Quasi-classical expansion of a hyperbolic solution to the star-star relation and multicomponent 5-point difference equations
Andrew P. Kels
TL;DR
This paper studies the quasi-classical expansion of a multicomponent ($n$-component) hyperbolic star-star solution in edge-interaction lattice models, using hyperbolic Boltzmann weights built from the hyperbolic gamma function. The authors scale variables with $\hbar$ and derive leading-order Lagrangian densities, yielding $n-1$ component 5-point difference equations that generalize known scalar equations on face-centered cubic lattices. In the hyperbolic and rational limits, these equations provide multicomponent extensions of scalar 5-point equations (e.g., $A3_{(1)}$ for $n=2$ and $A2_{(1;1)}$ in the rational $n=2$ case), with integrability conjectured to follow from consistency-around-a-face-centered-cube (CAFCC) and IRF Yang-Baxter structures. The work highlights a deep connection between integrable lattice models and discrete integrable systems, offering a pathway to analyze Lax pairs and CAFCC for $n>2$ and to explore multicomponent reductions and related hex systems. Overall, the paper extends the bridge between star-star integrable models and multicomponent discrete equations, enriching the landscape of discrete integrability.
Abstract
The quasi-classical expansion of a multicomponent spin solution of the star-star relation with hyperbolic Boltzmann weights is investigated. The equations obtained in a quasi-classical limit provide n-1-component extensions of certain scalar 5-point equations (corresponding to n=2) that were previously investigated by the author in the context of integrability and consistency of equations on face-centered cubics.
