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Chapter 4<br />

Data analysis<br />

A correct data analysis is crucial to every experiment. In experiments on<br />

cold atoms, the raw data is normally the <strong>de</strong>nsity distribution of the atoms<br />

acquired using absorption imaging techniques. Most often, the total<br />

number of the atoms and the extent of the cloud in the two directions is<br />

sufficient to interpret the data and can be achieved easily by performing<br />

an appropriate fit on the atomic distribution. Here we want to focus<br />

on a more advanced method of data analysis: firstly, the shape of the<br />

cloud contains important information about the temperature of the cloud,<br />

which can be extracted using appropriate fitting functions. Secondly,<br />

the cloud we see on the computer screen is only a two dimensional<br />

projection. Knowing that the original cloud has rotational symmetry, we<br />

can reconstruct the three dimensional distribution of the atoms.<br />

4.1 Determination of the temperature of a fermionic<br />

gas<br />

The temperature of a c<strong>la</strong>ssical gas in a trap can be <strong>de</strong>termined easily:<br />

after a time-of-flight expansion, the momentum distribution of the gas<br />

is known from which the temperature can be easily calcu<strong>la</strong>ted. The<br />

case of a bosonic gas is very different: once the gas has con<strong>de</strong>nsed<br />

into a Bose-Einstein-Con<strong>de</strong>nsate, the fraction of the non-con<strong>de</strong>nsed<br />

atoms is directly re<strong>la</strong>ted to the temperature of the gas. At very low<br />

temperatures, the con<strong>de</strong>nsate becomes nearly pure, and a temperature<br />

measurement becomes a task that is difficult to accomplish. The case<br />

of a fermionic gas is as tricky. At low temperatures, especially below<br />

the Fermi temperature, the momentum distribution shows no changes<br />

except that the smearing of the step in the Fermi distribution.<br />

73

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