Although particle-mesh simulation techniques have proved extremely valuable in the study of galactic evolution, the high cost of the calculations on serial computers and the limited resolution which can be employed have severely restricted applications. The vector and array processors now available
โฆ LIBER โฆ
Numerical simulators of stability in astrophysical problems
โ Scribed by J. N. Tokis
- Publisher
- Springer Netherlands
- Year
- 1992
- Tongue
- English
- Weight
- 321 KB
- Volume
- 191
- Category
- Article
- ISSN
- 0004-640X
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## Abstract A novel integral equation technique is employed for the analysis of dynamic stability problems. The governing equation of the linearized parametric resonance problem is transformed into an integral equation. The kernel of the integral equation is computed as the influence function for t