2007
DOI: 10.1103/physreva.76.053418
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Sub-Doppler laser cooling and magnetic trapping of erbium

Abstract: We investigate cooling mechanisms in magneto-optically and magnetically trapped erbium. We find efficient sub-Doppler cooling in our trap, which can persist even in large magnetic fields due to the near degeneracy of two Lande g factors. Furthermore, a continuously loaded magnetic trap is demonstrated where we observe temperatures below 25 microkelvin. These favorable cooling and trapping properties suggest a number of scientific possibilities for rare-earth atomic physics, including narrow linewidth laser coo… Show more

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Cited by 42 publications
(44 citation statements)
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“…Temperature heating data-e.g., Fig. 3(b)-are fit to an exponential, resulting at early times to a heating rate of 17(2) µK/s, which is consistent with the heating rate in spin unpolarized Er and Cr MTs [23,24] and is likely due to spin-relaxation collisions. The MT population is initially distributed among the weak-field seeking Zeeman states, and spin exchange collisions tend to polarize the sample toward m J = 8.…”
supporting
confidence: 66%
See 1 more Smart Citation
“…Temperature heating data-e.g., Fig. 3(b)-are fit to an exponential, resulting at early times to a heating rate of 17(2) µK/s, which is consistent with the heating rate in spin unpolarized Er and Cr MTs [23,24] and is likely due to spin-relaxation collisions. The MT population is initially distributed among the weak-field seeking Zeeman states, and spin exchange collisions tend to polarize the sample toward m J = 8.…”
supporting
confidence: 66%
“…In ballistic expansion after extinguishing the MOT, a dual component gas is observed comprised of a dense symmetric core of ∼200 µK atoms surrounded by a hot, 2-3 mK shell containing 70% of the atoms. Doppler cooling theory in 1D predicts a cloud temperature of 1.2 mK for the MOT parameters, but comparisons to the Er MOT [23] suggest the entire intra-MOT population should be subDoppler cooled to ∼100 µK as a consequence of the near equal Landé g-factors in the ground and excited states (∆g/g = 1.7%). Despite ∆g being slightly larger than in Er, numerical 1D sub-Doppler cooling simulations (based on Ref.…”
mentioning
confidence: 97%
“…Transition f) may have a larger linewidth, but this will have to be studied experimentally. If not there is the possibility of cooling on the very strong transition labeled g) to the level 4f 11 ( 4 I o 15/2 )6s6p( 1 P o 1 ), J = 17/2 at 410.5 nm which appears analogous to the strong blue line used for cooling of Er to subDoppler temperatures [36]. This transition has a linewidth of γ = 204 × 10 6 s −1 and a Doppler cooling limit of 780 µK.…”
Section: B Cooling and Trappingmentioning
confidence: 99%
“…Efficient sub-Doppler cooling directly in the MOT is possible if the Landé g-factors of the upper and the lower cooling levels are nearly equal [21]. In our case the relative difference of the Landé g-factors of the cooling levels in Tm is only 2% which enables efficient sub-Doppler cooling.…”
Section: Sub-doppler Coolingmentioning
confidence: 75%