For an infinitesimal spacetime-dependent parameter, the action variation has the Noether current formIn canonical quantization, apply the corresponding transformation inside an equal-time correlation function. Integrating the resulting Ward-Takahashi identity over a thin time interval around an insertion givesComparison with yieldsin the conventions of the question. Current conservation makes time independent when the surface flux vanishes, so the same charge generates the symmetry at every time.
A symmetry generated by is spontaneously broken when the vacuum is not invariant:A local order parameter is obtained by finding a field for whichwith the sign depending on the commutator convention. This criterion is useful in infinite volume because it can remain finite even when the spatially integrated charge itself is not a well-defined normalizable operator.
For an unbroken internal symmetry, and . If , then is either zero or another state of the same energy, so particles fill degenerate symmetry multiplets.
In a spontaneously broken phase, applying the finite symmetry changes the vacuum and moves to a distinct infinite-volume superselection sector. The charge is not a well-defined finite-norm operator within one such sector, so the usual argument that is a physical partner state can fail; particle masses need not occur in multiplets of the broken group. Formally, however,Thus the broken directions are degenerate with the vacuum. In a local relativistic theory these zero-energy, long-wavelength excitations become the Goldstone bosons.
Goldstone's theorem states that every spontaneously broken generator of a continuous global internal symmetry gives a massless scalar excitation in a Lorentz-invariant quantum field theory, subject to the standard locality and positivity assumptions.
Choose a local field with and write . Translation invariance givesLorentz covariance forces the contribution of a spin-zero intermediate state to have . Current conservation then implies . The nonzero equal-time integral demanded by the order parameter rules out , so the spectral density must contain support at . Hence there is a massless one-particle pole withwhich is the required Goldstone boson. Independent broken generators give independent massless modes in the ordinary relativistic case.
Up to a vacuum-energy constant and the topological Abelian term, the most general renormalizable Abelian Higgs model isIt has three local dynamical parameters, . Stability requires , and spontaneous symmetry breaking occurs for . Writingand choosing unitary gauge removes . The physical masses areThe interactions include , , , and . The original massless vector's two polarizations and the complex scalar's two real components become a massive vector with three polarizations and one massive scalar. This rearrangement, in which the gauge field absorbs the would-be Goldstone mode and acquires mass without explicitly breaking gauge invariance, is the Higgs mechanism.
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