Abstract

We consider a one dimensional infinite chain of harmonic oscillators whose dynamics is perturbed by a stochastic term conserving energy and momentum. We prove that in the unpinned case the macroscopic evolution of the energy converges to the solution of the fractional diffusion equation $${\partial_t u = -|\Delta|^{3/4}u}$$ . For a pinned system we prove that its energy evolves diffusively, generalizing some results of Basile and Olla (J. Stat. Phys. 155(6):1126–1142, 2014).

Highlights

  • Superdiffusion of energy and the corresponding anomalous thermal conductivity have been observed numerically in the dynamics of unpinned FPU chains [15,16]

  • The problem has been studied in models where the Hamiltonian dynamics is perturbed by stochastic terms that conserve energy and momentum, like random exchange of velocity between nearest neighbors particles [1,2]

  • In the cases when the conductivity is finite it is proven in [4] that energy fluctuations in equilibrium evolve diffusively

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Summary

Introduction

Superdiffusion of energy and the corresponding anomalous thermal conductivity have been observed numerically in the dynamics of unpinned FPU chains [15,16]. While this choice is quite natural in the situation of a pinned chain, it requires some explanation in the unpinned case In the latter situation, if we start with non-centered initial conditions, their respective macroscopic averages will evolve, at the hyperbolic space-time scale, following the linear wave equation. If we start with non-centered initial conditions, their respective macroscopic averages will evolve, at the hyperbolic space-time scale, following the linear wave equation As a result, they will disperse to infinity, since we start with the data whose realization has a finite L2 norm. We mention here the article [6], where a result similar to ours is proven, by very different techniques, for a dynamics with two conserved quantities (energy and volume) in the case when the initial data is given by a Gibbs equilibrium measure.

Main Results
Some Basic Notation
Finite Macroscopic Energy
Fluctuations in Equilibrium
Evolution of the Wigner Transform
11. Identification of the Limit of the Wigner Transform
14. Auxiliary Results
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