English

Stability and chaos in the classical three rotor problem

Chaotic Dynamics 2019-09-25 v3 Mathematical Physics Dynamical Systems math.MP

Abstract

We study the equal-mass classical three rotor problem, a variant of the three body problem of celestial mechanics. The quantum NN-rotor problem has been used to model chains of coupled Josephson junctions and also arises via a partial continuum limit of the Wick-rotated XY model. In units of the coupling, the energy serves as a control parameter. We find periodic 'pendulum' and 'breather' orbits at all energies and choreographies at relatively low energies. They furnish analogs of the Euler-Lagrange and figure-8 solutions of the planar three body problem. Integrability at very low energies gives way to a rather marked transition to chaos at Ec4E_c \approx 4, followed by a gradual return to regularity as EE \to \infty. We find four signatures of this transition: (a) the fraction of the area of Poincar\'e surfaces occupied by chaotic sections rises sharply at EcE_c, (b) discrete symmetries are spontaneously broken at EcE_c, (c) E=4E=4 is an accumulation point of stable to unstable transitions in pendulum solutions and (d) the Jacobi-Maupertuis curvature goes from being positive to having both signs above E=4E=4. Moreover, Poincar\'e plots also reveal a regime of global chaos slightly above EcE_c.

Keywords

Cite

@article{arxiv.1810.01317,
  title  = {Stability and chaos in the classical three rotor problem},
  author = {Govind S. Krishnaswami and Himalaya Senapati},
  journal= {arXiv preprint arXiv:1810.01317},
  year   = {2019}
}

Comments

8 pages, 8 figures, Presented at the Conference on Nonlinear Systems and Dynamics, New Delhi, Oct 2018

R2 v1 2026-06-23T04:26:03.857Z