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This study demonstrates that magnetic monopole physics can be simulated using quantum vortices in a spherical superfluid shell, offering an accessible platform to explore fundamental gauge field dynamics without requiring high-energy particle colliders. The research confirms theoretical predictions regarding charge quantization and vortex motion through numerical simulations, bridging condensed matter systems with topological concepts central to both AI-driven material discovery and foundational quantum theory.
A magnetic monopole in a superfluid bubble
arXiv:2607.15093v2 Announce Type: replace-cross Abstract: Magnetic monopoles lie at the crossroads of gauge fields, topology, geometric phases, and charge quantization, yet they remain elusive as fundamental particles. Here we show that an emergent Dirac-monopole framework arises naturally from the dynamics of massive quantum vortices in a spherical superfluid shell. Their dynamics is formally equivalent to that of interacting charged particles constrained to a sphere in the field of a magnetic monopole. The monopole charge is fixed by the superfluid density and automatically satisfies Dirac's quantization condition. The emergent monopole description predicts cyclotron-like vortex motion, in quantitative agreement with Gross--Pitaevskii simulations. We further show that topological frustration induced by two like-charged polar vortices gives rise to the formation of an equatorial vortex necklace, a configuration reminiscent of the polygonal cyclone clusters observed around Jupiter's poles, before its subsequent breakup through a Kelvin--Helmholtz-like instability. Within this framework, the equatorial vortex necklace emerges as the quantized realization of the effective electrostatic line charge that restores global charge neutrality on the sphere. Our results establish spherical superfluids as a versatile platform for realizing and exploring fundamental aspects of Dirac-monopole physics.
Abstract:Magnetic monopoles lie at the crossroads of gauge fields, topology, geometric phases, and charge quantization, yet they remain elusive as fundamental particles. Here we show that an emergent Dirac-monopole framework arises naturally from the dynamics of massive quantum vortices in a spherical superfluid shell. Their dynamics is formally equivalent to that of interacting charged particles constrained to a sphere in the field of a magnetic monopole. The monopole charge is fixed by the superfluid density and automatically satisfies Dirac's quantization condition. The emergent monopole description predicts cyclotron-like vortex motion, in quantitative agreement with Gross--Pitaevskii simulations. We further show that topological frustration induced by two like-charged polar vortices gives rise to the formation of an equatorial vortex necklace, a configuration reminiscent of the polygonal cyclone clusters observed around Jupiter's poles, before its subsequent breakup through a Kelvin--Helmholtz-like instability. Within this framework, the equatorial vortex necklace emerges as the quantized realization of the effective electrostatic line charge that restores global charge neutrality on the sphere. Our results establish spherical superfluids as a versatile platform for realizing and exploring fundamental aspects of Dirac-monopole physics.
9 pages (including 3 figures) + 11 pages (including 4 figures) of Sup. Mat
Quantum Gases (cond-mat.quant-gas); Quantum Physics (quant-ph)
arXiv:2607.15093 [cond-mat.quant-gas]
(or arXiv:2607.15093v2 [cond-mat.quant-gas] for this version)
https://doi.org/10.48550/arXiv.2607.15093 Focus to learn more arXiv-issued DOI via DataCite
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Full text under the publisher's open licence · 290 words
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