Experiments to Control Atom Number and Phase-Space Density in ...
Experiments to Control Atom Number and Phase-Space Density in ...
Experiments to Control Atom Number and Phase-Space Density in ...
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phase-space density is def<strong>in</strong>ed as ρ ≡ nλ3 dB , λdB = √ √ 2π , where n is the spatial density<br />
mkBT<br />
of a<strong>to</strong>ms with mass m at temperature T. The phase-space density is limited by the<br />
temperature achievable <strong>in</strong> a MOT as well as by the spatial density of a<strong>to</strong>ms (typically<br />
on the order of ≈ 10 11 cm −3 ) [38]. Once the density exceeds a critical value a<strong>to</strong>ms<br />
start absorb<strong>in</strong>g fluorescent light emitted by other a<strong>to</strong>ms. This leads <strong>to</strong> a repulsive force<br />
between the a<strong>to</strong>ms limit<strong>in</strong>g the maximum density [35].<br />
2.10 Evaporative Cool<strong>in</strong>g<br />
The phase-space density <strong>in</strong> a magne<strong>to</strong>-optical trap is still about 6 orders of mag-<br />
nitude below degeneracy. The st<strong>and</strong>ard method of cool<strong>in</strong>g alkali a<strong>to</strong>ms further is evap-<br />
orative cool<strong>in</strong>g. This can happen <strong>in</strong> either a magnetic trap us<strong>in</strong>g an RF-knife, as is<br />
typically done for 87 Rb or 23 Na, or <strong>in</strong> an optical dipole trap, as is typically done for<br />
6 Li, where evaporative cool<strong>in</strong>g <strong>in</strong> a magnetic trap is not possible, see chapter 2.5.1. The<br />
basic pr<strong>in</strong>ciple of evaporative cool<strong>in</strong>g is illustrated <strong>in</strong> figure 2.19.<br />
Consider an a<strong>to</strong>mic cloud trapped <strong>in</strong> an optical dipole trap of trap depth U. If<br />
the thermal tail extends above the trap depth, the hottest a<strong>to</strong>ms with E > U will leave<br />
the trap, effectively lower<strong>in</strong>g the average energy of the rema<strong>in</strong><strong>in</strong>g a<strong>to</strong>ms. The rema<strong>in</strong><strong>in</strong>g<br />
a<strong>to</strong>ms then rethermalize through collisions, thus lower<strong>in</strong>g the average temperature of the<br />
trapped a<strong>to</strong>ms. Both of these processes happen simultaneously, until the thermal tail<br />
no longer extends above the trap depth <strong>and</strong> evaporation s<strong>to</strong>ps. The evaporative cool<strong>in</strong>g<br />
process can be forced <strong>to</strong> cont<strong>in</strong>ue by reduc<strong>in</strong>g the trap depth U.<br />
Evaporative cool<strong>in</strong>g can only be applied successfully if elastic collisions between<br />
a<strong>to</strong>ms dom<strong>in</strong>ate over <strong>in</strong>elastic collisions. This is true for both fermions <strong>and</strong> bosons.<br />
However, fermions cannot scatter with other fermions <strong>in</strong> the same state, due <strong>to</strong> the<br />
anti-symmetric nature of their wavefunction. Evaporative cool<strong>in</strong>g can therefore only be<br />
done us<strong>in</strong>g either a<strong>to</strong>ms <strong>in</strong> two different states [39], us<strong>in</strong>g two different a<strong>to</strong>ms, or by<br />
sympathetic cool<strong>in</strong>g [14]. The condition of a dom<strong>in</strong>at<strong>in</strong>g elastic cross section is satisfied<br />
for the two lowest states of 6 Li, |F = 1/2,mF = 1/2〉 <strong>and</strong> |F = 1/2,mF = −1/2〉, <strong>and</strong><br />
it is therefore possible <strong>to</strong> use these states for evaporative cool<strong>in</strong>g.<br />
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