Instabilities and chaos in the classical three-body and three-rotor problems
Himalaya Senapati

TL;DR
This thesis explores the geometric and dynamical complexities of the classical three-body and three-rotor problems, revealing instabilities, chaos, and ergodic behavior through curvature analysis and numerical simulations.
Contribution
It extends geometric methods to analyze instabilities and chaos in these classical systems, including regularization of collisions and identification of chaos transition mechanisms.
Findings
Negative scalar curvature indicates geodesic instability.
Chaos emerges sharply at a critical energy in the 3-rotor problem.
Evidence of ergodicity and mixing near the chaos threshold.
Abstract
This thesis studies instabilities and singularities in a geometrical approach to the planar 3-body problem as well as instabilities, chaos and ergodicity in the 3-rotor problem. Trajectories of the planar 3-body problem are expressed as geodesics of the Jacobi-Maupertuis (JM) metric on the configuration space . Translation, rotation and scaling isometries lead to reduced dynamics on quotients of that encode information on the full dynamics. Riemannian submersions are used to find the quotient metrics and to show that the geodesic formulation regularizes collisions for the but not for the potential. Extending work of Montgomery, we show the negativity of the scalar curvature on the center of mass configuration space and certain quotients for equal masses and zero energy. Sectional curvatures are also found to be largely negative indicating widespread geodesic…
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Taxonomy
TopicsQuantum chaos and dynamical systems · Astro and Planetary Science · Stellar, planetary, and galactic studies
