Casimir effect in critical $\mathrm{O}(N)$ models from non-equilibrium Monte Carlo simulations
Andrea Bulgarelli, Michele Caselle, Alessandro Nada, Marco Panero
TL;DR
The paper tackles universal critical Casimir forces in three-dimensional $O(N)$ vector models by developing a non-equilibrium Monte Carlo method to compute the Casimir amplitude $\Delta$ from the second derivative of the excess free energy in a slab geometry. The slab-exchange protocol, coupled with Jarzynski's equality, provides a direct, primary observable for $\Delta$ and enables systematic control of finite-size effects. High-precision results for $N=1,2,3,4,6$ reveal a non-monotonic dependence on $N$ and show tension with conformal bootstrap estimates, with $N=4$ and $N=6$ reported as new Monte Carlo results. The study emphasizes the role of accurate finite-size analyses and motivates larger-$N$ investigations and improved $1/N$ corrections to understand convergence to the large-$N$ limit.
Abstract
$\mathrm{O}(N)$ vector models in three dimensions, when defined in a geometry with a compact direction and tuned to criticality, exhibit long-range fluctuations which induce a Casimir effect. The strength of the resulting interaction is encoded in the excess free-energy density, which depends on a universal coefficient: the Casimir amplitude. We present a high-precision numerical calculation of the latter, by means of a novel non-equilibrium Monte Carlo algorithm, and compare our findings with results obtained from large-$N$ expansions and from the conformal bootstrap.
