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Vortex patterns of a two-dimensional Bose-Einstein condensate at the almost critical rotation speed

This paper numerically investigates vortex patterns in a two-dimensional Bose-Einstein condensate near critical rotation, demonstrating that repulsive interactions yield Abrikosov vortex lattices consistent with Thomas-Fermi theory, while attractive interactions preclude vortex lattices in favor of collapsing giant vortex solitons whose stability thresholds are determined by equivariant Gagliardo-Nirenberg inequalities.

Original authors: Bao-Duy Le, Dinh-Thi Nguyen

Published 2026-08-18
📖 5 min read🧠 Deep dive

Original authors: Bao-Duy Le, Dinh-Thi Nguyen

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

Imagine a cloud of atoms so cold that they stop behaving like individual particles and start acting as a single, giant wave. This state of matter, known as a Bose-Einstein condensate, is one of the most exotic creations in modern physics. When scientists spin this cloud, it does not just swirl like water in a bucket; it reacts in a way that reveals the deep quantum rules governing the universe. If the atoms push away from each other, the spinning cloud organizes itself into a perfect grid of tiny holes, much like the pattern of holes in a sponge. But if the atoms pull toward each other, the cloud behaves in a completely opposite manner, shrinking inward and collapsing into a single, dense point. Understanding how these two different behaviors play out when the cloud is spun at nearly its maximum possible speed is the central question explored in a recent study.

Researchers set out to map the patterns that form inside these spinning clouds, focusing on the moment just before the rotation becomes so fast that the trap holding the atoms together begins to fail. They treated the two types of atomic interactions separately, using different computational tools for each. For the repulsive case, where atoms push apart, they used a method that projects the system onto a specific quantum state known as the Lowest Landau Level. This approach allowed them to simulate the formation of a triangular lattice of vortices. These vortices are tiny whirlpools of quantum fluid, and the team found that as the rotation speed increased, the cloud settled into a highly ordered structure. The density of these whirlpools matched the predictions of a theory developed decades ago for superconductors, confirming that the rotating cloud behaves like a superconductor made of atoms. The researchers calculated a specific numerical value that describes the efficiency of this vortex packing, finding it to be approximately 1.16, a number that has long been expected in this field but is difficult to pin down with such precision in a simulation.

In stark contrast, the researchers turned their attention to the attractive case, where the atoms pull toward one another. Here, the results were surprising and definitive. No matter how fast they spun the cloud, or how strong the attraction became, the atoms never formed a grid of vortices. Instead, the cloud simply contracted, pulling all its mass toward the center. The simulations showed that as the attraction grew stronger, the cloud would eventually collapse into a singularity, a process that happens regardless of the rotation speed. The only stable spinning states they found were "giant vortices," which are essentially a single, massive hole in the center of the cloud rather than a grid of many small ones. These giant vortices are fragile; they exist only up to a specific limit of attraction. Once the pull between atoms exceeds a precise threshold, the giant vortex collapses just like the non-spinning cloud does. The team identified these critical thresholds for different types of giant vortices, noting that a vortex with no spin requires an attraction strength of about 11.7 to collapse, while a vortex with a single unit of spin requires a much higher strength of roughly 48.3, and so on.

The study also addressed a common misconception about what happens when you try to force a vortex pattern into an attractive cloud. In earlier work, some researchers had managed to create these patterns by artificially imprinting them onto the cloud, but this new research showed that such patterns are not stable. When the artificial imprint was removed and the system was allowed to relax, the vortices were immediately expelled, and the cloud returned to its smooth, nodeless shape. This confirmed that the attractive force is so dominant that it actively fights against the formation of any rotational structure, preferring instead to concentrate all its energy into a single, shrinking lump. The researchers ran these simulations with extreme care, testing their methods against different mathematical approaches to ensure the results were not just artifacts of the computer code. They found that their methods for the repulsive case were highly accurate, reproducing known theoretical values, while their methods for the attractive case correctly predicted the collapse behavior and the specific limits at which it occurs.

Ultimately, this work provides a clear, numerical benchmark for how quantum gases behave under extreme conditions. It confirms that the universe offers two distinct paths for these spinning clouds: one leads to a beautiful, crystalline order of many small whirlpools, and the other leads to a dramatic, singular collapse. The findings suggest that the rotation speed, while dramatic, does not change the fundamental nature of these two outcomes. Whether the atoms are pushing apart or pulling together, the rotation acts as a background condition rather than a switch that changes the rules. The repulsive cloud finds stability in a lattice, while the attractive cloud finds its only stability in a single, collapsing point, with the rotation speed playing a minor role in the final fate of the system.

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