Published February 15, 2006
| Version v1
Journal article
Iterated Crank-Nicolson method for hyperbolic and parabolic equations in numerical relativity
- 1. Max-Planck-Institut fuer Gravitationsphysik, Albert Einstein Institut, Golm (Germany)
- 2. Department of Physics, Udine University, Udine (Italy)
- 3. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803-4001 (United States)
- 4. SISSA, International School for Advanced Studies and INFN, Trieste (Italy)
Description
The iterated Crank-Nicolson is a predictor-corrector algorithm commonly used in numerical relativity for the solution of both hyperbolic and parabolic partial differential equations. We here extend the recent work on the stability of this scheme for hyperbolic equations by investigating the properties when the average between the predicted and corrected values is made with unequal weights and when the scheme is applied to a parabolic equation. We also propose a variant of the scheme in which the coefficients in the averages are swapped between two corrections leading to systematically larger amplification factors and to a smaller numerical dispersion
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.73.044001;
- arXiv
- arXiv:gr-qc/0601139v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 73
- Journal Issue
- 4
- Journal Page Range
- p. 044001-044001.7
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37080938
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ALGORITHMS; AMPLIFICATION; CORRECTIONS; COSMOLOGY; GENERAL RELATIVITY THEORY; ITERATIVE METHODS; MATHEMATICAL SOLUTIONS; PARTIAL DIFFERENTIAL EQUATIONS; STABILITY
- Descriptors DEC
- CALCULATION METHODS; DIFFERENTIAL EQUATIONS; EQUATIONS; FIELD THEORIES; MATHEMATICAL LOGIC; RELATIVITY THEORY
Optional Information
- Notes
- (c) 2006 The American Physical Society