The constrained normal form algorithm

Details The constrained normal form algorithm The constrained normal form algorithm

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cemec..45..181c&link_type=abstract

Celestial Mechanics, Volume 45, Issue 1-3, pp. 181-187

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Applications

Scientific paper

This paper describes an algorithm which brings a regularizable polynomial perturbation of a three degree of freedom Kepler problem into a normal form which Poisson commutes with the Kepler Hamiltonian. We illustrate the alogrithm with an example: the quadratic Zeeman effect. For other applications of this algorithm see [1],[4], and [5]. The authors have written a program in MAPLE which implements the constrained normal form.

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