Bose-Einstein Condensates in Rotating Traps and Optical ... - BEC
Bose-Einstein Condensates in Rotating Traps and Optical ... - BEC
Bose-Einstein Condensates in Rotating Traps and Optical ... - BEC
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168 Condensate fraction<br />
depletion (12.62) can be rewritten <strong>in</strong> the form ∆Ntot/Ntot = a/ √ 2πσ <strong>in</strong> co<strong>in</strong>cidence with the<br />
expression for the depletion <strong>in</strong> a disc (12.33). This means that we are not deal<strong>in</strong>g with an array<br />
of separated two-dimensional condensates, but with one condensate only be<strong>in</strong>g distributed over<br />
several sites. Equivalently, we can refer to the system as a coherent array of two-dimensional<br />
condensates, each of them conta<strong>in</strong><strong>in</strong>g a non-condensed fraction<br />
∆N<br />
N<br />
giv<strong>in</strong>g rise to a non-condensed fraction of the whole system<br />
∆Ntot<br />
Ntot<br />
= 1 <br />
<br />
∆N<br />
Nw N<br />
<br />
l<br />
= ã<br />
, (12.63)<br />
d<br />
= ã<br />
, (12.64)<br />
d<br />
where the fact that we can simply added up the number of non-condensed atoms at each site<br />
is a non-trivial step presuppos<strong>in</strong>g the coherence of the system as a whole.<br />
It is <strong>in</strong>terest<strong>in</strong>g to note that the depletion (12.62) is obta<strong>in</strong>ed by lett<strong>in</strong>g the tunnel<strong>in</strong>g<br />
parametergotozero(δ → 0). Still, the result<strong>in</strong>g depletion takes values much smaller than<br />
one provided that the conf<strong>in</strong>ement with<strong>in</strong> each well does not become <strong>in</strong>f<strong>in</strong>itely large giv<strong>in</strong>g rise<br />
to a diverg<strong>in</strong>g ˜g <strong>and</strong> hence ã 1 . The reason for this is that before lett<strong>in</strong>g δ → 0 we have taken<br />
the limit Ntot, L→∞,n= const.. This forces the system as a whole to be coherent s<strong>in</strong>ce<br />
the ratio between the Josephson tunnel<strong>in</strong>g energy EJ <strong>and</strong> the Josephson charg<strong>in</strong>g energy EC<br />
(see Eqs.(10.34,10.49)) diverges<br />
l<br />
l<br />
EJ/EC = Nκδ/2 →∞ (12.65)<br />
for fixed κ, δ as N →∞, while the average density n is kept constant. This <strong>in</strong>dicates that<br />
coherence is ma<strong>in</strong>ta<strong>in</strong>ed across the whole sample (see discussion <strong>in</strong> section 10.1).<br />
In conclusion, we can say that the result (12.62) does not tell us what happens to the<br />
condensate fraction when the system size <strong>and</strong> the total number of particles are kept fixed<br />
while the lattice is made very deep. Surely, we expect the true result to differ from (12.62)<br />
<strong>in</strong> this case: In connection with the occurence of number squeez<strong>in</strong>g <strong>and</strong> the approach to the<br />
superfluid-<strong>in</strong>sulator transition the condensed fraction should become small as a signature of<br />
the decoherence of the system break<strong>in</strong>g up <strong>in</strong>to disconnected parts each one of them occupy<strong>in</strong>g<br />
one lattice site.<br />
1D thermodynamic limit<br />
We have seen that <strong>in</strong> the thermodynamic limit, the quantum depletion is upper-bounded by<br />
the usually very small quantity ã/d. If the cont<strong>in</strong>uum approximation (12.58) <strong>in</strong> the radial<br />
1 If δ → 0 is achieved by lett<strong>in</strong>g s →∞,also˜g →∞<strong>and</strong> thus ã →∞(see Eq.(6.54) with σ given by<br />
(6.50)). Yet, there are other ways of tak<strong>in</strong>g the limit δ → 0 which do not affect ˜g: For example, the tunnel<strong>in</strong>g<br />
rate can be made zero by <strong>in</strong>creas<strong>in</strong>g d or by rais<strong>in</strong>g the barriers of the periodic potential while keep<strong>in</strong>g the<br />
potential unchanged close to its m<strong>in</strong>ima.