Math 2.0

Mechanics of particles and systems Definition

Covariant Hamiltonian field theory

Builds on Fiber bundleDifferential formLagrangian densityLegendre transformation

Definition

Let Y→XY \to X be a smooth fiber bundle over an oriented nn-dimensional manifold XX, with fibers of dimension kk. Use bundle coordinates (xμ,yi)(x^\mu, y^i), μ=1,…,n\mu = 1, \dots, n, i=1,…,ki = 1, \dots, k. Let ω=dx1∧⋯∧dxn\omega = dx^1 \wedge \cdots \wedge dx^n and ωμ=ι∂μω\omega_\mu = \iota_{\partial_\mu} \omega, the contraction of ω\omega with ∂/∂xμ\partial / \partial x^\mu.

Let VYV Y be the vertical tangent bundle of YY.

  1. The momentum phase space is the Legendre bundle Π→Y\Pi \to Y with fiber Vy∗Y⊗TxX⊗ΛnTx∗XV^*_y Y \otimes T_x X \otimes \Lambda^n T^*_x X over y∈Yy \in Y above x∈Xx \in X. Its elements are piμ dyi⊗∂μ⊗ωp^\mu_i \, dy^i \otimes \partial_\mu \otimes \omega, and (xμ,yi,piμ)(x^\mu, y^i, p^\mu_i) are coordinates on Π\Pi.
  2. A Hamiltonian form is a differential form on Π\Pi that reads in these coordinates H=piμ dyi∧ωμ−ℋ(xν,yj,pjν) ω,H = p^\mu_i \, dy^i \wedge \omega_\mu - \mathcal{H}(x^\nu, y^j, p^\nu_j) \, \omega, for a smooth local function ℋ\mathcal{H}, the Hamiltonian density. Here the first term is summed over μ\mu and ii.
  3. For a section x↦(yi(x),piμ(x))x \mapsto (y^i(x), p^\mu_i(x)) of Π→X\Pi \to X, its covariant Hamilton equations for HH are ∂μyi=∂ℋ∂piμ,∑μ=1n∂μpiμ=−∂ℋ∂yi.\partial_\mu y^i = \frac{\partial \mathcal{H}}{\partial p^\mu_i}, \qquad \sum_{\mu = 1}^n \partial_\mu p^\mu_i = -\frac{\partial \mathcal{H}}{\partial y^i}.

Covariant Hamiltonian field theory is the study of the fields as solutions of the covariant Hamilton equations of a Hamiltonian form.

Remarks

The function ℋ\mathcal{H} depends on the chosen coordinates, but the form HH is a global object on Π\Pi; the covariant Hamilton equations do not depend on the coordinates.

A first-order Lagrangian density ℒ(x,y,z)\mathcal{L}(x, y, z) with zμiz^i_\mu standing for ∂μyi\partial_\mu y^i defines the Legendre map piμ=∂ℒ/∂zμip^\mu_i = \partial \mathcal{L} / \partial z^i_\mu, a fiberwise Legendre transformation. If this map is a diffeomorphism, then ℋ=piμzμi−ℒ\mathcal{H} = p^\mu_i z^i_\mu - \mathcal{L}, with zz expressed through pp, defines a Hamiltonian form, and its covariant Hamilton equations are equivalent to the Euler–Lagrange equations of ℒ\mathcal{L}.

Example: let X=ℝ2X = \R^2 with η=diag(1,−1)\eta = \mathrm{diag}(1, -1), Y=X×ℝY = X \times \R and ℋ=12ημνpμpν\mathcal{H} = \frac{1}{2} \eta_{\mu\nu} p^\mu p^\nu. The equations read ∂μy=ημνpν\partial_\mu y = \eta_{\mu\nu} p^\nu and ∂μpμ=0\partial_\mu p^\mu = 0, so ημν∂μ∂νy=0\eta^{\mu\nu} \partial_\mu \partial_\nu y = 0, which is the wave equation ∂12y−∂22y=0\partial_1^2 y - \partial_2^2 y = 0.

Non-example: the canonical Hamiltonian formulation has one momentum π(x)\pi(x) conjugate to ∂tφ\partial_t \varphi at each point of space. It is not of this form, because it splits spacetime into space and time and uses an infinite-dimensional phase space.

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  1. Differential form concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Hamiltonian_field_theory
About this page
Tag4TK9SZ9T0G
URIm2://4TK9SZ9T0G
Kinddefinition
WritingW0 stub
MSC70S05, 70G45
DefinesCovariant Hamiltonian field theory
UsesFiber bundle, Differential form, Lagrangian density, Legendre transformation
Changed3 November 2026

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