Some aspects of the classical three-body problem that are close or foreign to physical intuition

DOI10.1063/1.533318zbMath0972.70010OpenAlexW1978537168MaRDI QIDQ2738015

W. Thirring, Harald A. Posch

Publication date: 30 August 2001

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.533318

zbMATH Keywords

chaotic motioncomputer simulationoscillator modelreduced three-body problemsmall mass ratiosstability of orbits with small eccentricity

Mathematics Subject Classification ID

Three-body problems (70F07) Dynamical systems in classical and celestial mechanics (37N05) Stability problems for problems in Hamiltonian and Lagrangian mechanics (70H14)

Related Items (1)

Gravitational collapse and ergodicity in confined gravitational systems

Cites Work

• The existence of noncollision singularities in Newtonian systems
• The phase space structure of the extended Sitnikov problem

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