Experiments with Supersonic Beams as a Source of Cold Atoms
Experiments with Supersonic Beams as a Source of Cold Atoms
Experiments with Supersonic Beams as a Source of Cold Atoms
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Since the output power <strong>of</strong> the l<strong>as</strong>er described above is only 2 mW, the 1S − 2S<br />
transition cannot be driven effectively. Two steps are being taken to incre<strong>as</strong>e the<br />
power. The first step is the addition <strong>of</strong> a build up cavity around the atoms. This<br />
should allow the UV power to be incre<strong>as</strong>ed by a factor <strong>of</strong> around 50. The second step<br />
is to replace the ECDL and TA <strong>of</strong> the current system <strong>with</strong> an OPSL l<strong>as</strong>er [117, 118].<br />
The OPSL h<strong>as</strong> an output power <strong>of</strong> over 1.3 W and the mode quality is much better<br />
than that <strong>of</strong> the TA. This should enable more light to be coupled into the first doubler,<br />
hopefully incre<strong>as</strong>ing the output power at 486 nm to over 500 mW. This much blue<br />
power should incre<strong>as</strong>e the efficiency <strong>of</strong> the second doubler, <strong>with</strong> the goal <strong>of</strong> having<br />
50 mW <strong>of</strong> power at 243 nm. When used in conjunction <strong>with</strong> the build up cavity, the<br />
atoms should see 2.5 W <strong>of</strong> 243 nm light. Calculations performed by Robert Clark<br />
indicate that this much light should be sufficient to excite a few percent <strong>of</strong> the atoms<br />
in the trap, and enabling the l<strong>as</strong>er to be used <strong>as</strong> a background free detection method.<br />
Finally, linewidth <strong>of</strong> the OPSL (and thus the l<strong>as</strong>er linewidth broadening) can be<br />
reduced <strong>as</strong> needed by locking the l<strong>as</strong>er to an external cavity.<br />
5.4.1.3 Spectroscopic Goals<br />
While the l<strong>as</strong>er will initially be used to detect the atoms in the trap, it can also<br />
be used to perform spectroscopy on the trapped hydrogen. Of particular importance<br />
is the isotopic shift <strong>of</strong> the 1S − 2S transition in tritium. The current uncertainty on<br />
this me<strong>as</strong>urement is several MHz [119]. By lowering the uncertainty to a few hundred<br />
kHz, the size <strong>of</strong> the triton charge radius can be me<strong>as</strong>ured, which is <strong>of</strong> great interest to<br />
nuclear theorists [120]. There is no re<strong>as</strong>on why the linewidth <strong>of</strong> the OPSL should not<br />
be able to narrowed to below this uncertainty, and the waist <strong>of</strong> the beam in the cavity<br />
can be set so that the time <strong>of</strong> flight broadening is equivalent to the l<strong>as</strong>er linewidth.<br />
Since the Zeeman broadening in the trap is only a few tens <strong>of</strong> kHz, this should not<br />
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