Axial anomaly effects in finite isospin in a magnetic field
Abstract
In this paper, we consider finite isospin chiral perturbation theory including the effects of the axial anomaly (through the Wess-Zumino-Witten term) in a strong magnetic field. We firstly prove that in a strong external magnetic field (H ext) or more precisely the Schwinger limit, where photon back-reactions are suppressed, only neutral pions can condense and the condensation of charged pions is forbidden. Secondly, we find that the π0 domain wall is an example of a phase that can exist in a strong magnetic field and suggest the existence of a new phase transition line from the normal vacuum state to the π0 domain wall state. This phase transition exists for non-zero pion masses if the baryon chemical potential exceeds a critical value 16π fπ2mπ/eH ext. The phase transition line persists away from the Schwinger limit when the photons can back-react to the external magnetic field.
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