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

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4. Continuously monitored <strong>Bose</strong> condensates: quasiprobability distributionsbe rather broad, leading to large sampling errors in any numerical simulation <strong>of</strong> the correspondingphase-space equations. A more natural set <strong>of</strong> states to work with is that <strong>of</strong>the atomic coherent states ∣ ∣µ 〉 , defined in Sec. 4.3.1. Distribution functions defined interms <strong>of</strong> these states are constrained to remain on the Bloch sphere. The disadvantagein using a quasiprobability distribution that better reflects the structure <strong>of</strong> the masterequation, is that the governing equations are more complicated and not so amenable tosimple analysis.In order to obtain an equation for the atomic Q function, the following matrix elementsare needed[148]:〈µ∣ ∣ ρĴ+∣∣µ 〉 =〈µ∣ ∣ ρĴ−∣∣µ 〉 =1 ∂(1 + |µ| 2 ) 2j ∂µ(1(1 + |µ| 2 ) 2j 2jµ − µ 2 ∂∂µQ(µ) (4.34a))Q(µ),(4.34b)whereQ(µ) = ( 1+|µ| 2) 2j 〈µ∣ ∣ρ∣ ∣µ〉. (4.35)We can transform the conditional master equation (Eq. (3.21)) into a differential equationfor Q(µ) using the correspondences:as well as the conjugates <strong>of</strong> these.The resultant equation isˆρ c Ĵ + ⇐⇒ ∂ Q, (4.36a)∂µ(ˆρ c Ĵ − ⇐⇒ 2(j +1)µ − ∂ )∂µ µ2 Q, (4.36b)( )∂ˆρ c Ĵ z ⇐⇒∂µ µ − (j +1) Q, (4.36c)[ ( √ΓdWdQ(t, µ, µ ∗ )= (j +1)(µ + µ ∗ )+ 1 ∂ (1 − µ2 )2 ∂µ+ 1 ∂(2 ∂µ ∗ 1 − µ ∗2) − 2 〈 〉 ) ]Ĵ x + dt (S + L Q + D Q ) Q, (4.37a)103

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