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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A<strong>to</strong>ms are then optically pumped <strong>to</strong> the |F = 2,mF = 2〉 state. A weak uniform<br />
magnetic field (B ≈ 1 G) is turned on dur<strong>in</strong>g the optical pump<strong>in</strong>g time (≈ 100 µs)<br />
<strong>to</strong> def<strong>in</strong>e a quantization axis. Approximately 73% of the a<strong>to</strong>ms are transferred <strong>to</strong> the<br />
|F = 2,mF = 2〉 state, while the other a<strong>to</strong>ms rema<strong>in</strong> <strong>in</strong> the |F = 2,mF = 1〉 state.<br />
All beams are then turned off <strong>and</strong> shuttered, <strong>and</strong> the magnetic field gradients<br />
are <strong>in</strong>creased <strong>to</strong> 48 G/cm with<strong>in</strong> a few ms, conf<strong>in</strong><strong>in</strong>g the a<strong>to</strong>ms <strong>in</strong> the magnetic trap.<br />
To decrease the thermal equilibration time, the magnetic field gradients are <strong>in</strong>creased<br />
<strong>to</strong> 96 G/cm <strong>in</strong> about 200 ms, <strong>in</strong>creas<strong>in</strong>g the collision rate. After about 5 seconds the<br />
a<strong>to</strong>ms reach thermal equilibrium <strong>and</strong> the gradients are reduced <strong>to</strong> 72 G/cm. At this<br />
po<strong>in</strong>t about 10 7 Rb a<strong>to</strong>ms at a temperature of 50 µK are conf<strong>in</strong>ed <strong>in</strong> the magnetic trap.<br />
<strong>Control</strong>l<strong>in</strong>g the temperature of the a<strong>to</strong>ms <strong>in</strong> the magnetic trap is important for the<br />
study of s<strong>in</strong>gle-pho<strong>to</strong>n cool<strong>in</strong>g. By vary<strong>in</strong>g the detun<strong>in</strong>g <strong>in</strong> the MOT beams dur<strong>in</strong>g the<br />
load<strong>in</strong>g <strong>and</strong> optical molasses phases, the temperature can be varied between about 30<br />
<strong>and</strong> 55 µK.<br />
Us<strong>in</strong>g st<strong>and</strong>ard laser cool<strong>in</strong>g techniques is, however, not required <strong>to</strong> load a<strong>to</strong>ms<br />
<strong>in</strong><strong>to</strong> a magnetic trap. It has been shown that it is feasible <strong>to</strong> decelerate a supersonic<br />
beam of a<strong>to</strong>ms us<strong>in</strong>g an a<strong>to</strong>mic coilgun [77–79]. At low velocities these a<strong>to</strong>ms can then<br />
be directly loaded <strong>in</strong><strong>to</strong> a magnetic trap.<br />
h<br />
demon beam<br />
Figure 5.1: Alignment of the demon beam <strong>in</strong>side the optical trough.<br />
Once the rubidium a<strong>to</strong>ms are transferred <strong>in</strong><strong>to</strong> the magnetic trap, the optical<br />
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