Observable Resonances in Efimov-unfavored Systems
Karim I. Elghazawy, Chris H. Greene
TL;DR
The paper addresses how the intraspecies scattering length $a_ ext{BB}$ shifts Efimov resonances and the three-body parameter $a_-^{(0)}$ in Efimov-unfavored LLH systems. It introduces a finite-range, separable-potential three-body framework and compares with zero-range hyperspherical results to study ^{23}Na$_2$^{40}$K, revealing two distinct mechanisms dictated by the sign of $a_ ext{BB}$ and the large disparity between scaling parameters $s_0$ and $s_0^*$. For $a_ ext{BB}<0$, a transition region between two Efimov scalings causes strong $|a_ ext{BB}|$-dependence of the spectrum and $a_-^{(n)}$, while for $a_ ext{BB}>0$ the spectrum splits into two well-separated ladders, pushing the first resonance $a_-^{(0)}$ to very large values. Theoretical results show good agreement with experimental Na$_2$K trimer binding energies, validating the mechanisms and highlighting that observable 3BP values arise in LLH systems when $a_ ext{BB}<0$.
Abstract
Three-body loss resonances associated with heavy-heavy-light Efimov states have been observed for over a decade in ultracold mixtures tuned near interspecies Feshbach resonances. For light-light-heavy systems, observing such resonances has been far more challenging due to the substantially large Efimov spacing. In these Efimov-unfavored systems, the intraspecies scattering length $a_\text{BB}$ has been shown to significantly affect the overall Efimov scenario, namely, the positions of the Efimov resonances $a_{-}^{(n)}$ and the three-body parameter (3BP) $a_{-}^{(0)}$. The present article explains the origin behind this influence by highlighting two primary mechanisms via which both the magnitude and sign of $a_\text{BB}$ govern the Efimov spectrum and set the resulting 3BP $a_{-}^{(0)}$. By employing van der Waals interactions for $^{23}$Na$_2{}^{40}$K, we attribute the vital role of $a_\text{BB}$ in Efimov-unfavored systems to the large difference between the Efimov scaling parameters for two and three resonant interactions, $s_0$ and $s_0^*$. In particular, we account for the unusually large $a_{-}^{(0)}$ obtained in light-light-heavy systems with $a_\text{BB}>0$ (e.g., $^{41}$K$_2{}^{87}$Rb), and show that the first Efimov resonance can still occur at an experimentally accessible value when $a_\text{BB}<0$.
