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It is also possible to obtain such superfluid states by increasing the density and/or changing the interaction strength. Here, as we consider a fixed total number of atoms in a harmonic trap and weak interactions, it is the temperature which plays the most important role in obtaining BEC or BCS.
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85015758572
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note
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40K. This has been conjectured to be due to the differing widths of the Feshbach resonances. See [42] for further discussion on the matter.
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40
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85015789039
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note
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We note that there is a certain similarity between entropic cooling and forced evaporative cooling [51].
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41
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43
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85015784944
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1/3 for ω in all expressions.
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45
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46
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85015796935
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See [53] and references therein for more sophisticated theoretical treatments
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See [53] and references therein for more sophisticated theoretical treatments.
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47
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52
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85015791646
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note
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F are sufficient to achieve a weakly interacting BCS transition.
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