Predicted signatures of rotating Bose–Einstein condensates

Superfluids are distinguished from normal fluids by their peculiar response1 to rotation: circulating flow in superfluid helium2,3, a strongly coupled Bose liquid, can appear only as quantized vortices4,5,6. The newly created Bose–Einstein condensates7,9—clouds of millions of ultracold, weakly interacting alkali-metal atoms that occupy a single quantum state—offer the possibility of investigating superfluidity in the weak-coupling regime. An outstanding question is whether Bose–Einstein condensates exhibit a mesoscopic quantum analogue of the macroscopic vortices in superfluids, and what its experimental signature would be. Here we report calculations of the low-energy states of a rotating, weakly interacting Bose gas. We find a succession of transitions between stable vortex patterns of differing symmetries that are in general qualitative agreement with observations5 of rotating superfluid helium, a strong-coupling superfluid. Counterintuitively, the angular momentum per particle is not quantized. Some angular momenta are forbidden, corresponding to asymmetrical unstable states that provide a physical mechanism for the entry of vorticity into the condensate.