Ampère phase in frustrated magnets

We report a new class of algebraic spin liquids, in which the macroscopically degenerate ground state manifold is not Coulombic, like in spin ices, but Amp\`ere-like. The local constraint characterizing an Amp\`ere phase is not a Gauss law, but rather an Amp\`ere law, i.e., a condition on the curl of the magnetization vector field and not on its divergence. As a consequence, the excitations evolving in such a manifold are not magnetically charged scalar quasiparticles, the so-called magnetic monopoles in Coulomb phases, but instead vectorial magnetic loops (or fictional current lines). We demonstrate analytically that in a macroscopically degenerate manifold inheriting the properties of a cooperative paramagnet and subject to a local curl-free constraint, magnetic correlations decay in space with a power law whose exponent is the space dimension $d$: the Amp\`ere phase is a $d$-algebraic spin liquid. Using Monte Carlo simulations with appropriate cluster dynamics, we confirm this physics numerically in two- and three-dimensional examples and illustrate how the Amp\`ere phase compares to its Coulomb counterpart.

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Publication Details

Journal
Physical review. B./Physical review. B
Published
2025-02-03
DOI
https://doi.org/10.1103/physrevb.111.064402
Citations
1
Primary Topic
Advanced Condensed Matter Physics
Type
article
Field-Weighted Citation Impact
1.26
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article

Ampère phase in frustrated magnets

B. Canals, Johann Coraux, Nicolas Rougemaille
1 citations
Physical review. B./Physical review. B
Advanced Condensed Matter Physics
1.26
article

Ampère phase in frustrated magnets

B. Canals, Johann Coraux, Nicolas Rougemaille
article en
1 citations

Abstract

We report a new class of algebraic spin liquids, in which the macroscopically degenerate ground state manifold is not Coulombic, like in spin ices, but Amp\`ere-like. The local constraint characterizing an Amp\`ere phase is not a Gauss law, but rather an Amp\`ere law, i.e., a condition on the curl of the magnetization vector field and not on its divergence. As a consequence, the excitations evolving in such a manifold are not magnetically charged scalar quasiparticles, the so-called magnetic monopoles in Coulomb phases, but instead vectorial magnetic loops (or fictional current lines). We demonstrate analytically that in a macroscopically degenerate manifold inheriting the properties of a cooperative paramagnet and subject to a local curl-free constraint, magnetic correlations decay in space with a power law whose exponent is the space dimension $d$: the Amp\`ere phase is a $d$-algebraic spin liquid. Using Monte Carlo simulations with appropriate cluster dynamics, we confirm this physics numerically in two- and three-dimensional examples and illustrate how the Amp\`ere phase compares to its Coulomb counterpart.

Physical review. B./Physical review. BVol. 111(6)
Institut polytechnique de Grenoble (FR), Institut Néel (FR), Institut des langues et cultures d'Europe, Amérique, Afrique, Asie et Australie (FR), Université Grenoble Alpes (FR)
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Openalex Percentile: Top 25%
Advanced Condensed Matter Physics
1.26
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Ampère phase in frustrated magnets — B. Canals, Johann Coraux, et al. · Physical review. B./Physical review. B (2025) | TGRS Research Map | TGRS