Rigorous Anderson-type lower bounds on the ground-state energy of the pyrochlore Heisenberg antiferromagnet
Péter Kránitz, Karlo Penc
TL;DR
This work develops a systematic, motif-based extension of Anderson’s rigorous lower bounds to the frustrated pyrochlore Heisenberg antiferromagnet for spin-$S$ spins. By organizing local sub-Hamiltonians into a hierarchy of clusters—the star, tetrahedron, seven-site hourglass, and the 18-site crown—the authors derive increasingly tight lower bounds, with a closed-form bound for arbitrary $S$ in the hourglass motif and exact results for $S=\tfrac{1}{2}$ and $S=1$ on the crown cluster. The approach generalizes to extended models including $J_1$-$J_2$-$J_{3b}$ exchanges, ring exchange, and scalar spin chirality, often producing piecewise-analytic bounds governed by level crossings; notably, the Klein point saturates the hourglass bound in the quadrilinear case. The results provide tight, rigorous benchmarks that complement numerical estimates and variational bounds, and they point to a scalable path toward even larger motifs and broader lattice geometries in frustrated quantum magnets.
Abstract
We construct rigorous Anderson-type lower bounds on the ground-state energy of the spin-$S$ Heisenberg antiferromagnet on the pyrochlore lattice. By formulating and optimizing a hierarchy of local cluster motifs ordered by size, we generate a sequence of increasingly tight bounds. A seven-site "hourglass" cluster composed of two corner-sharing tetrahedra furnishes an optimal lower bound that admits a closed-form expression for arbitrary spin $S$. We also derive exact lower bounds for generalized models with further-neighbor exchange, ring exchange, and scalar spin-chirality interactions. For $S=1/2$ and $S=1$, numerical optimization of an 18-site "crown" cluster containing a hexagonal loop yields rigorous lower bounds on the ground-state energy per site of the nearest-neighbor Heisenberg model with unit exchange, $e_\mathrm{GS} \geq -0.549832$ and $e_\mathrm{GS} \geq -1.632985$, respectively. We compare the resulting bounds with numerical ground-state energy estimates from the literature.
