Gibbs-non-Gibbs dynamical transitions for mean-field interacting Brownian motions
arXiv:1312.3438 · doi:10.1016/j.spa.2014.09.011
Abstract
We consider a system of real-valued spins interacting with each other through a mean-field Hamiltonian that depends on the empirical magnetization of the spins via a general potential. The system is subjected to a stochastic dynamics where the spins perform independent Brownian motions. As in \cite{FedHoMa13}, which considers the Curie-Weiss model with Ising spins interacting via a quadratic potential and subjected to independent spins flips, we follow the program outlined in \cite{vEFedHoRe10}. We show that in the thermodynamic limit the system is non-Gibbs at time if and only if there exists an such that the large deviation rate function for the trajectory of the magnetization conditional on hitting the value at time has multiple global minimizers. We further show that different minimizing trajectories are different at time . We give conditions on the potential under which the system is Gibbs at time , classify the possible scenarios of being Gibbs at time in terms of the second difference quotient of the potential, and show that the system cannot become Gibbs once it has become non-Gibbs, i.e., there is a unique and explicitly computable crossover time from Gibbs to non-Gibbs. We give examples of immediate loss of Gibbsianness (), short-time conservation of Gibbsianness, large-time loss of Gibbsianness (), and preservation of Gibbsianness (). Depending on the potential, the system can be Gibbs or non-Gibbs at the cross-over time time .
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