We consider the parabolic Anderson model (PAM) on the n-dimensional hypercube with random i.i.d. potentials. We parametrize time by volume and study the solution at the location of the k-th largest potential. Our main result is that, for a certain class of potential distributions, the solution exhibits a phase transition: for short time scales it behaves like a system without diffusion, whereas, for long time scales the growth is dictated by the principle eigenvalue and the corresponding eigenfunction of the Anderson operator, for which we give precise asymptotics. Moreover, the transition time depends only on the difference between the largest and k-th largest potential. One of our main motivations in this article is to investigate the mut...
We consider the parabolic Anderson model (PAM) which is given by the equation ¿u=¿t = k¿u+¿u with u:...
We consider the solution u:[0,∞)×Zd→[0,∞) to the parabolic Anderson model, where the potential is...
We continue our study of the parabolic Anderson equation ¿u/¿t =k¿u+¿¿u for the space-time field u: ...
We consider the parabolic Anderson model (PAM) on the n-dimensional hypercube with random i.i.d. pot...
We consider branching particle processes on discrete structures like the hypercube in a random fitne...
International audienceThe parabolic Anderson model is defined as the partial differential equation ∂...
This is a comprehensive survey on the research on the parabolic Anderson model – the heat equation w...
We study the long-time asymptotics of the total mass of the solution to the parabolic Anderson model...
We discuss the long time behaviour of the parabolic Anderson model, the Cauchy problem for the heat ...
30 pagesInternational audienceThe parabolic Anderson model is defined as the partial differential eq...
We investigate a variant of the parabolic Anderson model, introduced in previous work, i...
We consider branching particle processes on discrete structures like the hypercube in a random fitne...
This thesis studies global solutions to the semidiscrete stochastic heat equation and the associated...
35 pages, 4 figures.International audienceWe continue our study of the parabolic Anderson equation $...
We study the long-time asymptotics of the total mass of the solution to the parabolic Anderson model...
We consider the parabolic Anderson model (PAM) which is given by the equation ¿u=¿t = k¿u+¿u with u:...
We consider the solution u:[0,∞)×Zd→[0,∞) to the parabolic Anderson model, where the potential is...
We continue our study of the parabolic Anderson equation ¿u/¿t =k¿u+¿¿u for the space-time field u: ...
We consider the parabolic Anderson model (PAM) on the n-dimensional hypercube with random i.i.d. pot...
We consider branching particle processes on discrete structures like the hypercube in a random fitne...
International audienceThe parabolic Anderson model is defined as the partial differential equation ∂...
This is a comprehensive survey on the research on the parabolic Anderson model – the heat equation w...
We study the long-time asymptotics of the total mass of the solution to the parabolic Anderson model...
We discuss the long time behaviour of the parabolic Anderson model, the Cauchy problem for the heat ...
30 pagesInternational audienceThe parabolic Anderson model is defined as the partial differential eq...
We investigate a variant of the parabolic Anderson model, introduced in previous work, i...
We consider branching particle processes on discrete structures like the hypercube in a random fitne...
This thesis studies global solutions to the semidiscrete stochastic heat equation and the associated...
35 pages, 4 figures.International audienceWe continue our study of the parabolic Anderson equation $...
We study the long-time asymptotics of the total mass of the solution to the parabolic Anderson model...
We consider the parabolic Anderson model (PAM) which is given by the equation ¿u=¿t = k¿u+¿u with u:...
We consider the solution u:[0,∞)×Zd→[0,∞) to the parabolic Anderson model, where the potential is...
We continue our study of the parabolic Anderson equation ¿u/¿t =k¿u+¿¿u for the space-time field u: ...