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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4.2 Tight b<strong>in</strong>d<strong>in</strong>g regime 45<br />
parameter (4.30) (see for example [101]). The result reads<br />
1<br />
δj = ER<br />
2 (−1)j<br />
2<br />
π<br />
1/2 s<br />
4<br />
<br />
(j−1)/2+3/4 24(j−1)+5 e<br />
(j − 1)!<br />
−2√s , (4.35)<br />
where j =1, 2, ... is the <strong>in</strong>dex of the b<strong>and</strong> for which the tight b<strong>in</strong>d<strong>in</strong>g regime is considered. In<br />
order for expression (4.35) to be valid, the considered energy b<strong>and</strong> must be a slowly vary<strong>in</strong>g<br />
function of the quasi-momentum. Hence, the potential depth s must be sufficiently large.<br />
Fig. 4.8 depicts (4.35) as a function of potential depth for the b<strong>and</strong>s j = 1, 2. The<br />
tunnel<strong>in</strong>g parameter δj=1 of the lowest b<strong>and</strong> is much smaller than δj=2. This reflects the fact<br />
that the Wannier functions of the lowest b<strong>and</strong> concentrate at one site more easily than those<br />
of higher b<strong>and</strong>s.<br />
In Fig.4.9 we also plot the ratio between the approximative δ (4.35) for j =1<strong>and</strong> the exact<br />
δ as obta<strong>in</strong>ed from Eq.(4.33) us<strong>in</strong>g the numerical data for m∗ .Wef<strong>in</strong>dthatfors>30 (4.35)<br />
differs from the numeric result by less than 10%.<br />
δ/ER<br />
10 1<br />
10 0<br />
10 −1<br />
10 −2<br />
10<br />
10 15 20 25 30<br />
−3<br />
Figure 4.8: Tunnel<strong>in</strong>g parameter (4.35) of the 1D Mathieu problem as a function of potential<br />
depth for the b<strong>and</strong>s j =1(solid l<strong>in</strong>e) <strong>and</strong> j =2(dashed l<strong>in</strong>e).<br />
s