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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the electron g-factor which causes the resonance energy <strong>of</strong> the the 1S − 2S transition<br />
to vary <strong>with</strong> magnetic field. The g-factor varies <strong>with</strong> the principle quantum number<br />
n <strong>as</strong> [108]<br />
ge(n) =ge<br />
This leads to a frequency shift <strong>of</strong> [109]<br />
<br />
1 − α2<br />
3n2 <br />
. (5.5)<br />
δν = 186kHz/T. (5.6)<br />
In the quadrupole trap, this corresponds to shift <strong>of</strong> up to 65 kHz, which will limit the<br />
resolution <strong>of</strong> any spectroscopy performed in the trap.<br />
5.4.1.2 The Hydrogen L<strong>as</strong>er<br />
The l<strong>as</strong>er which will be used to excite the 1S −2S transition is currently under<br />
construction. The original design w<strong>as</strong> b<strong>as</strong>ed on the l<strong>as</strong>er described in [110]. To create<br />
light at 243 nm, a diode l<strong>as</strong>er at 972 nm w<strong>as</strong> amplified and frequency doubled twice.<br />
This l<strong>as</strong>er w<strong>as</strong> found not to produce enough power at 243 nm to efficiently drive the<br />
transition, and the front end <strong>of</strong> the l<strong>as</strong>er is currently being replaced <strong>with</strong> an optically<br />
pumped semiconductor l<strong>as</strong>er (OPSL) at 972 nm which should enable more UV power<br />
to be generated.<br />
A schematic <strong>of</strong> the original l<strong>as</strong>er system constructed by Travis Bannerman is<br />
shown in figure 5.23. A tunable extended cavity diode l<strong>as</strong>er (ECDL) is used to produce<br />
single-mode light at 972 nm. Because the l<strong>as</strong>er frequency must be quadrupled, and<br />
the eventual excitation is a two-photon process, ph<strong>as</strong>e noise in the l<strong>as</strong>er must be<br />
reduced <strong>as</strong> much <strong>as</strong> possible. A diffraction grating mounted 27 cm from the diode<br />
creates a long cavity <strong>with</strong> acts <strong>as</strong> a flywheel, reducing high-frequency ph<strong>as</strong>e noise.<br />
The frequency <strong>of</strong> the l<strong>as</strong>er can be tuned by changing the angle <strong>of</strong> the diffraction<br />
grating <strong>with</strong> a piezo stack, and the frequency and single mode operation <strong>of</strong> the l<strong>as</strong>er<br />
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