The parabolic Anderson model on the hypercube

preprint2016arXivOpen access

Abstract

We consider the parabolic Anderson model ∂∂tvn=κΔnvn+ξnvn\frac{\partial}{\partial t} v_n=κΔ_n v_n + ξ_n v_n on the nn-dimensional hypercube {−1,+1}n\{-1,+1\}^n with random i.i.d. potential ξnξ_n. We parametrize time by volume and study vnv_n at the location of the kk-th largest potential, xk,2nx_{k,2^n}. Our main result is that, for a certain class of potential distributions, the solution exhibits a phase transition: for short time scales vn(tn,xk,2n)v_n(t_n,x_{k,2^n}) behaves like a system without diffusion and grows as exp⁡{(ξn(xk,2n)−κ)tn}\exp\big\{(ξ_n(x_{k,2^n}) - κ)t_n\big\}, whereas, for long time scales the growth is dictated by the principle eigenvalue and the corresponding eigenfunction of the operator κΔn+ξnκΔ_n+ξ_n, for which we give precise asymptotics. Moreover, the transition time depends only on the difference ξn(x1,2n)−ξn(xk,2n)ξ_n(x_{1,2^n})-ξ_n(x_{k,2^n}). One of our main motivations in this article is to investigate the mutation-selection model of population genetics on a random fitness landscape, which is given by the ratio of vnv_n to its total mass, with ξnξ_n corresponding to the fitness landscape. We show that the phase transition of the solution translates to the mutation-selection model as follows: a population initially concentrated at xk,2nx_{k,2^n} moves completely to x1,2nx_{1,2^n} on time scales where the transition of growth rates happens. The class of potentials we consider involves the Random Energy Model (REM) of statistical physics which is studied as one of the main examples of a random fitness landscape.

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