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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9.1 Macroscopic density <strong>and</strong> macroscopic superfluid velocity 117<br />
In accordance with the basic idea <strong>in</strong>troduced above, we assume nM to be approximately<br />
constant on the length scale D <strong>in</strong> the z-direction at any given time t.<br />
In analogy to the def<strong>in</strong>ition of the average density nl(r⊥), we <strong>in</strong>troduce the average zcomponent<br />
of the superfluid velocity field at site l<br />
vzl(r⊥,t)= 1<br />
ld+d/2 <br />
¯h<br />
dz<br />
d ld−d/2 m ∂zS(r⊥,z,t)<br />
<br />
= ¯h 1<br />
m d [S(r⊥,ld+ d/2,t) − S(r⊥,ld− d/2,t)] , (9.3)<br />
where S(r⊥,z,t) is the phase of the order parameter <strong>and</strong> (¯h/m)∂zS(r⊥,z,t) is the zcomponent<br />
of the superfluid velocity field obta<strong>in</strong>ed by solv<strong>in</strong>g the time-dependent GP-equation<br />
<strong>in</strong> the presence of optical lattice <strong>and</strong> an additional slowly vary<strong>in</strong>g external potential as for example<br />
a harmonic trap. The quantity (9.3) is required to be approximately constant over a<br />
distance D. Hence, we can rewrite (9.3) <strong>in</strong> the form<br />
vzl(r⊥,t)= ¯h 1<br />
m D [S(r⊥,ld+ D/2,t) − S(r⊥,ld− D/2,t)] . (9.4)<br />
Now, we go a step further <strong>and</strong> require the approximate stationary state <strong>in</strong> the w<strong>in</strong>dow of size<br />
D around the site l to be of the Bloch form ϕk = exp(iklz)˜ϕk (6.2) with quasi-momentum<br />
kl(r⊥,t). Note that kl(r⊥,t) must be a slowly vary<strong>in</strong>g function of the <strong>in</strong>dex l <strong>and</strong> the variable<br />
r⊥. The phase S <strong>in</strong> the w<strong>in</strong>dow of size D around the site l is then approximately given by<br />
S(r⊥,z,t)=kl(t)z + ˜ Sk(r⊥,z,t) , (9.5)<br />
where the second contribution ˜ Sk is the phase of the Bloch wave ˜ϕk <strong>and</strong> thus ˜ Sk(r⊥,z,t)=<br />
˜Sk(r⊥,z+ ld, t). Insert<strong>in</strong>g (9.5) <strong>in</strong>to (9.4) we f<strong>in</strong>d<br />
vzl(r⊥,t)= ¯hkl(t)<br />
m<br />
¯h ˜Sjk(r⊥,ld+ D/2,t) −<br />
+<br />
m<br />
˜ Sjk(r⊥,ld− D/2,t)<br />
. (9.6)<br />
D<br />
S<strong>in</strong>ce ˜ Sjk is periodic <strong>in</strong> z with periodicity d, the second contribution becomes small for D>>d.<br />
It can consequently be neglected for sufficiently large D <strong>and</strong> we are left with<br />
vzl(r⊥,t)= ¯hkl(r⊥,t)<br />
. (9.7)<br />
m<br />
We smooth (9.7) <strong>in</strong> the z-direction <strong>in</strong> the same way as the average density profile<br />
l → z = ld ⇒ vzl(r⊥,t) → vMz(r⊥,z,t) , (9.8)<br />
where the z-component of the macroscopic superfluid velocity field vM is given by<br />
vMz(r⊥,z,t)= ¯hk(r⊥,z,t)<br />
m<br />
. (9.9)<br />
The x, y-components vMx,vMy are given by the usual expressions (¯h/m)∂x,yS(r⊥,z,t).<br />
It is important to note that vMz =¯hk/m does not co<strong>in</strong>cide with the group velocity ¯vk<br />
of a Bloch state condensate with quasi-momentum ¯hk. This is a very peculiar feature of a