Universal three-body physics at finite energies
POSTER
Abstract
We discuss the universal three-body scattering physics for cold atoms up to energies far beyond the ultracold limit. We have found universal features in the energy-dependence of the three-body recombination rates which can be traced to Efimov physics. These new features, however, have different character for positive and negative scattering length ($a$) because the high partial wave contributions are very different. In particular, we show that for $a>0$, the very high partial wave contributions are still important in a certain energy range. For $a<0$, however, the $S$-wave contribution is dominant up to the highest energy where the three-body recombination is universal. We also discuss modifications of the universal three-body physics that arise near a narrow Feshbach resonance. Our results provide a complete picture for the universal features in the three-body recombination, and will assist the experimental study of the universal three-body physics under very different experimental conditions.
*Supported by the National Science Foundation.