Dimensional Regularization

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SUMMARY

The discussion focuses on the nuances of dimensional regularization in quantum field theory, specifically the choice between using \(d = 4 - \epsilon\) and \(d = 4 - 2\epsilon\). It concludes that while both forms are mathematically valid, the factor of 2 is primarily for convenience and does not affect physical outcomes. The technique maintains Lorentz invariance and respects gauge symmetries, although complications arise with 4-dimensional specific objects like the Levi-Civita tensor and \(\gamma_5\). The discussion highlights the importance of these concepts in addressing chiral anomalies in QED and QCD.

PREREQUISITES
  • Understanding of dimensional regularization in quantum field theory
  • Familiarity with Feynman diagrams and loop integrals
  • Knowledge of Lorentz invariance and gauge symmetries
  • Basic concepts of chiral anomalies and the role of \(\gamma_5\)
NEXT STEPS
  • Study the mathematical foundations of dimensional regularization
  • Explore the implications of chiral anomalies in quantum electrodynamics (QED)
  • Learn about the 't Hooft-Veltman resolution of \(\gamma_5\) in arbitrary dimensions
  • Investigate the role of the Levi-Civita tensor in quantum field theories
USEFUL FOR

Quantum field theorists, particle physicists, and researchers dealing with gauge theories and regularization techniques will benefit from this discussion.

Break1
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Hi guys! I was wondering if there is any difference choosing between d = 4 -e or d = 4 - 2e. If so, what are the impacts ?
 
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The only difference is that 2e will appear in some places instead of e. There is no actual impact on anything physical.
 
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Is it e (elementary charge) or ##\epsilon##? I think the second.
 
dextercioby said:
Is it e (elementary charge) or ##\epsilon##? I think the second.
Yes!

(Expression would not make sense if it was elementary charge.)
 
The idea behind "dimensional regularization" is to write down the integrals given by loops in Feynman diagrams in ##d## space-time dimensions and read the results as functions of continuous ##d##. Then you do expansions around ##d=4## by setting ##d=4-2\epsilon## and expanding around ##\epsilon=0##. The factor ##2## in the expression is just for a bit more convenience but doesn't really matter in any serious way.

The beauty of this regularization technique is that it obeys a lot of symmetries, i.e., Lorentz invariance and many global and local gauge symmetries.

The only difficulty comes into the game when you deal with objects that are specific to 4 space-time dimensions as the Levi-Civita tensor ##\epsilon^{\mu \nu \rho \sigma}## or (closely related with it) ##\gamma_5## in the Dirac-spinor formalism. This difficulties are, e.g., related to the problem of chiral anomalies, where you can choose, which combination of the vector and axial vector current you want to be not conserved due to the anomaly. In QED and QCD you are forced to break the axial-vector current conservation and keep the vector current conserved, because otherwise you break the local gauge symmetry of these theories, and then they become meaningless. The breaking of the ##\mathrm{U}_{\mathrm{A}}(1)## (accidental) symmetry is, however not a bug but a feature, because it resolves the tension about the decay rate for ##\pi^0 \rightarrow \gamma \gamma## and chiral symmetry.

With this application in mind, there's an ad-hoc resolution of the problem with ##\gamma_5## and arbitrary dimensions, invented by 't Hooft and Veltman: make ##\gamma_5## anticommute with ##\gamma^0 \ldots \gamma^3## and commute with all other ##\gamma## matrices ;-).
 

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