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arxiv: 1802.07593 · v2 · pith:OMS2TO2Enew · submitted 2018-02-21 · 🧮 math-ph · hep-th· math.MP· nlin.SI

From Hamiltonian to zero curvature formulation for classical integrable boundary conditions

classification 🧮 math-ph hep-thmath.MPnlin.SI
keywords boundarycurvatureintegrablematricesmatrixzeroclassicalconditions
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We reconcile the Hamiltonian formalism and the zero curvature representation in the approach to integrable boundary conditions for a classical integrable system in 1+1 space-time dimensions. We start from an ultralocal Poisson algebra involving a Lax matrix and two (dynamical) boundary matrices. Sklyanin's formula for the double-row transfer matrix is used to derive Hamilton's equations of motion for both the Lax matrix {\bf and} the boundary matrices in the form of zero curvature equations. A key ingredient of the method is a boundary version of the Semenov-Tian-Shansky formula for the generating function of the time-part of a Lax pair. The procedure is illustrated on the finite Toda chain for which we derive Lax pairs of size $2\times 2$ for previously known Hamiltonians of type $BC_N$ and $D_N$ corresponding to constant and dynamical boundary matrices respectively.

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