2020
DOI: 10.1103/physrevresearch.2.013212
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Loading and cooling in an optical trap via hyperfine dark states

Abstract: We present a novel optical cooling scheme that relies on hyperfine dark states to enhance loading and cooling atoms inside deep optical dipole traps. We demonstrate a seven-fold increase in the number of atoms loaded in the conservative potential with strongly shifted excited states. In addition, we use the energy selective dark-state to efficiently cool the atoms trapped inside the conservative potential rapidly and without losses. Our findings open the door to optically assisted cooling of trapped atoms and … Show more

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Cited by 10 publications
(6 citation statements)
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References 30 publications
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“…An even larger d opt would be required for experiments on many-body physics with light [31,61], which seems to be feasible. Secondly, as the loading efficiency is in part limited by density-dependent losses, in-fiber cooling [62] will have to be applied with care. On the one hand, cooling will lead to a reduction of inhomogenous broadening and compensation of heating.…”
Section: Discussionmentioning
confidence: 99%
“…An even larger d opt would be required for experiments on many-body physics with light [31,61], which seems to be feasible. Secondly, as the loading efficiency is in part limited by density-dependent losses, in-fiber cooling [62] will have to be applied with care. On the one hand, cooling will lead to a reduction of inhomogenous broadening and compensation of heating.…”
Section: Discussionmentioning
confidence: 99%
“…The ICE (Interférométrie Cohérente pour l'Espace) project, funded by CNES is aiming to a WEP test with a dual species Rb/K atom interferometer on board of parabolic flights of 20 s each. The experiment uses frequency-doubled telecom lasers to manipulate the atoms [17], and hyperfine dark state cooling and loading of Rb, and possibly K, to improve the phase space density of the atomic source [143]. Recently the payload was put on a 3-m microgravity simulator and produced an alloptical degenerate source of Rb at 35 nK temperature allowing to explore the relevant weightlessness times of 400 ms [142].…”
Section: Heritage and Development Activitiesmentioning
confidence: 99%
“…Raman sideband cooling [67][68][69] might be a better alternative for thermal ensembles even if it is limited to about an order of magnitude larger temperatures than what the BEC ensembles could reach. Other recent techniques avoiding evaporation [70][71][72] might also be promising for a future use in the field.…”
Section: Expansion Rate and Collimationmentioning
confidence: 99%