English

Isotropy Groups and Kinematic Orbits for 1 and 2-$d$ $N$-Body Problems

General Relativity and Quantum Cosmology 2018-10-10 v1

Abstract

Mitchell and Littlejohn showed that isotropy groups and orbits for NN-body problems attain a sense of genericity for N=5N = 5. The author recently showed that the arbitrary-dd generalization of this 3-dd result is that genericity in this sense occurs for N=d+2N = d + 2. The author also showed that a second sense of genericity -- now order-theoretic rather than a matter of counting -- occurs for N=2d+1N = 2 d + 1, excepting d=3d = 3, for which it is not 7 but 8. Applications of this work include 1) that some of the increase in complexity in passing from 3 to 4 and 5 body problems in 3-dd is already present in the more-well known setting of passing from intervals to triangles and then to quadrilaterals in 2-dd. 2) That not (d,N)=(3,6)(d, N) = (3, 6) but (4,6)(4, 6) is a natural theoretical successor of (3,5)(3, 5). 3) Such consideration isotropy groups and orbits is moreover a model for a larger case of interest, namely that of GR's reduced configuration spaces. The current Article presents the lower-dd cases explicitly: 0, 1 and 2-dd, including also the topological and geometrical form of the corresponding isotropy groups and orbits.

Keywords

Cite

@article{arxiv.1810.04043,
  title  = {Isotropy Groups and Kinematic Orbits for 1 and 2-$d$ $N$-Body Problems},
  author = {Edward Anderson},
  journal= {arXiv preprint arXiv:1810.04043},
  year   = {2018}
}

Comments

16 pages, including 4 figures. arXiv admin note: text overlap with arXiv:1807.08391

R2 v1 2026-06-23T04:33:35.752Z