Abstract
Renormalized perturbation-theory methods with dimensional regularization are applied to the localization transition of electrons in random potentials within a field theory where the generating functional is the configurational averaged Znav for Z the vacuum-to-vacuum amplitude expressed as a functional integral over Grassman fields, in the replica limit n=0. The bare parameters of the theory are the Fermi level E0 and the variance of the random potential W0. Power counting says that at dimensionality d=2+ε the theory is super-renormalizable. Renormalization of the inverse propagator by the definition of renormalized Fermi level and interaction, EF and u=(πW0EF)κd2, respectively, in order to cancel the single dimensional pole, leads to the same Wilson function β(u) as for the compact nonlinear σ model when the scale parameter κ is varied at constant W0E0. The conductivity is calculated in a perturbation expansion in (τEF)1, with τ1=πW0EFd21 being the inverse lifetime, at d=2+ε. It is explicitly shown that in ultraviolet-divergent d-dimensional loop integrals over advanced and retarded propagators, the leading term is regular while the dimensional pole occurs in the next-to-leading term. Then to leading order the conductivity σ0(ω) is regular while the first correction that includes the diffusion modes has a dimensional pole with residue (iωκ2)ε2. To cancel this pole a renormalized inverse conductance t(u) is defined, and the new Wilson function β(t) obtained by varying κ at constant "bare" interaction W0EF coincides with the scaling theory of Abrahams, Anderson, Licciardello, and Ramakrishnan. Scaling laws are derived from the solution of the renormalization-group equation for the conductivity.