Cauchy boundaries in linearized gravitational theory

Bela Szilágyi, Roberto Gómez, Nigel T. Bishop, and Jeffrey Winicour
Phys. Rev. D 62, 104006 – Published 9 October 2000
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Abstract

We investigate the numerical stability of Cauchy evolution of linearized gravitational theory in a three-dimensional bounded domain. Criteria of robust stability are proposed, developed into a testbed and used to study various evolution-boundary algorithms. We construct a standard explicit finite difference code which solves the unconstrained linearized Einstein equations in the 3+1 formulation and measure its stability properties under Dirichlet, Neumann, and Sommerfeld boundary conditions. We demonstrate the robust stability of a specific evolution-boundary algorithm under random constraint violating initial data and random boundary data.

  • Received 9 December 1999

DOI:https://doi.org/10.1103/PhysRevD.62.104006

©2000 American Physical Society

Authors & Affiliations

Bela Szilágyi1, Roberto Gómez1, Nigel T. Bishop2, and Jeffrey Winicour1,3

  • 1Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260
  • 2Department of Mathematics, Applied Mathematics and Astronomy, University of South Africa, P.O. Box 392, Pretoria 0003, South Africa
  • 3Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, 14476 Golm, Germany

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Issue

Vol. 62, Iss. 10 — 15 November 2000

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