Parallel/vector integration methods for dynamical astronomy (Q1976095)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Parallel/vector integration methods for dynamical astronomy |
scientific article; zbMATH DE number 1442265
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Parallel/vector integration methods for dynamical astronomy |
scientific article; zbMATH DE number 1442265 |
Statements
Parallel/vector integration methods for dynamical astronomy (English)
0 references
1999
0 references
The author investigates the effect of parallelization in three typical numerical ODE integrators. First, in the Picard-Chebyshev method using a large number of Chebyshev polynomials, 100-1000 times acceleration is detected. Second, by the parallelization of a symplectic integrator (using fixed point iterations) 50 times acceleration is achieved. Third, an extrapolation method which uses trial integrations in parallel, is accelerated by the ``folding'' technique. The author also presents an all-purpose method for which 3.5 times acceleration is achieved, and gives a perspective of employing implicit integrators with multiple corrections.
0 references
folding technique
0 references
parallelization
0 references
Picard-Chebyshev method
0 references
Chebyshev polynomials
0 references
symplectic integrator
0 references
fixed point iterations
0 references
extrapolation method
0 references
trial integrations
0 references
all-purpose method
0 references
implicit integrators with multiple corrections
0 references