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JOURNALS // Regular and Chaotic Dynamics // Archive

Regul. Chaotic Dyn., 1998 Volume 3, Issue 3, Pages 132–160 (Mi rcd954)

This article is cited in 16 papers

On the 70th birthday of J.Moser

A Lie algebraic generalization of the Mumford system, its symmetries and its multi-Hamiltonian structure

M. Pedronia, P. Vanhaeckebc

a Università di Genova, Dipartitnento di Matematica, Via, Dodecanese 35, 1-16146 Genova, Italy
b Université des Sciences et Technologies de Lille, U.F.R. de Mathématiques, 59655 Villeneuve d'Ascq Cedex, France
c University of California, 1015 Department of Mathematics, Davis, CA 95616-8633, USA

Abstract: In this paper we generalize the Mumford system which describes for any fixed $g$ all linear flows on all hyperelliptic Jacobians of dimension $g$. The phase space of the Mumford system consists of triples of polynomials, subject to certain degree constraints, and is naturally seen as an affine subspace of the loop algebra of $\mathfrak{sl}(2)$. In our generalizations to an arbitrary simple Lie algebra $\mathfrak{g}$ the phase space consists of $\dim \mathfrak{g}$ polynomials, again subject to certain degree constraints. This phase space and its multi-Hamiltonian structure is obtained by a Poisson reduction along a subvariety $N$ of the loop algebra $\mathfrak{g} ((\lambda - 1))$ of $\mathfrak{g}$. Since $N$ is not a Poisson subvariety for the whole multi-Hamiltonian structure we prove an algebraic. Poisson reduction theorem for reduction along arbitrary subvarieties of an affine Poisson variety; this theorem is similar in spirit to the Marsden–Ratiu reduction theorem. We also give a different perspective on the multi-Hamiltonian structure of the Mumford system (and its generalizations) by introducing a master symmetry; this master symmetry can be described on the loop algebra $\mathfrak{g} ((\lambda -1))$ as the derivative in the direction of $\lambda$ and is shown to survive the Poisson reduction. When acting (as a Lie derivative) on one of the Poisson structures of the system it produces a next one, similarly when acting on one of the Hamiltonians (in involution) or their (commuting) vector fields it produces a next one. In this way we arrive at several multi-Hamiltonian hierarchies, built up by a master symmetry.

MSC: 34A05, 58F05, 58F07

Received: 21.07.1998

Language: English

DOI: 10.1070/RD1998v003n03ABEH000086



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