Hamiltonian structure of peakons as weak solutions for the modified Camassa-Holm equation

preprint2019arXivOpen access

Abstract

The modified Camassa-Holm (mCH) equation is a bi-Hamiltonian system possessing NN-peakon weak solutions, for all N≥1N\geq 1, in the setting of an integral formulation which is used in analysis for studying local well-posedness, global existence, and wave breaking for non-peakon solutions. Unlike the original Camassa-Holm equation, the two Hamiltonians of the mCH equation do not reduce to conserved integrals (constants of motion) for 22-peakon weak solutions. This perplexing situation is addressed here by finding an explicit conserved integral for NN-peakon weak solutions for all N≥2N\geq 2. When NN is even, the conserved integral is shown to provide a Hamiltonian structure with the use of a natural Poisson bracket that arises from reduction of one of the Hamiltonian structures of the mCH equation. But when NN is odd, the Hamiltonian equations of motion arising from the conserved integral using this Poisson bracket are found to differ from the dynamical equations for the mCH NN-peakon weak solutions. Moreover, the lack of conservation of the two Hamiltonians of the mCH equation when they are reduced to 22-peakon weak solutions is shown to extend to NN-peakon weak solutions for all N≥2N\geq 2. The connection between this loss of integrability structure and related work by Chang and Szmigielski on the Lax pair for the mCH equation is discussed.

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