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Experiments to Control Atom Number and Phase-Space Density in ...

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Figure 5.8: A<strong>to</strong>m number as a function of trap depth.<br />

Additionally, the optical trough truncates the spatial distribution along the x<br />

<strong>and</strong> y directions. Figure 5.9 shows the number of a<strong>to</strong>ms captured <strong>in</strong> the optical trough<br />

as a function of the separation between the end caps. A larger trap volume leads <strong>to</strong> less<br />

truncation <strong>and</strong> hence an <strong>in</strong>creased number <strong>in</strong> the a<strong>to</strong>ms captured from the ensemble.<br />

This analysis shows that the f<strong>in</strong>al phase-space density is not necessarily the best<br />

measure <strong>to</strong> evaluate the efficiency of s<strong>in</strong>gle-pho<strong>to</strong>n cool<strong>in</strong>g. The f<strong>in</strong>al phase-space density<br />

measured is a three-dimensional quantity, while the cool<strong>in</strong>g process <strong>in</strong> this implemen-<br />

tation is only one-dimensional. To evaluate the vertical phase-space compression, it is<br />

helpful <strong>to</strong> look at the transfer efficiency η from the magnetic trap <strong>to</strong> the optical trap,<br />

η = NO<br />

NB , NO is the a<strong>to</strong>m number <strong>in</strong> the optical trough <strong>and</strong> NB the number of mag-<br />

netically trapped a<strong>to</strong>ms, <strong>and</strong> compare the measured values with the maximum values<br />

expected from an adiabatic transfer process.<br />

The model describ<strong>in</strong>g the adiabatic transfer is greatly simplified by approximat<strong>in</strong>g<br />

the spatial distributions as Gaussian. The temperature distributions are assumed <strong>to</strong><br />

follow Maxwell-Boltzmann velocity distributions. Neither the magnetic nor the optical<br />

trap provide harmonic potentials <strong>and</strong> thus the approximation of the spatial profile as<br />

77

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