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Quantum group deformation of the Kittel--Shore model

A. Ballesteros, I. Gutiérrez-Sagredo, V. Mariscal, J. J. Relancio

TL;DR

The paper addresses constructing and solving a $U_q(\mathfrak{su}(2))$-invariant deformation of the Kittel–Shore model to preserve integrability for arbitrary spins. It develops the q-KS Hamiltonian by enforcing quantum group coalgebra symmetry, derives exact spectra and eigenvectors via $q$-Clebsch–Gordan coefficients, and analyzes spin-\tfrac{1}{2}$ cases at $N=2$ and $N=3$ with higher-spin extensions sketched. A thorough numerical study of the Curie temperature reveals an exponential rise with deformation parameter $\eta$, and the work outlines how to extend these results to arbitrary spin and potential connections to thermodynamics and quantum information. The results establish a new, exactly solvable long-range spin model with nonlocal, $q$-dependent couplings, enriching the landscape of integrable quantum spin systems and offering a framework for exploring deformation effects in finite-size and thermodynamic regimes.

Abstract

The Kittel--Shore (KS) Hamiltonian describes $N$ spins with long-range interactions that are identically coupled; therefore, this (mean-field) model is also known as the Heisenberg XXX model on the complete graph. In this paper, the underlying $U(\mathfrak{su}(2))$ coalgebra symmetry of the KS model is demonstrated for arbitrary spins, and the quantum deformation of the KS Hamiltonian ($q$-KS model) is obtained using the corresponding $U_q(\mathfrak{su}(2))$ quantum group. By construction, the existence of such a symmetry guarantees that all integrability properties of the KS model are preserved under $q$-deformation. In particular, the $q$-KS model for spin-$1/2$ particles is analysed, the cases with $N=2$ and $3$ spins are studied in detail, and higher-spin $q$-KS models are sketched. As a first excursion into the thermodynamic properties of the spin-$1/2$ $q$-KS model, the dependence of the Curie temperature on the deformation parameter is studied through numerical analysis.

Quantum group deformation of the Kittel--Shore model

TL;DR

The paper addresses constructing and solving a -invariant deformation of the Kittel–Shore model to preserve integrability for arbitrary spins. It develops the q-KS Hamiltonian by enforcing quantum group coalgebra symmetry, derives exact spectra and eigenvectors via -Clebsch–Gordan coefficients, and analyzes spin-\tfrac{1}{2}N=2N=3\etaq$-dependent couplings, enriching the landscape of integrable quantum spin systems and offering a framework for exploring deformation effects in finite-size and thermodynamic regimes.

Abstract

The Kittel--Shore (KS) Hamiltonian describes spins with long-range interactions that are identically coupled; therefore, this (mean-field) model is also known as the Heisenberg XXX model on the complete graph. In this paper, the underlying coalgebra symmetry of the KS model is demonstrated for arbitrary spins, and the quantum deformation of the KS Hamiltonian (-KS model) is obtained using the corresponding quantum group. By construction, the existence of such a symmetry guarantees that all integrability properties of the KS model are preserved under -deformation. In particular, the -KS model for spin- particles is analysed, the cases with and spins are studied in detail, and higher-spin -KS models are sketched. As a first excursion into the thermodynamic properties of the spin- -KS model, the dependence of the Curie temperature on the deformation parameter is studied through numerical analysis.

Paper Structure

This paper contains 20 sections, 100 equations, 19 figures.

Figures (19)

  • Figure 1: Energy levels (in the units $|I|/4$) and their degeneracies for $N=2,3,4,5$ spins with $j=1/2$ coupled antiferromagnetically (a) without an external magnetic field $(h=0)$ and (b) with an external magnetic field $(h=0.5)$. Adapted from al1998exact. Note that $(1/2)^{\otimes 2} = 1 \oplus 0$, $(1/2)^{\otimes 3} = 3/2 \oplus (1/2)^{\oplus 2}$, $(1/2)^{\otimes 4} = 2 \oplus 1^{\oplus 3} \oplus 0^{2}$ and $(1/2)^{\otimes 5} = 5/2 \oplus (3/2)^{\oplus 4} \oplus (1/2)^{\oplus 4}$.
  • Figure 2: Density of energy levels (with zero energy ground state) for $N=20$ in the antiferromagnetic case.
  • Figure 3: Density of energy levels for $N=100$, $I\rightarrow\frac{I}{N}$ in the antiferromagnetic case.
  • Figure 4: Density of energy levels for $N=1000$, $I\rightarrow\frac{I}{N}$ in the antiferromagnetic case.
  • Figure 5: Density of energy levels for $N=20$ as a function of the parameter $\eta=0$ (red) and $\eta=0.2$ (dashed blue) in the antiferromagnetic case.
  • ...and 14 more figures