Die u:cris Detailansicht:
Some aspects of the classical three-body problem that are close or foreign to physical intuition
- Autor(en)
- Harald Posch, Walter Thirring
- Abstrakt
We propose a simple oscillator model for the reduced three-body problem to understand the stability of orbits with small eccentricity of a light planet. It models the main short-time features for small mass ratios of the other bodies. These results are confronted with the exact mathematical analysis for stability for all times, and with computer simulation results for bigger mass ratios, where chaotic features emerge. Œ 2000 American Institute of Physics.
- Organisation(en)
- Computergestützte Physik und Physik der Weichen Materie
- Journal
- Journal of Mathematical Physics
- Band
- 41
- Seiten
- 3430-3447
- Anzahl der Seiten
- 18
- ISSN
- 0022-2488
- DOI
- https://doi.org/10.1063/1.533318
- Publikationsdatum
- 2000
- Peer-reviewed
- Ja
- ÖFOS 2012
- 103036 Theoretische Physik
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/5d172fb3-febf-4bd5-9d5d-afbc8cdbcbea