The Physics Travel Guide

Stueckelberg Trick

Prerequisites: Gauge Symmetry, Proca Equation. Full path (23 pages)

Intuitive

A massless particle of spin 1, such as the photon, has two polarization states. A massive spin-1 particle, such as the W or Z boson, has three. The extra one is the longitudinal polarization, which oscillates along the direction of motion. The theory of a massive vector field written in the simplest way, by adding a mass term to Maxwell's theory, has no gauge symmetry, and many of the tools developed for gauge theories cannot be used.

The Stueckelberg trick restores the gauge symmetry by adding a new field and at the same time a new redundancy that exactly removes it again. The bookkeeping is the same as rewriting a function of one variable as a function of two variables that depends only on their difference. Nothing physical changes: the number of degrees of freedom stays the same, and one can always go back to the original description by choosing a gauge in which the new field is zero.

The point of the rewriting is that the new field makes one piece of physics explicit. At energies far above the mass, the longitudinal polarization of the massive vector behaves like a spin-0 particle, and in this regime the Stueckelberg field describes it. Questions about high-energy scattering of massive vector bosons can then be answered by studying a scalar, which is often much easier. The same idea is used for massive gravitons, where the broken symmetry is general coordinate invariance instead of an internal gauge symmetry.

Concrete

[W]e review the implementation of the Stückelberg trick in the theory of massive SU(N)SU(N) YM gauge bosons which, for simplicity, all have the same mass mm, L=−14g2trFμνFμν−m22g2trAμAμ .\begin{align} \mathcal{L}&=-\frac{1}{4g^{2}}{\rm tr}F_{\mu\nu}F^{\mu\nu}-\frac{m^{2}}{2g^{2}}{\rm tr} A_{\mu}A^{\mu}\ . \tag{ 3.22} \end{align}

This lagrangian is not gauge invariant, but gauge invariance can be restored by coupling in new fields, πa(x)\pi^{a}(x), with a∈{1,…,N2−1}a\in\{1,\ldots,N^2-1\}, i.e. , one field for each generator of SU(N)SU(N). In order to insert the πa(x)\pi^{a}(x)'s appropriately, one first performs a gauge transformation with πa(x)\pi^{a}(x) as the gauge parameter, Aμ⟼U†(π)(Aμ+∂μ)U(π)≡Aμ′Fμν⟼U†(π)FμνU(π)≡Fμν′\begin{align} A_{\mu}&\longmapsto U^\dagger(\pi)(A_{\mu}+\partial_{\mu})U(\pi)\equiv A'_{\mu} \\ F_{\mu\nu}&\longmapsto U^\dagger(\pi) F_{\mu\nu}U(\pi)\equiv F'_{\mu\nu} \end{align} where U(π)=eπa(x)TaU(\pi)=e^{\pi^{a}(x)T_{a}} is an element of SU(N)SU(N). We then define a new lagrangian L′\mathcal{L}' by taking (3.22) and replacing Aμ↦Aμ′A_{\mu}\mapsto A_{\mu}' and Fμν↦Fμν′F_{\mu\nu}\mapsto F_{\mu\nu}'. That is, L′=−14g2trFμν′F′μν−m22g2trAμ′A′μ= ⁣−14g2 ⁣trFμνFμν ⁣− ⁣m22g2trDμU(π)DμU†(π) ,\begin{align} \mathcal{L}'&=-\frac{1}{4g^{2}}{\rm tr}F'_{\mu\nu}F'^{\mu\nu}-\frac{m^{2}}{2g^{2}}{\rm tr}A'_{\mu}A'^{\mu} \\ &=\!-\frac{1}{4g^{2}}\!{\rm tr}F_{\mu\nu}F^{\mu\nu}\!-\!\frac{m^{2}}{2g^{2}} {\rm tr}D_{\mu}U(\pi)D^{\mu}U^\dagger(\pi)~, \end{align} where DμU(π)=∂μU(π)+AμU(π)D_{\mu}U(\pi)= \partial_{\mu}U(\pi)+A_{\mu}U(\pi) is the gauge covariant derivative of U(π)U(\pi). The lagrangian L′\mathcal{L}' then enjoys a gauge symmetry under which we simultaneously change Aμ⟼V†(x)(Aμ+1∂μ)V(x)U(π)⟼V†(x)U(π) ,\begin{align} A_{\mu}&\longmapsto V^\dagger(x)(A_{\mu}+ {1}\partial_{\mu})V(x) \\ U(\pi)&\longmapsto V^\dagger(x)U(\pi)~, \end{align} where V(x)∈SU(N)V(x)\in SU(N).

The physics of the L\mathcal{L} and L′\mathcal{L}' lagrangians is the same, we have just made the degrees of freedom in Eq. (3.22) manifest. In L′\mathcal{L}', we introduced N2−1N^{2}-1 new fields, but also restored N2−1N^{2}-1 gauge symmetries and hence degree of freedom counting is the same for both cases. We can demonstrate the equivalence explicitly by using the gauge symmetry of L′\mathcal{L}' to go ``unitary gauge" in which we set U(π)→1U(\pi)\to {1}, where the two lagrangians coincide.

The above process and its generalizations are known collectively as the Stückelberg trick, which is often a useful tool for elucidating the physics in certain regimes of theories, especially at high energies.

https://arxiv.org/abs/1405.5532

Abstract

Abelian case. With metric signature (+,−,−,−)(+,-,-,-), the Proca Lagrangian L=−14FμνFμν+12m2AμAμ\mathcal{L}=-\tfrac14F_{\mu\nu}F^{\mu\nu}+\tfrac12m^2A_\mu A^\mu is not invariant under Aμ→Aμ+∂μλA_\mu\to A_\mu+\partial_\mu\lambda. Replacing Aμ→Aμ−1m∂μϕA_\mu\to A_\mu-\tfrac1m\partial_\mu\phi gives L′=−14FμνFμν+12m2AμAμ−m Aμ∂μϕ+12∂μϕ ∂μϕ,\mathcal{L}'=-\tfrac14F_{\mu\nu}F^{\mu\nu}+\tfrac12m^2A_\mu A^\mu-m\,A^\mu\partial_\mu\phi+\tfrac12\partial_\mu\phi\,\partial^\mu\phi , which is invariant under Aμ→Aμ+∂μλA_\mu\to A_\mu+\partial_\mu\lambda, ϕ→ϕ+mλ\phi\to\phi+m\lambda. The gauge ϕ=0\phi=0 (unitary gauge) gives back the Proca theory. Alternatively, the gauge fixing term −12ξ(∂μAμ+ξmϕ)2-\frac{1}{2\xi}(\partial_\mu A^\mu+\xi m\phi)^2 cancels the mixing term −mAμ∂μϕ-mA^\mu\partial_\mu\phi up to a total derivative. The vector then has the propagator of the RξR_\xi gauges, which falls off like 1/k21/k^2 at large momentum, and ϕ\phi becomes a field of mass squared ξm2\xi m^2 whose contributions cancel against the unphysical vector modes in physical amplitudes. For a vector coupled to a conserved current the abelian theory is renormalizable.

General structure. Let GG be a gauge group and L[A]\mathcal{L}[A] a Lagrangian that is not GG-invariant. Introduce a field U:M→GU:M\to G and define L′[A,U]=L[AU]\mathcal{L}'[A,U]=\mathcal{L}[A^U], where AU=U−1AU+U−1dUA^U=U^{-1}AU+U^{-1}dU is the gauge transform of AA by UU. Under a gauge transformation VV, acting as A→AVA\to A^V and U→V−1UU\to V^{-1}U, we have AU→(AV)V−1U=AUA^U\to (A^V)^{V^{-1}U}=A^U, so L′\mathcal{L}' is invariant. The gauge U=1U=1 recovers L\mathcal{L}, so the two theories are equivalent. For a mass term tr⁡AμAμ\operatorname{tr}A_\mu A^\mu the result is a GG-valued nonlinear sigma model coupled to the gauge field, which is the limit of a Higgs model in which the radial Higgs modes are infinitely heavy. When only a subgroup H⊂GH\subset G is unbroken, the Stueckelberg fields take values in the coset G/HG/H. Stueckelberg fields are therefore Goldstone bosons in a nonlinear realization of the gauge symmetry.

Equivalence theorem. For momentum kμk^\mu with energy E≫mE\gg m the longitudinal polarization vector satisfies ϵLμ=kμ/m+O(m/E)\epsilon_L^\mu=k^\mu/m+O(m/E). In the Stueckelberg description this means that amplitudes with external longitudinal vectors agree, at leading order in m/Em/E, with amplitudes in which they are replaced by the Stueckelberg scalars (the Goldstone boson equivalence theorem). In the non-abelian case the sigma model interactions are nonrenormalizable, with derivative couplings suppressed by m/gm/g, and tree-level unitarity of longitudinal vector scattering fails at energies of order 4πm/g4\pi m/g unless new states, such as a Higgs boson, appear. In massive gravity the same construction applied to diffeomorphisms introduces Stueckelberg fields that restore general covariance, and their scalar part controls the strong coupling scale of the theory.

Path to this page

  1. Calculus
  2. Imaginary Numbers
  3. Linear Algebra
  4. Functional
  5. Group Theory
  6. Legendre Transformation
  7. Newton's Second Law
  8. Vector Calculus
  9. Coulomb's law
  10. Newtonian Mechanics
  11. Symmetry
  12. Variational Calculus
  13. Configuration Space
  14. Euler-Lagrange Equations
  15. Maxwell Equations
  16. Special Relativity
  17. Lagrangian Formalism
  18. Phase Space
  19. Gauge Symmetry
  20. Hamiltonian Formalism
  21. Schrödinger Equation
  22. Klein-Gordon Equation
  23. Proca Equation