Sub-Doppler cooling of ytterbium with the $^{1}S_{0}$-$^{1}P_{1}$ transition including $^{171}$Yb (I=1/2)

TL;DR

This paper demonstrates sub-Doppler laser cooling of ytterbium isotopes, including the fermionic $^{171}$Yb with I=1/2, achieving temperatures below the Doppler limit, and provides evidence for Sisyphus cooling mechanisms in a 3D magneto-optical trap.

Contribution

It reports the first sub-Doppler cooling of $^{171}$Yb in a magneto-optical trap using the $^{1}S_{0}$-$^{1}P_{1}$ transition, highlighting the role of Sisyphus cooling in such systems.

Findings

Temperatures below 400μK for $^{171}$Yb and 200μK for $^{173}$Yb.

Consistent temperature measurements via two independent methods.

Evidence supporting Sisyphus cooling mechanism in 3D MOTs.

Abstract

We report on the sub-Doppler laser cooling of neutral $^{171}$Yb and $^{173}$Yb in a magneto-optical trap using the $^{1}S_{0}$-$^{1}P_{1}$ transition at 398.9nm. We use two independent means to estimate the temperature of the atomic cloud for several of the Yb isotopes. The two methods of MOT-cloud-imaging and release-and-recapture show consistency with one another. Temperatures below 400$\mu$K and 200$\mu$K are recorded for $^{171}$Yb and $^{173}$Yb, respectively, while ~1mK is measured for both $^{172}$Yb and $^{174}$Yb. By comparison, the associated 1D Doppler cooling temperature limit is 694$\mu$K. The sub-Doppler cooling of the I=1/2 $^{171}$Yb isotope in a $\sigma^{+}-\sigma^{-}$ light-field trap adds further evidence that the Sisyphus cooling mechanism is occurring in such 3D magneto-optical traps.