B. Quasiprobability distributions using squeezed-state expansionsξ m that would minimise the spread in phase space. But not only do we not know thisoptimum value, we also have no guarantee that it exists as a constant independent <strong>of</strong> thesystem dynamics. In fact, we would expect the optimum value ξ m to be correlated toα (for the single-mode case the phase <strong>of</strong> ξ m must be such as to minimise the amplitudefluctuations). So we need a phase-space representation in which ξ is a variable:∫ˆρ = dαdα ∗ dξdξ ∗ P (α, α ∗ ,ξ,ξ ∗ ) ∣ ∣α, ξ 〉〈 α, ξ ∣ (B.11)To obtain evolution equations for ξ, we need to rewrite the effect <strong>of</strong> the creation andannihilations on the squeezed state in terms <strong>of</strong> partial derivatives with respect to ξ, inthe manner <strong>of</strong> Eq. (B.7). To prevent any higher order derivative terms from appearingin the evolution equation for the P distribution, we need direct operator correspondencesfor â 2 and â †2 . One may consider doing this via the squeezing operator S(ξ,ξ ∗ ). Thesimplest way to differentiate this operator (because [ â 2 , â †2] does not commute with â 2 orâ †2 )appearstobeL(ξ,ξ ∗ )S(ξ,ξ ∗ ) =(= 1 2ξ ∗ ∂∂ξ ∗ + ξ ∂ )S(ξ,ξ ∗ )∂ξ(ξ ∗ â 2 − ξâ †2) S(ξ,ξ ∗ ),(B.12)which is not useful, since we cannot generate operator correspondences separately for â 2and â †2 . The exponent <strong>of</strong> S(ξ,ξ ∗ ) can be factored to find ∂ ∂ξ S andlike[156]∂∂ξ ∗ S using resultse ξ∗Â−ξ† = e −ξ† e − ln cosh r ˆBe ξ∗ ,(B.13)where  = 1 2â2 and ˆB =â † â + 1 2. But this does not appear to lead to anything moreuseful.Alternatively the phase <strong>of</strong> ξ can be locked into that <strong>of</strong> α to ensure an expansion inamplitude-squeezed states:ˆρ =∫dαdα ∗ drP (α, α ∗ ,r) ∣ ∣ α, r〉〈α, r∣ ∣.(B.14)This reduces the phase-space dimensionality, but has complications <strong>of</strong> its own: sinceS(ξ,ξ ∗ ) −→ S(α, α ∗ ,r), the correspondences for â and â † must be rederived.Thus there are many ways in which generalised phase-space representations couldbe generated. However, finding one which gives exact phase-space equations (regardless<strong>of</strong> whether these give improved statistics) is not a trivial matter, without having thesimplicity <strong>of</strong> coherent states.175
Bibliography[1] Agrawal, G. P. Nonlinear Fiber Optics, second ed. Academic Press, 1995.[2] Anderson, B. P., and Kasevich, M. A. Macroscopic quantum interference fromatomic tunnel arrays. Science 282 (Nov. 1998), 1686–1689.[3] Anderson, M. H., Ensher, J. R., Matthews, M. R., Weiman, C. E., andCornell, E. A. Observations <strong>of</strong> <strong>Bose</strong>-<strong>Einstein</strong> condensation in a dilute atomicvapor. Science 269, 5221 (July 14 1995), 198–201.[4] Andrews, M. R., Townsend, C. G., and Ketterle, W. Observation <strong>of</strong> interferencebetween two <strong>Bose</strong> condensates. Science 275, 5300 (Jan. 31 1997), 637.[5] Anglin, J. R., and Zurek, W. H. Vortices in the wake <strong>of</strong> rapid <strong>Bose</strong>-<strong>Einstein</strong>condensation. Physical Review Letters 83, 9 (Aug. 30 1999), 1707–1710.[6] Arecchi,F.T.,Courtens,E.,Gilmore,R.,andThomas,H.Atomic coherentstates in quantum optics. Physical Review A 6, 6 (Dec. 1972), 2211–2236.[7] Baboiu, D.-M., Mihalache, D., and Panoiu, N.-C. Combined influence <strong>of</strong>amplifier noise and intrapulse Raman scattering on the bit-rate limit <strong>of</strong> optical fibercommunication systems. Optics Letters 20, 18 (Sept. 18 1995), 1865–1867.[8] Berg-Sørensen, K. Kinetics for evaporative cooling <strong>of</strong> a trapped gas. PhysicalReview A 55, 1 (Feb. 1997), 1281–1287.[9] Bergman, K., Haus, H. A., and Shirasaki, M. Applied <strong>Physics</strong> B 55, 3 (Sept.1 1992), 242.[10] Bernstein, L., Eilbeck, J. C., and Scott, A. C. The quantum theory <strong>of</strong> localmodes in a coupled system <strong>of</strong> nonlinear oscillators. Nonlinearity 3 (1990), 293–323.176
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