Description

We calculate the leading radiative corrections to the axial current in the chiral separation effect in dense QED in a magnetic field. Contrary to the conventional wisdom suggesting that the axial current should be exactly fixed by the chiral anomaly

We calculate the leading radiative corrections to the axial current in the chiral separation effect in dense QED in a magnetic field. Contrary to the conventional wisdom suggesting that the axial current should be exactly fixed by the chiral anomaly relation and is described by the topological contribution on the lowest Landau level in the free theory, we find in fact that the axial current receives nontrivial radiative corrections. The direct calculations performed to the linear order in the external magnetic field show that the nontrivial radiative corrections to the axial current are provided by the Fermi surface singularity in the fermion propagator at nonzero fermion density.

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Title
  • Radiative Corrections to Chiral Separation Effect in QED
Contributors
Date Created
2013
Resource Type
  • Text
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    Identifier
    • Digital object identifier: 10.1103/PhysRevD.88.025025
    • Identifier Type
      International standard serial number
      Identifier Value
      1088-6826
    • Identifier Type
      International standard serial number
      Identifier Value
      0002-9939
    Note
    • Copyright (2013) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. along with the following message: The following article appeared in (Physical Review D, 88(2)) and may be found at (http://journals.aps.org.ezproxy1.lib.asu.edu/prd/abstract/10.1103/PhysRevD.88.025025).

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    This is a suggested citation. Consult the appropriate style guide for specific citation guidelines.

    Gorbar, E. V., Miransky, V. A., Shovkovy, I. A., & Wang, X. (2013). Radiative corrections to chiral separation effect in QED. Physical Review D, 88(2), 025025. doi:10.1103/PhysRevD.88.025025

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