RENORMALIZATION GROUP METHODS

Abstract

The method of the renormalization group was originally introduced by Gell-Mann and Low as a means of dealing with the failure of perturbation theory at very high energies in quantum electrodynamics. An n -loop contribution to an amplitude involving momenta of order q , such as the vacuum polarization Π μν ( q ), is found to contain up to n factors of In() as well as a factor α n , so perturbation theory will break down when is large, even though the fine structure constant a is small. Even in a massless theory like a non-Abelian gauge theory we must introduce some scale μ to specify a renormalization point at which the renormalized coupling constants are to be defined, and in this case we encounter logarithms In( E /μ), so that perturbation theory may break down if E ≫ μ or E ≪ μ, even if the coupling constant is small. Fortunately, there is a modified version of perturbation theory that can often be used in such cases. The key idea of this approach consists in the introduction of coupling constants g μ defined at a sliding renormalization scale μ — that is, a scale that is not related to particle masses in any fixed way. By then choosing μ to be of the same order of magnitude as the energy E that is typical of the process in question, the factors In( E /μ) are rendered harmless. We can then do perturbation theory as long as g μ remains small.