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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6.2 Tight b<strong>in</strong>d<strong>in</strong>g regime 81<br />
The lead<strong>in</strong>g contribution yields the s<strong>in</strong>gle particle harmonic oscillator groundstate where σ =<br />
s−1/4d/π = ¯h/m˜ω for the harmonic well with frequency ˜ω =2 √ sER/¯h, while the second<br />
term is a small correction aris<strong>in</strong>g from the anharmonicity which slightly <strong>in</strong>creases the width σ<br />
of the groundstate.<br />
Insert<strong>in</strong>g the gaussian ansatz <strong>in</strong>to the expressions (6.30) <strong>and</strong> (6.33) for the on-site contribution<br />
to the energy <strong>and</strong> the chemical potential, we obta<strong>in</strong><br />
ε0<br />
ER<br />
µ0<br />
ER<br />
= d2<br />
2π 2<br />
<br />
1 1π2 + s<br />
σ2 2d2 σ2 − 1π4<br />
σ4<br />
4d4 <br />
+ 1 gn d 1<br />
√ , (6.51)<br />
8π ER π σ<br />
= ε0<br />
+<br />
ER<br />
1 gn d 1<br />
√ . (6.52)<br />
8π ER π σ<br />
With<strong>in</strong> the gaussian approximation, the <strong>in</strong>verse compressibility (6.44) can be rewritten as<br />
κ −1 = gnd<br />
√ 2πσ<br />
<strong>and</strong> the tight b<strong>in</strong>d<strong>in</strong>g effective coupl<strong>in</strong>g constant (6.45) takes the form<br />
˜g = gd<br />
√ 2πσ<br />
(6.53)<br />
(6.54)<br />
with σ given by (6.50). For s =10,gn=0.5ER the approximation κ −1 =˜gn with ˜g given by<br />
Eq.(6.54) differs from the exact value of κ −1 by less than 1%.<br />
In section 5.4, we have found that the average density at the central site of a condensate<br />
loaded <strong>in</strong> the comb<strong>in</strong>ed potential of optical lattice <strong>and</strong> harmonic trap decreases like nl=0 ∼<br />
(˜g/g) −3/5 ∼ s −3/20 . As already mentioned there, the decrease of the average density at<br />
the trap center (5.31) is to be contrasted with the <strong>in</strong>crease of the non-averaged peak density<br />
n(r⊥ =0,z =0)∼ (˜g/g) 2/5 ∼ s 1/10 . We can now prove the latter statement us<strong>in</strong>g the<br />
gaussian ansatz (6.46) with σ given by (6.49): The peak density then reads<br />
n(r⊥ =0,z =0)=f(z =0) 2 nl=0(r⊥ =0;s) = 1<br />
π1/2 (µ − µgn=0)<br />
, (6.55)<br />
σ ˜g<br />
where we have used the approximative solution (µ − µgn=0)/˜g for the average density profile<br />
(see Eq.(5.31)) with µ − µgn=0 <strong>and</strong> ˜g given by Eqs.(5.29) <strong>and</strong> (6.54) respectively. At s =0,<br />
the density at the center is given by n(r⊥ =0,z =0)=µ/g where µ is the usual TF-value<br />
of the chemical potential (see Eq.(5.29) with ˜g = g <strong>and</strong> µgn=0 =0). It follows that the ratio<br />
between the peak densities at large s <strong>and</strong> at s =0equals √ 2(˜g/g) 2/5 .Fors =20<strong>and</strong> s =50,<br />
this amounts to a 32% <strong>and</strong> 46% <strong>in</strong>crease respectively.