Periodic orbits for three particles with finite angular momentum
arXiv:nlin/0112003 · doi:10.1016/S0375-9601(01)00768-X
Abstract
We present a novel numerical method to calculate periodic orbits for dynamical systems by an iterative process which is based directly on the action integral in classical mechanics. New solutions are obtained for the planar motion of three equal mass particles on a common periodic orbit with finite total angular momentum, under the action of attractive pairwise forces of the form . It is shown that for , Lagrange's 1772 circular solution is the limiting case of a complex symmetric orbit. The evolution of this orbit and another recently discovered one in the shape of a figure eight is investigated for a range of angular momenta. Extensions to n equal mass particles and to three particles of different masses are also discussed briefly.
6 pages, 7 figures. Accepted for publication in Physics Letters A
Cited by in corpus (8)
- Three Classes of Newtonian Three-Body Planar Periodic Orbits
- An existence of simple choreographies for N-body problem - a computer assisted proof
- More than six hundreds new families of Newtonian periodic planar collisionless three-body orbits
- Characterization of the gravitational wave emission of three black holes
- Stability and chaos of hierarchical three black hole configurations
- A commend on "Three Classes of Newtonian Three-Body Planar Periodic Orbits" by Šuvakov and Dmitrašinović (PRL, 2013)
- Chaotic dynamics in the planar gravitational many-body problem with rigid body rotations
- Numerical Methods and Closed Orbits in the Kepler-Heisenberg Problem