Dimensional regularization and renormalization scale.

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SUMMARY

The discussion centers on the introduction of a renormalization scale ##\mu## in dimensional regularization within quantum field theory (QFT). Ryder advocates for its use to maintain the dimensionless nature of the coupling constant in the Lagrangian, while Weinberg and Peskin & Schroeder do not adopt this approach uniformly. The pros of introducing the scale include clarity in calculations and avoidance of dimensionful logarithmic arguments, which can lead to confusion. The debate highlights the subjective nature of methodological preferences in QFT, particularly regarding the treatment of renormalization and dimensional regularization.

PREREQUISITES
  • Understanding of quantum field theory (QFT) principles
  • Familiarity with dimensional regularization techniques
  • Knowledge of renormalization group concepts
  • Proficiency in handling logarithmic functions in theoretical physics
NEXT STEPS
  • Study Ryder's approach to dimensional regularization and its implications
  • Examine Weinberg's methodology in electrodynamics, particularly chapter 11 of volume 1
  • Explore the on-shell renormalization scheme and its applications
  • Investigate the implications of dimensionful arguments in logarithmic calculations in QFT
USEFUL FOR

The discussion is beneficial for theoretical physicists, quantum field theorists, and students seeking a deeper understanding of renormalization techniques and dimensional regularization in QFT.

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Hi. I have observed that Ryder in his book on QFT before doing dimensional regularization introduces a scale ##\mu## in order to keep the coupling constant dimensionless in the lagragnian. However in two other books; Weinberg and Peskin and Schroeder, they do not introduce this scale in the same way. Is it really up to preference if one wants to do this or not? If so what are the pro's and con's by introducing the scale in this way? And why is it up to one to choose?

Personally I feel that the most natural way to introduce a scale is through the renormalization prescription; for example ##i\Gamma^{(4)}(\mu) = g_R## in ##\phi^4## theory.
 
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Don't use Peskin Schroeder on this issue. In this book you find logarithms with dimensionful arguments, and this even in the very chapter on the renormalization group! This can only lead to confusion! There must never ever by dimensionful quantities in logarithms (or any other transcendental function for that matter).

Weinberg choses not to introduce the scale in the chapter on electrodynamics (ch. 11 in vol. 1), but he manages to never have logarithms with dimensionful quantities by the trick of directly calculating the renormalized values of the photon-field normalization factor Z_3 by doing the appropriate subtraction of the photon-polarization tensor (or photon self-energy) at the photon momentum 0, i.e., in the on-shell scheme, which is allowed as long as you keep the Dirac fields massive. In this way he directly can calculate the value for d \rightarrow 4, without ever having dimensionful arguments of logarithms.

Personally, I don't like this, because it is way more clear to calculate the regularized but unrenormalized values first, and there you must introduce a scale in order to avoid dimensionful arguments of the logarithms when doing the Laurent expansion around d=4, and that's where the renormalization scale enteres in dimensional regularization.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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