What is the `physical' meaning of consistent anomalies and covariant anomalies?
Perhaps a good Reference is: Consistent and covariant anomalies in gauge and gravitational theories - William A. Bardeen and Bruno Zumino
I kind of remember (and used to think) that: consistent anomaly=(1/2)(covariant anomaly)
So the physical picture I have is, for example a 1+1D system. See a Reference doi.org/10.1103/PhysRevB.107.014311. Consider this 1+1D theory lives as the edge theory on the boundary of a 2+1D spatial cylinder. There is an (integer) quantum hall state with charge U(1) symmetry.
On the left edge, there is a left-moving current with a `consistent' anomaly ∂μJμL=(e/4π)ϵμνFμν(=consistent anomaly?)
On the right edge, there is a right-moving current with another `consistent' anomaly ∂μJμR=−(e/4π)ϵμνFμν(=−consistent anomaly?)
Consider putting these two edges more-or-less together as the same 1+1D (but without direct interactions), shows axial anomaly: ∂μJμA=∂μ(JμL−JμR)=(e/2π)ϵμνFμν(=covariant anomaly?)
while vector current conserved: ∂μJμV=∂μ(JμL+JμR)=0
At least, this physical picture produces: consistent anomaly=(1/2)(covariant anomaly)
Can someone inform whether this is a right picture or not for the consistent anomalies and covariant anomalies?
This post imported from StackExchange Physics at 2014-06-04 11:40 (UCT), posted by SE-user Idear