Math 2.0

Mechanics of particles and systems Definition

De Donder–Weyl theory

Builds on Lagrangian densityLegendre transformationEuler–Lagrange equation

Definition

Let n,k≥1n, k \ge 1 and let U⊆ℝnU \subseteq \R^n be open, with coordinates x1,…,xnx^1, \dots, x^n. Let ℒ(x,ya,zμa)\mathcal{L}(x, y^a, z^a_\mu) be a first-order Lagrangian density for fields φ ⁣:U→ℝk\varphi \colon U \to \R^k, where zμaz^a_\mu stands for ∂μφa\partial_\mu \varphi^a.

  1. The polymomenta are paμ=∂ℒ∂zμa(x,y,z)p^\mu_a = \dfrac{\partial \mathcal{L}}{\partial z^a_\mu}(x, y, z).
  2. The density ℒ\mathcal{L} is regular if, for all fixed (x,y)(x, y), the map z↦pz \mapsto p is a diffeomorphism onto an open set; then z=z(x,y,p)z = z(x, y, p) is its inverse.
  3. For regular ℒ\mathcal{L}, the De Donder–Weyl Hamiltonian is H(x,y,p)=paμ zμa(x,y,p)−ℒ(x,y,z(x,y,p)),H(x, y, p) = p^\mu_a \, z^a_\mu(x, y, p) - \mathcal{L}\big(x, y, z(x, y, p)\big), with summation over μ\mu and aa.
  4. The De Donder–Weyl equations for φ\varphi and paμ ⁣:U→ℝp^\mu_a \colon U \to \R are ∂μφa=∂H∂paμ,∑μ=1n∂μpaμ=−∂H∂ya.\partial_\mu \varphi^a = \frac{\partial H}{\partial p^\mu_a}, \qquad \sum_{\mu = 1}^n \partial_\mu p^\mu_a = -\frac{\partial H}{\partial y^a}.

De Donder–Weyl theory is the description of the field theory of ℒ\mathcal{L} by HH and these equations.

Remarks

The map z↦pz \mapsto p is a fiberwise Legendre transformation. For regular ℒ\mathcal{L}, a smooth φ\varphi solves the Euler–Lagrange equations of ℒ\mathcal{L} if and only if φ\varphi together with paμ=∂ℒ/∂zμa(x,φ,∂φ)p^\mu_a = \partial \mathcal{L} / \partial z^a_\mu (x, \varphi, \partial \varphi) solves the De Donder–Weyl equations.

Example: for n=1n = 1, the variable x1=tx^1 = t is time, there is one momentum pap_a per coordinate, HH is the usual Hamiltonian, and the equations are Hamilton's equations φ˙a=∂H/∂pa\dot\varphi^a = \partial H / \partial p_a, p˙a=−∂H/∂ya\dot p_a = -\partial H / \partial y^a.

Example: for n=4n = 4, k=1k = 1, η=diag(1,−1,−1,−1)\eta = \mathrm{diag}(1, -1, -1, -1) and ℒ=12ημνzμzν−12m2y2\mathcal{L} = \frac{1}{2} \eta^{\mu\nu} z_\mu z_\nu - \frac{1}{2} m^2 y^2, one has pμ=ημνzνp^\mu = \eta^{\mu\nu} z_\nu, which is invertible. Then H=12ημνpμpν+12m2y2H = \frac{1}{2} \eta_{\mu\nu} p^\mu p^\nu + \frac{1}{2} m^2 y^2, and the equations ∂μφ=ημνpν\partial_\mu \varphi = \eta_{\mu\nu} p^\nu, ∂μpμ=−m2φ\partial_\mu p^\mu = -m^2 \varphi give the Klein–Gordon equation ημν∂μ∂νφ+m2φ=0\eta^{\mu\nu} \partial_\mu \partial_\nu \varphi + m^2 \varphi = 0.

Non-example: for n=2n = 2, k=1k = 1 and ℒ=z1\mathcal{L} = z_1, the polymomenta are p1=1p^1 = 1, p2=0p^2 = 0 for all zz, so the map z↦pz \mapsto p is not injective and clause 2 fails.

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To understand this page from the ground up, read these 4 pages in order. The foundations come first.

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  1. Euler–Lagrange equation concept
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  3. Legendre transformation concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/De_Donder%E2%80%93Weyl_theory
About this page
TagQS9YR5WDZD
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Kinddefinition
WritingW0 stub
MSC70S05, 70G45, 49S05
DefinesDe Donder–Weyl theory
UsesLagrangian density, Legendre transformation, Euler–Lagrange equation
Changed3 November 2026

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