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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<strong>in</strong>teraction. The shift <strong>in</strong> the energy states is then well approximated by<br />
∆E ≈ µBgJmJB (2.17)<br />
The energy level structure of lithium <strong>in</strong> the Zeeman regime is shown <strong>in</strong> figure<br />
2.10. Even though the highest three magnetic states (labeled |4〉, |5〉 <strong>and</strong> |6〉 <strong>in</strong> figure<br />
2.10) are low-field seek<strong>in</strong>g states, it is unfortunately not possible <strong>to</strong> evaporatively cool<br />
6 Li a<strong>to</strong>ms conf<strong>in</strong>ed <strong>in</strong> a magnetic trap. Scatter<strong>in</strong>g events dur<strong>in</strong>g evaporation causes<br />
sp<strong>in</strong>-flips <strong>to</strong> anti-trapped states lead<strong>in</strong>g trap loss [28].<br />
Energy Shift/ MHz<br />
300<br />
200<br />
100<br />
-100<br />
-200<br />
-300<br />
50 100 150<br />
| F , m F ; m S ,m I ,m L ><br />
|6>: |3/2, 3/2; 1/2, 1, 0><br />
|5>: |3/2, 1/2; 1/2, 1, 0><br />
|4>: |3/2, -1/2; 1/2,-1, 0><br />
B/ Gauss<br />
|3>: |3/2,-3/2;-1/2,-1, 0><br />
|2>: |1/2,-1/2;-1/2, 0, 0><br />
|1>: |1/2, 1/2;-1/2, 1, 0><br />
Figure 2.10: Energy shift of the 6 Li ground state <strong>in</strong> an external magnetic field. For small<br />
magnetic field strengths the energy level splitt<strong>in</strong>g follows the anomalous Zeeman-effect.<br />
Above about 30 Gauss angular momenta decouple <strong>and</strong> the energy splitt<strong>in</strong>g is described<br />
by the normal Zeeman effect.<br />
2.5.2 Magnetic Feshbach Resonance<br />
A Feshbach resonance is a quantum mechanical scatter<strong>in</strong>g resonance, which was<br />
first encountered <strong>in</strong> the context of nuclear physics [29]. In general, a Feshbach resonance<br />
can be <strong>in</strong>duced optically as well as magnetically, however, this discussion is limited <strong>to</strong><br />
the magnetic case. A simple model is used <strong>to</strong> describe the general phenomenon.<br />
Consider two potential curves Vbg <strong>and</strong> VC, <strong>and</strong> two a<strong>to</strong>ms collid<strong>in</strong>g with the<br />
small energy E as shown <strong>in</strong> figure 2.11 [30]. For large a<strong>to</strong>mic separations R the potential<br />
Vbg asymp<strong>to</strong>tically connects <strong>to</strong> two free a<strong>to</strong>ms. For small energies E the potential Vbg<br />
14