Thermodynamic integration, fermion sign problem, and real-space renormalization
Koka Sathwik, Werner Krauth
TL;DR
This work reexamines real-space renormalization for the 2D Ising model by retracing Wilson’s real-space decimation using unbiased Monte Carlo sampling and thermodynamic integration. It implements a modified decimation with coupling parameter $\rho$ to avoid identifications that spoil critical scaling, and develops a Monte Carlo framework that also contends with the emergent fermion sign problem through an absolute-value reformulation and a correlated-sampling strategy. The study analyzes two-factor and fourteen-factor interaction sets on the Wilson patch, locating perturbative fixpoints and showing the sign problem remains manageable for practical parameter ranges, with significant precision gains from correlated sampling. The results illuminate the feasibility of Wilson’s program in a modern computational setting and suggest pathways to generalize real-space renormalization beyond simple models, while acknowledging open questions about uniqueness and universality.
Abstract
We reconsider real-space renormalization for the two-dimensional Ising model, following the path traced out by Wilson in Sect. VI of his 1975 Reviews of Modern Physics. In that reference, Wilson considerably extended the Kadanoff decimation procedure towards a possibly rigorous construction of a real-space scale-invariant hamiltonian. Wilson's construction has, to the best of our knowledge, never been fully understood and thus neither reproduced nor generalized. In the present work, we use Monte Carlo sampling in combination with thermodynamic integration in order to retrace Wilson's computation for a real-space renormalization with a number of terms in the hamiltonian. We elaborate on the connection of real-space renormalization with the fermion sign problem and discuss to which extent our Monte Carlo procedure actually implements Wilson's program from half a century ago.
