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Schwinger model
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In quantum field theory, the Schwinger model is a model describing 1+1D (time + 1 spatial dimension) quantum electrodynamics (QED) which includes , coupled to photons. It is named after named after who developed it in 1962.

The model defines the usual QED Lagrangian density

\mathcal{L} = - \frac{1}{4g^2}F_{\mu \nu}F^{\mu \nu} + \bar{\psi} (i \gamma^\mu D_\mu -m) \psi

over a with one spatial dimension and one temporal dimension. Where F_{\mu \nu} = \partial_\mu A_\nu - \partial_\nu A_\mu is the photon field strength with symmetry group \mathrm{U}(1) (), D_\mu = \partial_\mu - iA_\mu is the gauge covariant derivative, \psi is the , m is the fermion mass and \gamma^0, \gamma^1 form the two-dimensional representation of the .

This model exhibits confinement of the fermions and as such, is a toy model for quantum chromodynamics. A handwaving argument why this is so is because in two dimensions, classically, the potential between two charged particles goes linearly as r, instead of 1/r in 4 dimensions, 3 spatial, 1 time. This model also exhibits a spontaneous symmetry breaking of the U(1) symmetry due to a chiral condensate due to a pool of . The in this model becomes a massive particle at low temperatures. This model can be solved exactly and is used as a for other more complex theories.

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