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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ferred <strong>in</strong><strong>to</strong> the |F = 1,mF = 0〉 or |F = 1,mF = 1〉 state via the s<strong>in</strong>gle-pho<strong>to</strong>n cool<strong>in</strong>g<br />
process. For a<strong>to</strong>ms <strong>in</strong> the |F = 1,mF = 0〉 state this is a purely gravi<strong>to</strong>-optical poten-<br />
tial, while for a<strong>to</strong>ms <strong>in</strong> the |F = 1,mF = 1〉 the magnetic <strong>in</strong>teraction adds <strong>to</strong> the overall<br />
potential. Both states are trappable by the optical trough. In this new state, |F = 1〉,<br />
the a<strong>to</strong>ms cannot rega<strong>in</strong> the potential energy with<strong>in</strong> the optical trough <strong>and</strong> are therefore<br />
effectively cooled.<br />
The 87 Rb ground state hyperf<strong>in</strong>e splitt<strong>in</strong>g is 6.8 GHz, mean<strong>in</strong>g that once the<br />
a<strong>to</strong>ms are transferred <strong>to</strong> the |F = 1〉 state, the demon beam is detuned by 6.8 GHz.<br />
Scatter<strong>in</strong>g of the demon beam of a<strong>to</strong>ms <strong>in</strong> the |F = 1〉 state is therefore negligible,<br />
ensur<strong>in</strong>g the irreversibility of the process.<br />
By adiabatically reduc<strong>in</strong>g the current <strong>in</strong> the quadrupole coils, the magnetic po-<br />
tential is collapsed. Dur<strong>in</strong>g this ramp-off time tramp (typically on the order of 1 second)<br />
the a<strong>to</strong>ms encounter<strong>in</strong>g the demon beam are always near their classical turn<strong>in</strong>g po<strong>in</strong>ts,<br />
ensur<strong>in</strong>g the cool<strong>in</strong>g process. In order for the transfer <strong>to</strong> happen near the classical turn-<br />
<strong>in</strong>g po<strong>in</strong>ts, 〈τ〉 ≪ tramp must be satisfied, where 〈τ〉 is the average oscillation period <strong>in</strong><br />
the magnetic trap. In the rubidium magnetic trap 〈τ〉 is about 20 ms.<br />
Once the quadrupole coil current is reduced below 2.5 A (correspond<strong>in</strong>g <strong>to</strong> a<br />
magnetic field gradient of 12 G/cm) the s<strong>in</strong>gle-pho<strong>to</strong>n cool<strong>in</strong>g process is complete. At<br />
this po<strong>in</strong>t a<strong>to</strong>ms <strong>in</strong> the magnetic trap are no longer levitated aga<strong>in</strong>st gravity <strong>and</strong> are lost<br />
from the trap. The a<strong>to</strong>ms <strong>in</strong> the optical trough are then imaged <strong>to</strong> obta<strong>in</strong> <strong>in</strong>formation<br />
about the a<strong>to</strong>m number, spatial distribution <strong>and</strong> temperature.<br />
Figure 5.3 shows the <strong>in</strong>cremental transfer of a<strong>to</strong>ms <strong>in</strong><strong>to</strong> the optical trough as a<br />
function of the quadrupole coil current. The current is ramped l<strong>in</strong>early <strong>in</strong> time. The<br />
optical trough itself is a conservative trap, therefore any positive slope is <strong>in</strong>dicative of<br />
successful s<strong>in</strong>gle-pho<strong>to</strong>n cool<strong>in</strong>g.<br />
In the absence of any trap losses the <strong>in</strong>crease <strong>in</strong> phase space density <strong>in</strong> the optical<br />
trough <strong>in</strong>creases with a larger ramp time. However, unwanted scatter<strong>in</strong>g events <strong>and</strong><br />
collisions with background gas lead <strong>to</strong> a f<strong>in</strong>ite trap life time. Balanc<strong>in</strong>g these effects<br />
dictates the optimum ramp time.<br />
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