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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= E0<br />
1 −n2 √2 exp<br />
σ0<br />
± iE0<br />
√2 exp<br />
2(1+δ 2 )<br />
<br />
ik<br />
2f (x′2 +y ′2 )<br />
<br />
(1+iδ)<br />
<br />
ˆy ′<br />
<br />
ik<br />
exp<br />
2f (x′2 +y ′2 <br />
) ˆx ′<br />
Def<strong>in</strong><strong>in</strong>g I = k|E<strong>to</strong>t| 2 <strong>and</strong> I0 = k|E<strong>in</strong>c| 2 leads <strong>to</strong><br />
<br />
|E0|<br />
I0 = k<br />
2 2 |E0|<br />
+ = k|E0|<br />
2 2<br />
2<br />
<br />
|E0|<br />
I = k<br />
2<br />
2 exp<br />
1 −n 2σ0 1+δ 2<br />
<br />
+ |E0| 2<br />
2<br />
<strong>and</strong> thus<br />
I<br />
I0<br />
= 1<br />
2 exp<br />
1 −n 2σ0 1+δ 2<br />
<br />
+ 1<br />
2<br />
1<br />
=<br />
2 exp<br />
∗ −nσ<br />
1+δ 2<br />
<br />
(7.26)<br />
(7.27)<br />
(7.28)<br />
+ 1<br />
. (7.29)<br />
2<br />
The effective scatter<strong>in</strong>g cross section σ ∗ is only half of σ0. In addition, only half<br />
the light <strong>in</strong>teracts with the a<strong>to</strong>ms. The temperature of the MOT <strong>and</strong> the compressed<br />
MOT is measured us<strong>in</strong>g the setup shown <strong>in</strong> 7.38, where this calculation applies.<br />
For imag<strong>in</strong>g a<strong>to</strong>ms trapped <strong>in</strong> the CO2 laser a few changes <strong>to</strong> the optical setup<br />
shown <strong>in</strong> figure 7.38 are necessary. First, the f = 50 mm lens is removed, chang<strong>in</strong>g the<br />
magnification <strong>to</strong> be roughly 1:4. Because of the lower a<strong>to</strong>m number <strong>and</strong> the <strong>in</strong>creased<br />
magnification the signal-<strong>to</strong>-noise ratio is reduced as compared <strong>to</strong> imag<strong>in</strong>g of the MOT.<br />
Instead of us<strong>in</strong>g a polariz<strong>in</strong>g beam splitter cube <strong>to</strong> comb<strong>in</strong>e the MOT <strong>and</strong> the imag<strong>in</strong>g<br />
beam, a mirror mounted on a mo<strong>to</strong>rized flipper is added <strong>to</strong> the setup. It is then possible<br />
<strong>to</strong> use l<strong>in</strong>early polarized light for imag<strong>in</strong>g the a<strong>to</strong>ms. The <strong>in</strong>tensity <strong>in</strong> the image plane<br />
is then given by [109]<br />
I<br />
I0<br />
1 −n 2 = exp<br />
σ0<br />
1+δ 2<br />
<br />
. (7.30)<br />
The disadvantage of this setup is that a<strong>to</strong>ms cannot be imaged <strong>in</strong> the MOT, because<br />
the time the flipper requires exceeds the s<strong>to</strong>rage time of the a<strong>to</strong>ms.<br />
Lithium a<strong>to</strong>ms exp<strong>and</strong> faster than other alkali a<strong>to</strong>ms. This means that especially<br />
at MOT temperatures the a<strong>to</strong>ms can move a significant distance even dur<strong>in</strong>g the imag<strong>in</strong>g<br />
exposure time. The imag<strong>in</strong>g pulse duration is therefore restricted <strong>to</strong> between 10 µs <strong>and</strong><br />
20 µs <strong>to</strong> m<strong>in</strong>imize this effect.<br />
146