Recognition: unknown
Finite Temperature Schwinger Model
read the original abstract
The temperature dependence of the order parameter of the Schwinger model is calculated in the euclidean functional integral approach. For that we solve the model on a finite torus and let the spatial extension tend to infinity at the end of the computations. The induced actions, fermionic zero-modes, relevant Green functions and Wilson loop correlators on the torus are derived. We find the analytic form of the chiral condensate for any temperature and in particular show that it behaves like \< \bar\Psi\Psi \> \sim -2 T\exp(-\pi\sqrt{\pi}T/e) for temperatures large compared to the induced photon mass.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
de Sitter Vacua & pUniverses
The p-Schwinger model on de Sitter space supports p distinct de Sitter-invariant vacua that are Hadamard, and coupling a multi-flavor version to gravity yields a semiclassical de Sitter saddle at large N_f.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.