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Open Quantum Dynamics of Mesoscopic Bose-Einstein ... - Physics

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5. Weak force detection using a double <strong>Bose</strong>-<strong>Einstein</strong> condensatewhich is unaffected by ĤStr.If the Ω is not exactly zero then, for a strong atom-light interaction, a back actionmay develop over time which will induce tunnelling[33] through momentum fluctuations.This would directly affect the phase <strong>of</strong> the cavity field, and it also may open a way for theatom-atom interaction to have an effect. In order to prevent this, the interwell couplingmust be suppressed by switching on a high barrier, either magnetic or with a far detunedlaser pulse.5.6 Mean-field limitThe scheme outlined above depended on starting in a state which was a quantum superposition<strong>of</strong> two condensates and on the resulting entanglement. For comparison, we willanalyse the mean-field analogue to discover which features <strong>of</strong> this scheme remain in theabsence <strong>of</strong> quantum entanglement.In the mean-field limit, the system is described by a Gross-Pitaevskii (GP) equation[106,154, 185]:i ˙Φ(x, t) =(− 2 ∂ 2)2M ∂x 2 + Rx + V (x)+U 0N|Φ(x, t)| 2 Φ(x, t), (5.36)where M is the atomic mass, the constant R is the gradient <strong>of</strong> the force and U 0 is thestrength <strong>of</strong> the interparticle interactions. Suppose that the interatomic collisions are negligible.Then, when the overlap between the wells is small, we may expand the mean fieldin terms <strong>of</strong> the local wave functions <strong>of</strong> each well:Φ(x, t) =b 1 (t)e −iE0t/ u 1 (x)+b 2 (t)e −iE0t/ u 2 (x), (5.37)whereandu j (x) =√1e (x−(−1)j q 0 ) 2 /4r 2(2πr 0 ) 1 0, r0 = , (5.38)42Mω 0∫b j (t) =u ∗ j (x)Φ(x, t)dx. (5.39)The ground-state energy <strong>of</strong> each <strong>of</strong> the local modes is E 0 = (ν + ω 0 )/2, as in Ch. 2. TheGP equation (Eq. (5.36)), then generates the following equations <strong>of</strong> motion:ḃ j (t) = (−1)j+1 iRq 0b j (t)+ iΩ 2 b 3−j(t). (5.40)116

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