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5.1. MOMENTUM DISTRIBUTION<br />

get na 3 = 3π/16x 2 0 , or ∆2 = 4¯h 4 k 3 F /3πm2 a. Then from (5.4) we see that<br />

µ = −¯h 2 /2ma 2 . This is exactly the molecu<strong>la</strong>r binding energy per atom<br />

that has been found in equation (2.25). Developing the summands in the<br />

number equation (2.35) for small values of ∆/µ, in combination with the<br />

result from this paragraph, leads to<br />

nk = 4 3 1<br />

(kFa)<br />

3π (k2a2 + 1) 2<br />

(5.6)<br />

This result is interesting as it is the Fourier transform of a molecu<strong>la</strong>r<br />

bound state. This means that the center of mass motion of the molecules<br />

is con<strong>de</strong>nsed into p = 0 and only the re<strong>la</strong>tive motion of the atoms in<br />

the molecule is relevant. This shows that in the BEC limit the BCS<br />

wavefunction in<strong>de</strong>ed <strong>de</strong>scribes a Bose-Einstein-Con<strong>de</strong>nsate of molecules.<br />

5.1.4 Experiments<br />

We measure the momentum distribution at three different magnetic<br />

fields: at the unitarity limit at 83 mT, in the molecu<strong>la</strong>r regime and on<br />

the BCS si<strong>de</strong> of the Feshbach resonance.<br />

We perform evaporative cooling as <strong>de</strong>scribed in section 3.6. At the<br />

end of this cooling stage we lower both trapping <strong>la</strong>sers to 10% of their<br />

initial power, leading to transverse trapping frequencies of 2 kHz in both<br />

the horizontal and vertical beam. The <strong>de</strong>sired field is then ramped in<br />

500 ms to the <strong>de</strong>sired magnetic field.<br />

At this point we would like to verify that we are in<strong>de</strong>ed sufficiently<br />

cold to be con<strong>de</strong>nsed into the superfluid state. The easiest way to achieve<br />

that is to ramp the field to the BEC si<strong>de</strong> of the resonance and let the<br />

gas expand in the presence of the field. If the expan<strong>de</strong>d gas is elliptic,<br />

we know that the gas is Bose-Einstein con<strong>de</strong>nsed (we will go into more<br />

<strong>de</strong>tails on this in section 5.3). But this will only happen if the trap is<br />

non-isotropic in the observed p<strong>la</strong>ne, which is not the case. Therefore, we<br />

recompress the horizontal beam in 200 ms to a trap frequency of 5,5 kHz.<br />

Technically, it would not be necessary to recompress the horizontal<br />

beam for the momentum distribution experiments, but as it does not<br />

disturb the momentum distribution we prefer to keep the verified state<br />

as is.<br />

At the end, we switch off the trap, which takes about 5 µs. The gas<br />

expands for 0,5 ms, after which we take an absorption image. In or<strong>de</strong>r<br />

to reconstruct the three-dimensional distribution, we perform an inverse<br />

Abel transform as <strong>de</strong>scribed in section 4.2.<br />

87

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