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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of a<strong>to</strong>ms <strong>in</strong> the two hyperf<strong>in</strong>e ground states |F = 1/2,mF = 1/2〉 <strong>and</strong> |F = 1/2,mF =<br />
−1/2〉. Each energy level will then be filled with two a<strong>to</strong>ms up <strong>to</strong> the Fermi energy.<br />
The production of a s<strong>in</strong>gle-a<strong>to</strong>m Fock state can be separated <strong>in</strong><strong>to</strong> three steps,<br />
<strong>and</strong> the fidelity of each of these steps has <strong>to</strong> be analyzed.<br />
Step 1 is the production of the degenerate gas itself. The limit on the fidelity is<br />
given by the fidelity of hav<strong>in</strong>g the ground state of the trap filled with two a<strong>to</strong>ms.<br />
Step 2 is the laser cull<strong>in</strong>g sequence or the controlled reduction of the trapp<strong>in</strong>g<br />
potential. In this step the fidelity will be limited by the precision with which the po-<br />
tentials can be controlled <strong>and</strong> by the probability of excit<strong>in</strong>g a<strong>to</strong>ms out of the ground<br />
state of the trap. The larger the energy splitt<strong>in</strong>g between different energy eigenstates,<br />
the higher the achievable fidelity. After the laser cull<strong>in</strong>g process the trap depth should<br />
be <strong>in</strong>creased aga<strong>in</strong> <strong>to</strong> preserve the Fock state. This step is able <strong>to</strong> produce even number<br />
Fock states.<br />
Step 3 allows <strong>to</strong> go from a two-a<strong>to</strong>m Fock state <strong>to</strong> go <strong>to</strong> a one-a<strong>to</strong>m Fock state.<br />
This is achieved by splitt<strong>in</strong>g the trapp<strong>in</strong>g potentials <strong>in</strong><strong>to</strong> two separate wells.<br />
The ground state occupation probability <strong>in</strong> a degenerate gas will depend on the<br />
temperature of the gas. The average number of fermions with energy ǫi <strong>in</strong> state i is<br />
given by the Fermi-Dirac distribution<br />
ni =<br />
1<br />
e (ǫi−µ)/kBT +1 . (6.1)<br />
Approximat<strong>in</strong>g the chemical potential with the Fermi energy, µ ≈ EF, <strong>and</strong> assum<strong>in</strong>g ǫ1<br />
<strong>to</strong> be negligible, the ground state occupation probability can be estimated by<br />
n1 =<br />
1<br />
e −EF/kBT +1 . (6.2)<br />
Temperatures of T ≈ 0.05TF have previously been achieved <strong>in</strong> degenerate Fermi gases<br />
[104, 105]. At this temperature the ground state occupation probability is<br />
n1 ≈ 1−2×10 −9<br />
(6.3)<br />
<strong>and</strong> the loss of fidelity from vacancies <strong>in</strong> the ground state occupation are therefore<br />
negligible.<br />
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