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In mathematical physics, the De Donder–Weyl theory is a formalism in the calculus of variations over spacetime which treats the space and time coordinates on equal footing. In this framework, a field is represented as a system that varies both in space and in time. = -\partial H / \partial y^ |- | |- |} == De Donder–Weyl formulation of field theory == The De Donder–Weyl theory is based on a change of variables. Let ''xi'' be spacetime coordinates, for ''i'' = 1 to ''n'' (with ''n'' = 4 representing 3 + 1 dimensions of space and time), and ''ya'' field variables, for ''a'' = 1 to ''m'', and ''L'' the Lagrangian density. : With ''polymomenta'' ''pia'' defined as : and for ''De Donder–Weyl Hamiltonian function'' ''H'' defined as : the De Donder–Weyl equations are:〔Igor V. Kanatchikov: (''Towards the Born–Weyl quantization of fields'' ), arXiv:quant-ph/9712058v1 (submitted on 31 December 1997)〕 : These canonical equations of motion are covariant. The theory is a formulation of a covariant Hamiltonian field theory and for ''n'' = 1 it reduces to Hamiltonian mechanics (see also action principle in the calculus of variations). The generalization of Poisson brackets to the De Donder–Weyl theory and the representation of De Donder-Weyl equations in terms of generalized Poisson brackets was found by Kanatchikov in 1993.〔Igor V. Kanatchikov: (''On the Canonical Structure of the De Donder-Weyl Covariant Hamiltonian Formulation of Field Theory I. Graded Poisson brackets and equations of motion'' ), arXiv:hep-th/9312162v1 (submitted on 20 Dec 1993)〕 抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「De Donder–Weyl theory」の詳細全文を読む スポンサード リンク
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