Published September 1974
| Version v1
Journal article
Improved criteria for hyperbolic-elliptic motion in the general three-body problem, 2
Description
Abstract In addition to the previous criteria (YOSHIDA 1972) for the hyperbolic-elliptic motion in the general three-body problem, another one is given by taking into account the non-zero angular momentum. So long as the conditions regarding the angular momentum of the system are satisfied, the new criterion includes theorem 1 in YOSHIDA (1972). The effect of the new criterion is different in each case as illustrated in BECKER's (1920) numerical examples, having a negative total energy. In disregard of the rigorous estimations of numerical errors, these examples are shown to be hyperbolic-elliptic as t → +∞, and thus contradict CHAZY's (1929) assertion that there are no motions of the exchange type in the three-body problem.
Additional details
Identifiers
Publishing Information
- Journal Title
- Publications of the Astronomical Society of Japan
- Journal Volume
- 26
- Journal Issue
- 3
- Series
- Publ. Astron. Soc. Jap.
- Journal Page Range
- 367-377
- ISSN
- 2053-051X
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 6199087
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANGULAR MOMENTUM; ASYMPTOTIC SOLUTIONS; MOTION; NUMERICAL SOLUTION; THREE-BODY PROBLEM
- Descriptors DEC
- MANY-BODY PROBLEM
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent