Conductance distribution near the Anderson transition
I. M. Suslov (P.L. Kapitza Institute for Physical Problems, Moscow)

TL;DR
This paper introduces a two-parameter family of conductance distributions near the Anderson transition, unifying metallic, localized, and critical regimes through differential equations and analyzing their asymptotic behaviors.
Contribution
It develops a novel theoretical framework using differential equations to describe conductance distributions across different phases near the Anderson transition.
Findings
Distribution exhibits log-normal and exponential asymptotics.
Universal properties depend on two parameters related to system size and correlation length.
Critical distribution in three dimensions is well described by the theory.
Abstract
Using a modification of the Shapiro approach, we introduce the two-parameter family of conductance distributions W(g), defined by simple differential equations, which are in the one-to-one correspondence with conductance distributions for quasi-one-dimensional systems of size L^{d-1}\times L_z, characterizing by parameters L/\xi and L_z/L (\xi is the correlation length, d is the dimension of space). This family contains the Gaussian and log-normal distributions, typical for the metallic and localized phases. For a certain choice of parameters, we reproduce the results for the cumulants of conductance in the space dimension d=2+\epsilon obtained in the framework of the \sigma-model approach. The universal property of distributions is existence of two asymptotic regimes, log-normal for small g and exponential for large g. In the metallic phase they refer to remote tails, in the critical…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
