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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11.2 Current-Phase dynamics 145<br />
[148] was achieved by employ<strong>in</strong>g two different excitations methods: The first one consisted<br />
<strong>in</strong> rais<strong>in</strong>g a barrier <strong>in</strong> the center of a harmonically trapped condensate. The second method<br />
<strong>in</strong>stead consisted <strong>in</strong> lett<strong>in</strong>g the condensate equilibrate <strong>in</strong> presence of a barrier, which was then<br />
removed. The first method produces a density bump <strong>in</strong> the center of the trap, which splits<br />
<strong>in</strong>to two bright sound wavepackets; the second method on the contrary gives rise to a dip <strong>in</strong><br />
the density which splits <strong>in</strong>to two dark sound wavepackets.<br />
The excitation method we adopt is a comb<strong>in</strong>ation of these two: The <strong>in</strong>itial condensate<br />
is at equilibrium <strong>in</strong> a one-dimensional optical lattice superimposed to a simple box potential.<br />
We then switch on <strong>and</strong> off a gaussian potential barrier <strong>in</strong> the center. This procedure has the<br />
advantage that the ground states of the <strong>in</strong>itial <strong>and</strong> f<strong>in</strong>al potential are identical. For zero lattice<br />
depth, we get two composed bright-dark sound signals propagat<strong>in</strong>g symmetrically outwards.<br />
The potential creat<strong>in</strong>g the barrier is written as a product of its spatial <strong>and</strong> temporal dependence<br />
VB(x, t) =VBx(x)VBt(t) , (11.1)<br />
where<br />
<br />
VBx(x) =bER exp −x 2 /(wd) 2<br />
, (11.2)<br />
VBt(t) =s<strong>in</strong> 4<br />
<br />
πERt<br />
. (11.3)<br />
¯hTp<br />
The tunable parameters are the width of the barrier w, its height b <strong>and</strong> the time scale Tp.<br />
They are subject to the constra<strong>in</strong>ts<br />
w ≫ 1 , (11.4)<br />
<strong>in</strong> order to address only the quasi-momenta <strong>in</strong> the central part of the Brillou<strong>in</strong> zone,<br />
to ensure that the produced excitations are phonons, <strong>and</strong><br />
wd ≫ ξ, (11.5)<br />
Tp > 1 (11.6)<br />
<strong>in</strong> order to excite the lowest Bogoliubov b<strong>and</strong> only. Note that for typical densities <strong>and</strong> lattice<br />
spac<strong>in</strong>gs, w ≫ 1 automatically implies wd ≫ ξ.<br />
11.2 Current-Phase dynamics<br />
In order to study sound propagation <strong>in</strong> presence of the lattice, we use the GP-equation<br />
<br />
i¯h ˙ϕ = − ¯h2 ∂2 x<br />
2m + Vtot(x, t)+gnd|ϕ(x, t)| 2<br />
<br />
ϕ(x, t) (11.7)<br />
<strong>and</strong> the discrete nonl<strong>in</strong>ear Schröd<strong>in</strong>ger equation (DNLS)<br />
i¯h ˙ ψℓ = − δ<br />
2 (ψℓ+1 + ψℓ−1)+<br />
<br />
Vℓ(t)+U|ψℓ(t)| 2<br />
ψℓ(t), (11.8)