Chaotic motion in axially symmetric potentials with oblate quadrupole deformation

DOI10.1016/j.physleta.2011.08.050zbMath1252.70039OpenAlexW2088879055MaRDI QIDQ691955

Framsol López-Suspes, Javier Ramos-Caro, Patricio S. Letelier

Publication date: 4 December 2012

Published in: Physics Letters. A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.physleta.2011.08.050

zbMATH Keywords

chaosgravitationnuclear physicsmean field approachatomic physics

Mathematics Subject Classification ID

Model quantum field theories (81T10) Nuclear physics (81V35) Transition to stochasticity (chaotic behavior) for nonlinear problems in mechanics (70K55) Hamilton's equations (70H05) Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Quantum chaos (81Q50) Characteristic and Lyapunov exponents of ordinary differential equations (34D08) Atomic physics (81V45)

Related Items (2)

Chaos in the Kepler Problem with Quadrupole Perturbations ⋮ Stealth chaos due to frame-dragging

Cites Work

• On the numerical computation of Poincaré maps
• Non integrability of the \(J_ 2\) problem
• Non-integrability of the problem of motion around an oblate planet
• Unnamed Item

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