Dynamical random field Ising model at zero temperature
Jian Ding, Peng Yang, Zijie Zhuang
TL;DR
The paper studies the zero-temperature evolution of the RFIM as the external-field mean M increases, comparing ground-state evolution with zero-temperature Glauber dynamics. It establishes a sharp dimension-dependent picture: in 2D there is no global avalanche for any disorder strength, while in d≥3 a disorder-driven phase transition governs the occurrence of global avalanches, with small ε yielding a macroscopic flip and large ε suppressing it. A central methodological contribution is a multi-scale, isoperimetric approach that connects RFIM dynamics to polluted bootstrap percolation, enabling precise probabilistic control of flip sets and triggering times. The work also develops a rigorous polluted bootstrap percolation framework and leverages it to derive threshold results and to solve an open problem in Gravner-Holroyd-3D, with extensions to Glauber dynamics at positive temperature and open questions for higher dimensions. Overall, the paper provides a cohesive, dimension-aware treatment of dynamical RFIM behavior at zero temperature and establishes deep connections to percolation theory and multi-scale energy-change control.
Abstract
In this paper, we study the evolution of the zero-temperature random field Ising model as the mean of the external field $M$ increases from $-\infty$ to $\infty$. We focus on two types of evolutions: the ground state evolution and the Glauber evolution. For the ground state evolution, we investigate the occurrence of global avalanche, a moment where a large fraction of spins flip simultaneously from minus to plus. In two dimensions, no global avalanche occurs, while in three or higher dimensions, there is a phase transition: a global avalanche happens when the noise intensity is small, but not when it is large. Additionally, we study the zero-temperature Glauber evolution, where spins are updated locally to minimize the Hamiltonian. Our results show that for small noise intensity, in dimensions $d =2$ or $3$, most spins flip around a critical time $c_d = \frac{2 \sqrt{d}}{1 + \sqrt{d}}$ (but we cannot decide whether such flipping occurs simultaneously or not). We also connect this process to polluted bootstrap percolation and solve an open problem on it.
