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Cosets and Nonlinear Realizations

Once an exact continuous internal symmetry is broken from GG to HH, the Goldstone fields can be treated as local coordinates on G/HG/H. They do not usually form a linear representation of all of GG. Instead, a transformation by gGg\in G moves a chosen coset representative out of its chosen section, and a field-dependent compensator in HH brings it back. The Maurer–Cartan form then separates into a coset vielbein and a composite HH connection; contractions invariant under HH are automatically invariant under the nonlinear action of GG.

This page constructs those local building blocks for exact ordinary internal symmetries in a relativistic phase. It does not decide whether the broken phase exists, count its propagating modes, determine effective-theory coefficients, or develop spacetime-symmetry cosets and inverse-Higgs constraints.

Required background. Vacuum Orbits and Unbroken Subgroups supplies the homogeneous space G/HG/H and its tangent space g/h\mathfrak g/\mathfrak h. Lie Groups, Lie Algebras, and Exponential and Adjoint Maps supplies Lie brackets, exponentials, adjoint actions, and changes of generator basis.

Helpful background. Differential Forms, Integration, Orientation, and Stokes Theorem supplies the one-form and wedge-product language used for the Maurer–Cartan identity.

Let GG be a finite-dimensional compact Lie group, or more generally suppose that the required reductive structure exists, and let HGH\subset G be the closed unbroken subgroup. Choose Hermitian generators TiT_i for h\mathfrak h and representatives XaX_a of the broken directions. We assume an Ad(H)\operatorname{Ad}(H)-stable split

g=hm,hXah1=R(h)abXb.\mathfrak g=\mathfrak h\oplus\mathfrak m, \qquad hX_a h^{-1}=R(h)_a{}^bX_b.

When HH is compact—as it is for a closed subgroup of compact GG—averaging an inner product over HH supplies such a stable complement. For a more general non-reductive homogeneous space, the simple component transformation laws below require refinement.

On a neighborhood of the identity coset, choose the local section

ξ(π)=exp ⁣(iπaXaf),\xi(\pi) =\exp\!\left( \frac{i\pi^aX_a}{f} \right),

where ff is a convenient normalization scale. The exponential is a coordinate choice, not a claim that one chart covers all of G/HG/H.

For gGg\in G, and wherever the transformed point remains in the chosen chart, there is a unique local factorization

gξ(π)=ξ(π)h(g,π),h(g,π)H.g\,\xi(\pi) =\xi(\pi')\,h(g,\pi), \qquad h(g,\pi)\in H.

Equivalently, ξ(π)=gξ(π)h1\xi(\pi')=g\xi(\pi)h^{-1}. This equation defines both the generally nonlinear transformation ππ\pi\mapsto\pi' and the compensator h(g,π)h(g,\pi). Near π=0\pi=0, a broken transformation g=eiϵaXag=e^{i\epsilon^aX_a} begins as

πa=πa+fϵa+O(ϵπ),\pi'^a=\pi^a+f\epsilon^a +O(\epsilon\pi),

whereas an unbroken transformation acts linearly through R(h)R(h). A matter field ψ\psi that carries a representation DD of HH is assigned the nonlinear GG action

ψ(x)=D ⁣(h(g,π(x)))ψ(x).\psi'(x) =D\!\left(h(g,\pi(x))\right)\psi(x).

The compensators obey the composition rule

h(g2g1,π)=h(g2,g1π)×h(g1,π),\begin{aligned} h(g_2g_1,\pi) &=h(g_2,g_1\mathbin{\cdot}\pi) \\ &\qquad\times h(g_1,\pi), \end{aligned}

so these field transformations realize the group law. This local factorization and the induced HH action are developed in Weinberg 1995, § 19.6, pp. 211–217; the general Goldstone-coordinate viewpoint is summarized in Schwartz 2014, § 28.2.4, pp. 573–574.

A different local section replaces ξ(π)\xi(\pi) by ξ(π)k(π)\xi(\pi)k(\pi) with k(π)Hk(\pi)\in H, together with a coordinate redefinition. It changes the compensator and the intermediate components below, but not the GG-invariant theory. The compensator is therefore not an additional propagating field.

The Maurer–Cartan vielbein and composite connection

Section titled “The Maurer–Cartan vielbein and composite connection”

Pull back the left-invariant Maurer–Cartan form along the section and use Hermitian generators:

Ω(π)iξ1dξ=eaXa+ωiTi.\begin{aligned} \Omega(\pi) &\equiv-i\xi^{-1}\mathrm d\xi \\ &=e^aX_a+\omega^iT_i. \end{aligned}

Here e=eaXae=e^aX_a is the broken component and ω=ωiTi\omega=\omega^iT_i is the unbroken component. Under a constant gGg\in G, write h=h(g,π)h=h(g,\pi) and use ξ=gξh1\xi'=g\xi h^{-1}. Direct differentiation gives

Ω=hΩh1ihdh1.\Omega' =h\Omega h^{-1} -i h\,\mathrm d h^{-1}.

Because the complement m\mathfrak m is Ad(H)\operatorname{Ad}(H) stable, the two components transform separately:

eaXa=h(eaXa)h1,ωiTi=h(ωiTi)h1ihdh1.\begin{aligned} e'^aX_a &=h(e^aX_a)h^{-1}, \\ \omega'^iT_i &=h(\omega^iT_i)h^{-1} -i h\,\mathrm d h^{-1}. \end{aligned}

Thus ee transforms homogeneously, like a coframe on the coset, while ω\omega has the inhomogeneous term of an HH connection. After π=π(x)\pi=\pi(x), eμe_\mu is the pullback of this target-space coframe; it is not a gravitational spacetime vielbein. The connection ω\omega is a composite function of the Goldstone coordinates, not a new microscopic gauge field.

Writing

Π=πaXaf,\Pi=\frac{\pi^aX_a}{f},

the Baker–Campbell–Hausdorff expansion provides a sign check:

Ω=dΠi2[Π,dΠ]+O(Π2dΠ).\Omega =\mathrm d\Pi -\frac{i}{2}[\Pi,\mathrm d\Pi] +O(\Pi^2\mathrm d\Pi).

In particular, ea=dπa/f+e^a=\mathrm d\pi^a/f+\cdots. The full form also satisfies the Maurer–Cartan identity

dΩ+iΩΩ=0.\mathrm d\Omega+i\Omega\wedge\Omega=0.

This is a geometric identity, not an equation of motion. The transformation laws and their use in invariant interactions are derived in Weinberg 1995, § 19.6, pp. 215–220.

On spacetime, write

ea=eμadxμ,ωi=ωμidxμ.\begin{aligned} e^a&=e_\mu^a\,\mathrm dx^\mu, \\ \omega^i&=\omega_\mu^i\,\mathrm dx^\mu. \end{aligned}

If tit_i are the Hermitian HH generators in the representation of ψ\psi, define

μψ=(μ+iωμiti)ψ.\nabla_\mu\psi =\left( \partial_\mu+i\omega_\mu^i t_i \right)\psi.

The inhomogeneous term in ω\omega' cancels the derivative of the field-dependent compensator, giving

(μψ)=D(h)μψ.(\nabla_\mu\psi)' =D(h)\nabla_\mu\psi.

The sign is tied to the definition Ω=iξ1dξ\Omega=-i\xi^{-1}\mathrm d\xi and the convention ψ=D(h)ψ\psi'=D(h)\psi.

Let gabg_{ab} be an HH-invariant positive target-space metric on the broken representation:

gabR(h)acR(h)bd=gcd.g_{ab}R(h)^a{}_cR(h)^b{}_d =g_{cd}.

The leading Lorentz-invariant Goldstone term is then

L2=f22gabeμaeμb.\mathcal L_2 =\frac{f^2}{2}\, g_{ab}e_\mu^ae^{\mu b}.

If m\mathfrak m splits into inequivalent HH representations, there can be several independent invariant tensors and therefore several coefficients already at this order. Symmetry determines the allowed contractions, not their numerical values.

More generally, any local HH-singlet constructed from eμe_\mu, ψ\psi, μψ\nabla_\mu\psi, and their covariant derivatives is invariant under the nonlinear action of GG. An exact internal symmetry forbids a nonconstant invariant potential on a transitive coset, so undifferentiated Goldstone coordinates cannot acquire an ordinary mass term. Integrations by parts, equations of motion, and dimension-specific identities can still make an apparently distinct local basis redundant.

This construction captures strictly invariant local terms. Wess–Zumino terms, which may shift by a total derivative, require global and cohomological information beyond one chart. Power counting, loop renormalization, matching, and model-dependent coefficients belong to Renormalization and Effective Field Theory.

For SO(3)SO(2)SO(3)\to SO(2), let HH be generated by J3J_3 and take X1=J1X_1=J_1, X2=J2X_2=J_2, with

[Ji,Jj]=iϵijkJk.[J_i,J_j]=i\epsilon_{ijk}J_k.

The local coset is a patch of S2S^2. Substituting

Π=π1J1+π2J2f\Pi=\frac{\pi^1J_1+\pi^2J_2}{f}

into the expansion of Ω\Omega gives

e1=dπ1f+O ⁣(π2dπf3),e2=dπ2f+O ⁣(π2dπf3),ω3=π1dπ2π2dπ12f2+O ⁣(π3dπf4).\begin{aligned} e^1 &=\frac{\mathrm d\pi^1}{f} +O\!\left( \frac{\lVert\pi\rVert^2\mathrm d\pi}{f^3} \right), \\ e^2 &=\frac{\mathrm d\pi^2}{f} +O\!\left( \frac{\lVert\pi\rVert^2\mathrm d\pi}{f^3} \right), \\ \omega^3 &=\frac{ \pi^1\mathrm d\pi^2 -\pi^2\mathrm d\pi^1 }{2f^2} \\ &\qquad +O\!\left(\frac{\pi^3\mathrm d\pi}{f^4}\right). \end{aligned}

The pair (e1,e2)(e^1,e^2) rotates homogeneously under the unbroken SO(2)SO(2), while ω3\omega^3 supplies its composite connection. The calculation is local: another chart is needed near points where these exponential coordinates cease to be regular.

For the exact global complex-scalar symmetry

G=U(1),H={1},G=U(1), \qquad H=\{1\},

choose the charge-one generator and

ξ(π)=eiπ/f.\xi(\pi)=e^{i\pi/f}.

There is no nontrivial compensator or unbroken connection. A phase rotation by α\alpha gives

ππ+fα,\pi\longmapsto\pi+f\alpha,

with the global identification ππ+2πf\pi\sim\pi+2\pi f, and

Ω=e=dπf.\Omega=e=\frac{\mathrm d\pi}{f}.

The leading invariant is therefore

f22eμeμ=12μπμπ.\frac{f^2}{2}e_\mu e^\mu =\frac12\partial_\mu\pi\,\partial^\mu\pi.

In the weakly coupled scalar model, write locally

ϕ=v+σ2eiπ/f.\phi =\frac{v+\sigma}{\sqrt2} e^{i\pi/f}.

Its kinetic term becomes

μϕμϕ=12(σ)2+(v+σ)22f2(π)2.\begin{aligned} \partial_\mu\phi^\dagger\partial^\mu\phi &=\frac12(\partial\sigma)^2 \\ &\quad +\frac{(v+\sigma)^2}{2f^2} (\partial\pi)^2. \end{aligned}

At tree level and at energies well below the radial mass, setting the leading solution σ=0\sigma=0 and choosing f=vf=v reproduces the canonical Goldstone kinetic term. Eliminating σ\sigma more accurately generates higher-derivative interactions. In the exact interacting theory, ff is a physical low-energy normalization and need not equal a chosen order-parameter expectation value. The angular variable, shift action, and derivative interactions are worked out in Schwartz 2014, § 28.2.1, pp. 564–566. This Abelian example checks the sign and normalization but cannot test a non-Abelian compensator or connection.

Two finite-group statements must be kept distinct. If the exact symmetry is U(1)U(1) but the unbroken subgroup is ZN\mathbb Z_N, then U(1)/ZNU(1)/\mathbb Z_N is still one-dimensional and has a Goldstone coordinate. If a permanent deformation instead reduces the exact phase-rotation group itself to ZN\mathbb Z_N, there is no continuous coset tangent and no exact shift symmetry. The lifted angular mode belongs to Explicit Breaking and Pseudo-Goldstone Modes. A temporary selector removed after the infinite-volume limit does not alter the final exact group and is not retained in the coset action.

  1. Identify the exact physical global group GG and the actual stabilizer HH of the selected phase.
  2. Check that HH is closed and choose a local section of GG/HG\to G/H; for the simple component rules, choose an Ad(H)\operatorname{Ad}(H)-stable complement.
  3. Factor gξ(π)=ξ(π)h(g,π)g\xi(\pi)=\xi(\pi')h(g,\pi) to determine the nonlinear action and compensator.
  4. Compute iξ1dξ-i\xi^{-1}\mathrm d\xi and separate its broken vielbein from its unbroken connection.
  5. Assign non-Goldstone fields to representations of HH and form HH-invariant contractions of the covariant building blocks.
  6. Only then reduce the operator basis and impose power counting, matching, and loop organization in the effective-theory treatment.

This sequence is local in field space. Global patching, defects, Wess–Zumino terms, anomalies, and quantized coefficients need additional information. For broken spacetime symmetries, even the list of independent coordinates can change through demonstrated inverse-Higgs-type redundancies; the internal construction here should not be applied mechanically. See Goldstone Counting, Low-Dimensional Obstructions, and Spacetime Exceptions.

G/HG/H must be a quotient group.” It is a homogeneous space of cosets. It becomes a group only when HH is normal in GG.

“The compensator is a new gauge field.” The compensator is the field-dependent HH transformation that returns a representative to the chosen section. The connection ω\omega is built from π\pi; neither introduces an independent microscopic gauge degree of freedom.

“The exponential representative is global.” It supplies a useful chart near the identity coset. Compact or topologically nontrivial cosets generally require identifications or additional patches.

“The Maurer–Cartan connection transforms homogeneously.” The vielbein does; the connection has an inhomogeneous derivative term. That term is precisely what makes derivatives of HH-multiplet matter fields covariant.

“One coset coordinate always means one propagating mode.” That equality holds for the relativistic internal setting under the counting theorem’s assumptions. At finite density, type-B pairing can reduce the number of modes; spacetime generators can be redundant.

“An unbroken finite subgroup removes every Goldstone field.” If the exact group remains continuous, G/HG/H can still have a continuous tangent even when HH is finite. No continuous coset exists only when the exact symmetry available for the construction is itself finite.

These questions are for self-study and are not graded.

  1. Starting from ξ=gξh1\xi'=g\xi h^{-1} with constant gg, derive the transformation of Ω=iξ1dξ\Omega=-i\xi^{-1}\mathrm d\xi.
  2. Use Ω=dΠi2[Π,dΠ]+\Omega=\mathrm d\Pi-\tfrac{i}{2}[\Pi,\mathrm d\Pi]+\cdots to recover the leading ω3\omega^3 for SO(3)/SO(2)SO(3)/SO(2).
  3. Explain why both U(1)/{1}U(1)/\{1\} and U(1)/ZNU(1)/\mathbb Z_N have one local Goldstone coordinate, while a theory whose exact group is only ZN\mathbb Z_N does not.
Check
  1. Differentiate ξ=gξh1\xi'=g\xi h^{-1} and multiply by ξ1=hξ1g1\xi'^{-1}=h\xi^{-1}g^{-1}:

    ξ1dξ=h(ξ1dξ)h1+hdh1.\xi'^{-1}\mathrm d\xi' =h(\xi^{-1}\mathrm d\xi)h^{-1} +h\,\mathrm d h^{-1}.

    Multiplication by i-i gives

    Ω=hΩh1ihdh1.\Omega' =h\Omega h^{-1} -i h\,\mathrm d h^{-1}.
  2. With Π=(π1J1+π2J2)/f\Pi=(\pi^1J_1+\pi^2J_2)/f and [J1,J2]=iJ3[J_1,J_2]=iJ_3,

    [Π,dΠ]=if2(π1dπ2π2dπ1)J3.[\Pi,\mathrm d\Pi] =\frac{i}{f^2} \left( \pi^1\mathrm d\pi^2 -\pi^2\mathrm d\pi^1 \right)J_3.

    Therefore the unbroken component is

    ω3=π1dπ2π2dπ12f2+.\omega^3 =\frac{ \pi^1\mathrm d\pi^2 -\pi^2\mathrm d\pi^1 }{2f^2} +\cdots.
  3. Dividing a one-dimensional Lie group by either the trivial subgroup or a finite subgroup leaves a one-dimensional homogeneous space locally. By contrast, a finite exact group has a zero-dimensional Lie algebra and no infinitesimal broken direction from which to construct a Goldstone coordinate.

  • Schwartz, Matthew D. Quantum Field Theory and the Standard Model. Cambridge: Cambridge University Press, 2014. DOI.
  • Weinberg, Steven. The Quantum Theory of Fields, Volume II: Modern Applications. Cambridge: Cambridge University Press, 1995. DOI.