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arXiv:1707.00059 · Physics Letters A

Simulating sympathetic cooling of atomic mixtures in nonlinear traps

Francisco Jauffred, Roberto Onofrio, Bala Sundaram

Published Jul 3, 2017• 8 citations
arXivHTMLPDF
DOI
10.1016/j.physleta.2017.06.046

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Applying the direct simulation Monte Carlo (DSMC) method developed for the cold atom system, we explore the possibility of a high-efficiency sympathetic cooling process between 87 Rb and 40 K without gravitational force in an optical trap. The relation between the pre-cooling of Bosons and the sympathetic cooling efficiency is also studied. We find that the absence of gravitational force is beneficial to the process of sympathetic cooling. Furthermore, an inefficient pre-cooling process will in fact hamper the creation of Fermi degenerate gases. This suggests the advantages of sympathetic cooling in microgravity.
We report on the realization of a stable mixture of ultracold lithium and ytterbium atoms confined in a far-off-resonance optical dipole trap. We observe sympathetic cooling of 6Li^{6}\mathrm{Li}6Li by 174Yb^{174}\mathrm{Yb}174Yb and extract the sss-wave scattering length magnitude $|{a}_{^{6}\mathrm{Li}\mathrm{\text{\ensuremath{-}}}^{174}\mathrm{Yb}}|=(13\ifmmode\pm\else\textpm\fi{}3){a}_{0}$ from the rate of interspecies thermalization. Using forced evaporative cooling of 174Yb^{174}\mathrm{Yb}174Yb, we achieve reduction of the 6Li^{6}\mathrm{Li}6Li temperature to below the Fermi temperature, purely through interspecies sympathetic cooling.
We discuss fast frictionless cooling techniques in the framework of sympathetic cooling of cold atomic mixtures. It is argued that optimal cooling of an atomic species---in which the deepest quantum degeneracy regime is achieved---may be obtained by means of sympathetic cooling with another species whose trapping frequency is dynamically changed to maintain constancy of the Lewis-Riesenfeld adiabatic invariant. Advantages and limitations of this cooling strategy are discussed, with particular regard to the possibility of cooling Fermi gases to a deeper degenerate regime.