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    Altermagnetic band geometry and the antiferromagnetic thermal boundary in a coupled fermion-Ising model

    Xing-Can Liu1, Ho-Kin Tang2,3,*, Tao Ying1,†, and Xueru Zhang1,‡

    • *Contact author: denghaojian@hit.edu.cn
    • †Contact author: taoying86@hit.edu.cn
    • ‡Contact author: xrzhang@hit.edu.cn

    Phys. Rev. B 114, 235135 – Published 29 October, 2026

    DOI: https://doi.org/10.1103/f873-q422

    Abstract

    We study a minimal square-lattice model to examine the relation between momentum-space altermagnetic band geometry and real-space Ising criticality in a coupled fermion-Ising setting. In this model, itinerant fermions with explicitly spin-dependent nearest-neighbor hopping are locally coupled to transverse-field Ising moments. The hopping anisotropy parameter α tunes a dx2−y2-type altermagnetic band geometry in momentum space, whereas the transverse field h controls real-space antiferromagnetic (AFM) fluctuations and drives the finite-temperature AFM–paramagnetic (PM) transition of the Ising sector. Using determinant quantum Monte Carlo simulations, we show for the representative α<1 case studied in detail, α=0.5, that the momentum-space band-geometry fingerprint remains visible in the coupled system: the spin-resolved occupation imbalance n↑(k)−n↓(k) displays a sign-changing structure that follows the underlying spin-split Fermi-surface geometry. By contrast, finite-size scaling of the staggered Ising order parameter indicates that, in the representative comparison between α=0.5 and 1.0, the extracted thermal critical fields remain numerically close on the scale resolved by our finite-size analysis at both T/t=0.5 and 0.2. We argue that this separation reflects the coexistence of a tunable momentum-space altermagnetic band geometry with the nesting structure of the half-filled nearest-neighbor bare kinetic term, which remains an important constraint on the AFM channel in this benchmark. Our results show that, in this controlled setting, a visible altermagnetic band-geometry fingerprint in momentum space need not imply a comparably large shift of the collective real-space magnetic phase boundary.

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