Vortex formation in neutron-irradiated rotating superfluid 3He-B

Abstract

A convenient method to create vortices in meta-stable vortex-free superflow of 3He-B is to irradiate with thermal neutrons. The vortices are then formed in a rapid non-equilibrium process with very distinctive characteristics. Two models were suggested to explain the phenomenon. One is based on the Kibble-Zurek mechanism of defect formation in a quench-cooled second order phase transition. The second model builds on the instability of the moving front between superfluid and normal 3He, which is created by the heating from the neutron absorption event. The most detailed measurements with single-vortex resolution have been performed at temperatures close to Tc. We present an overview of the main experimental features and demonstrate that the measurements are consistent with the Kibble-Zurek picture. New data, collected at low temperatures, support this conclusion, but display superfluid turbulence as a new phenomenon. Below 0.6 Tc the damping of vortex motion from the normal component is reduced sufficiently so that turbulent vortex dynamics become possible. Here a single absorbed neutron may transfer the sample from the meta-stable vortex-free to the equilibrium vortex state. We find that the probability for a neutron to initiate such a turbulent transition grows with increasing superflow velocity and decreasing temperature.