
Quantized vortices that form in superfluid helium, exhibiting unique rotational properties.Superfluid vortices are quantized whirlpools that form in superfluids — fluids that flow without viscosity, such as helium-4 below 2.17 K. Unlike ordinary vortices, their circulation is quantized in discrete units of Planck's constant divided by the mass of the constituent particles. These vortices are topological defects that carry angular momentum and play a crucial role in the dynamics of superfluids, including their response to rotation and the transition to turbulence.
The concept of quantized vortices in superfluids was predicted by Lars Onsager in 1949 and independently by Richard Feynman in 1955. Experimental confirmation came in the 1960s with observations of vortex arrays in rotating superfluid helium.
When a superfluid is rotated, it cannot rotate as a solid body because the superfluid component has zero viscosity and cannot sustain velocity gradients. Instead, it forms an array of quantized vortices, each with a core where the superfluid density drops to zero. The circulation around each vortex is an integer multiple of h/m, where h is Planck's constant and m is the particle mass. These vortices interact with each other and with boundaries, leading to complex behaviors like vortex reconnection and quantum turbulence.
Superfluid vortices are studied in fundamental physics to understand quantum turbulence and topological defects, and they have inspired analogous systems in ultracold atomic gases and superconducting circuits, where vortices can be used to simulate hydrodynamic phenomena or store information.
In superfluid helium, the cores of quantized vortices are only about one angstrom in diameter — roughly the size of a single atom — yet they can be thousands of times longer.















