Two-body problem in the one-dimensional Heisenberg model
β Scribed by Shigetoshi Katsura
- Publisher
- Elsevier Science
- Year
- 1965
- Tongue
- English
- Weight
- 673 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0003-4916
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π SIMILAR VOLUMES
The problem presented in this paper is a model related to the collinear three-body problem which is itself a special case of the full three-body problem where three point masses interact under inverse square gravitation. The three-body problem has been known since Newton to be notoriously difficult.
The effect of the radiation-pressure in the problem of the two bodies is analysed. It is found that such an effect is the same as that of reducing the stellar mass, m, by the factor p (0 5 p 5 1 ) . The case p < 0 leads to stellar instability and, consequently, it is not considered here. The problem