Dimensional Regularization

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Discussion Overview

The discussion centers on the differences between using dimensional regularization with different definitions of the dimensional parameter \(d\), specifically \(d = 4 - \epsilon\) versus \(d = 4 - 2\epsilon\). Participants explore the implications of these choices in the context of Feynman diagrams and the associated mathematical and physical interpretations.

Discussion Character

  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that the only difference between using \(d = 4 - \epsilon\) and \(d = 4 - 2\epsilon\) is the appearance of the factor of 2 in certain expressions, with no significant impact on physical outcomes.
  • There is a question regarding whether \(e\) refers to the elementary charge or to \(\epsilon\), with a consensus leaning towards \(\epsilon\) as the intended variable.
  • One participant explains that dimensional regularization involves treating integrals in \(d\) dimensions and expanding around \(d=4\) by setting \(d=4-2\epsilon\), emphasizing that the factor of 2 is for convenience.
  • The discussion highlights that dimensional regularization maintains various symmetries, including Lorentz invariance and gauge symmetries, but introduces complications when dealing with objects specific to 4-dimensional space-time, such as the Levi-Civita tensor and \(\gamma_5\).
  • There is mention of the chiral anomaly problem and how it relates to the conservation of vector and axial-vector currents in quantum electrodynamics (QED) and quantum chromodynamics (QCD), with a reference to a resolution proposed by 't Hooft and Veltman regarding the treatment of \(\gamma_5\).

Areas of Agreement / Disagreement

Participants express differing views on the significance of the choice between \(d = 4 - \epsilon\) and \(d = 4 - 2\epsilon\), indicating that the discussion remains somewhat unresolved regarding the implications of these choices.

Contextual Notes

Some limitations include the dependence on the definitions of the parameters involved and the unresolved nature of the implications of using different forms of dimensional regularization.

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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