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Nonlinear Fiber Optics - 4 ed. Agrawal

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406 Chapter 10. Four-Wave Mixing<br />

Figure 10.18: Parametric gain as a function of ellipticity angle for κ = 0 (solid curve) and κ ≠ 0<br />

(dash<strong>ed</strong> curve) when the two pumps are elliptically polariz<strong>ed</strong> with orthogonal SOPs.<br />

they can make the pump SOPs nonorthogonal even if they were orthogonal initially at<br />

z = 0.<br />

To study such polarization changes, it is useful to write Eqs. (10.5.6) and (10.5.7)<br />

in the Stokes space after introducing the Stokes vectors of the two pumps as<br />

S 1 = 〈A 1 |σ|A 1 〉, S 2 = 〈A 2 |σ|A 2 〉, (10.5.18)<br />

where σ = σ 1 ê 1 + σ 2 ê 2 + σ 3 ê 3 is the Pauli spin vector in the Stoke space. Recall that<br />

a Stokes vector moves on the surface of the Poincaré sphere; it lies in the equatorial<br />

plane for linearly polariz<strong>ed</strong> light and points toward a pole for circularly polariz<strong>ed</strong> light.<br />

In the convention adopt<strong>ed</strong> here, the north pole corresponds to left-circular polarization.<br />

Recall also that orthogonally polariz<strong>ed</strong> pumps are represent<strong>ed</strong> by two Stokes vectors<br />

that point in opposite directions on the Poincaré sphere.<br />

By differentiating S 1 and S 2 and using Eqs. (10.5.6) and (10.5.7), one can show<br />

that the Stokes vectors for the two pumps satisfy<br />

dS 1<br />

dz = 2γ<br />

3 [(S 13 + 2S 23 )ê 3 − 2S 2 ] × S 1 , (10.5.19)<br />

dS 2<br />

dz = 2γ<br />

3 [(S 23 + 2S 13 )ê 3 − 2S 1 ] × S 2 , (10.5.20)<br />

where S j3 is the third component of S j (along the ê 3 direction). This equation shows<br />

that the SPM rotates the Stokes vector along the vertical direction. In contrast, the two<br />

XPM terms combine such that the XPM rotates the Stokes vector along a vector that lies<br />

in the equatorial plane. Equations (10.5.19) and (10.5.20) can be solv<strong>ed</strong> numerically

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