The constrained normal form algorithm

DOI10.1007/BF01229000zbMath0674.70018OpenAlexW4233291725MaRDI QIDQ3829110

Jan A. Sanders, Richard H. Cushman

Publication date: 1989

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01229000

zbMATH Keywords

MAPLEquadratic Zeeman effectKepler Hamiltonianregularizable polynomial perturbationthree degree of freedom Kepler problem

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Two-body problems (70F05) Motion of charged particles (78A35)

Related Items

Secular motion around synchronously orbiting planetary satellites, Normalization through invariants in \(n\)-dimensional Kepler problems

Uses Software

• Maple

Cites Work

• Constrained normalization of Hamiltonian systems and perturbed Keplerian motion
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