establishes an energy norm (L2 in the metric perturbations and selected first and second derivatives), in which the initial-boundary value problem, with initial data on an outgoing null cone and boundary data on a timelike cylinder or an ingoing null cone, is well posed, thus verifying a conjecture by Giannakopoulos et al. Unfortunately, our method does not extend to the pure initial-value problem on a null cone with regular vertex.
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
15 July 2024
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
Gundlach, Carsten
(2024)
Simulations of gravitational collapse in null coordinates. III. : Hyperbolicity.
Physical Review D, 110 (2), [024020].
(doi:10.1103/PhysRevD.110.024020).
Abstract
We investigate the well-posedness of the characteristic initial-boundary value problem for the Einstein equations in Bondi-like coordinates (including Bondi, double-null and affine). We propose a definition of strong hyperbolicity of a system of partial differential equations of any order, and show that the Einstein equations in Bondi-like coordinates in their second-order form used in numerical relativity do not meet it, in agreement with results of Giannakopoulos et al. for specific first-order reductions. In the principal part, frozen coefficient approximation that one uses to examine hyperbolicity, we explicitly construct the general solution to identify the solutions that obstruct strong hyperbolicity. Independently, we present a first-order symmetric hyperbolic formulation of the Einstein equations in Bondi gauge, linearized about Schwarzschild, thus completing work by Frittelli. This establishes an energy norm (L2 in the metric perturbations and selected first and second derivatives), in which the initial-boundary value problem, with initial data on an outgoing null cone and boundary data on a timelike cylinder or an ingoing null cone, is well posed, thus verifying a conjecture by Giannakopoulos et al. Unfortunately, our method does not extend to the pure initial-value problem on a null cone with regular vertex.
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e-pub ahead of print date: 9 July 2024
Published date: 15 July 2024
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© 2024 American Physical Society.
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Local EPrints ID: 492345
URI: http://eprints.soton.ac.uk/id/eprint/492345
ISSN: 2470-0010
PURE UUID: 0bc9c6c6-9f47-4dd5-97f9-f932cdc3f496
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Date deposited: 24 Jul 2024 16:49
Last modified: 25 Jul 2024 01:36
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