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

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6. <strong>Quantum</strong> effects in optical fibre communications systemsnumber dependence <strong>of</strong> the angular frequency ω:v = ∂ω∣ ∂k ∣ , ω ′′ = ∂2 ω ∣∣∣k=kck=kc∂k 2 . (6.4)The nonlinear term in Eq. (6.3) arises from the intensity dependent refractive indexn = n 0 + In 2 . It is <strong>of</strong>ten called the χ (3) effect, so named because it arises from the thirdorderterm in the expansion <strong>of</strong> the polarisation field in terms <strong>of</strong> the electric field[1]. Thecoefficient <strong>of</strong> the electronic nonlinearity is defined asχ e = (1 − f)n 2ωc 2v2, (6.5)Acwhere ω c is the carrier frequency, A is the effective cross-sectional area <strong>of</strong> the travelingmode, and f is the fraction <strong>of</strong> the nonlinearity due to the Raman gain:∫ ∞f = χ R= 2 ∫ ∞dt dωr 2 (ω)sin(ωt)χ e χ e 0 0≃ 0.2, (6.6)where the numerical value for f has been determined from a detailed fit to the experimentallymeasured Raman gain spectrum, details <strong>of</strong> which will be given later.In the last term <strong>of</strong> Eq. (6.3), the atomic vibrations within the silica structure <strong>of</strong> thefibre are modelled as a continuum <strong>of</strong> localised oscillators, and are coupled to the radiationmodes by a Raman transition with a frequency-dependent strength <strong>of</strong> r(ω). Theatomic displacement is proportional to Â+† , where the phonon annihilation and creationoperators,  and † , have the commutation relations[Â(x, ω),  † (x ′ ,ω )]′ = δ(x − x ′ )δ(ω − ω ′ ). (6.7)The frequency dependence <strong>of</strong> the coupling r(ω) has been determined empirically throughmeasurements <strong>of</strong> the Raman gain spectrum[23].Even though it has reduced dimensionality and lacks any spatially modulated terms,the fibre Hamiltonian Eq. (6.3) contains some complications not present in the atom opticsHamiltonian Eq. (2.1): it contains terms describing a finite group velocity and the Ramaninteraction. However, in a propagating frame <strong>of</strong> reference that moves with the radiationfield, the group velocity terms disappear in the Heisenberg equations <strong>of</strong> motion. Also,once we have integrated over the phonon reservoirs, the Raman terms contribute only anextra time-delayed nonlinearity and thermal noise sources to the equations <strong>of</strong> motion.125

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