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Nonlinear Fiber Optics - 4 ed. Agrawal

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6.3. Evolution of Polarization State 193<br />

Figure 6.6: Trajectories showing motion of the Stokes vector on the Poincaré sphere. (a) Linear<br />

birefringence case (upper left); (b) nonlinear case with Δβ = 0 (upper right); (c) mix<strong>ed</strong> case with<br />

Δβ > 0 and P 0 > P cr (lower row). Left and right spheres in the bottom row show the front and<br />

back of the Poincaré sphere. (After Ref. [33]; c○1986 OSA.)<br />

In the purely nonlinear case of isotropic fibers (Δβ = 0), W L = 0. The Stokes<br />

vector now rotates around the S 3 axis with an angular velocity 2γS 3 /3 (upper right<br />

sphere in Figure 6.6). This rotation is referr<strong>ed</strong> to as self-induc<strong>ed</strong> ellipse rotation, or as<br />

nonlinear polarization rotation, because it has its origin in the nonlinear birefringence.<br />

Two fix<strong>ed</strong> points in this case correspond to the north and south poles of the Poincaré<br />

sphere and represent right and left circular polarizations, respectively.<br />

In the mix<strong>ed</strong> case, the behavior depends on the power of incident light. As long as<br />

P 0 < P cr , nonlinear effects play a minor role, and the situation is similar to the linear<br />

case. At higher power levels, the motion of the Stokes vector on the Poincaré sphere<br />

becomes quite complicat<strong>ed</strong> because W L is orient<strong>ed</strong> along the S 1 axis while W NL is<br />

orient<strong>ed</strong> along the S 3 axis. Moreover, the nonlinear rotation of the Stokes vector along<br />

the S 3 axis depends on the magnitude of S 3 itself. The bottom row in Figure 6.6 shows<br />

motion of the Stokes vector on the front and back of the Poincaré sphere in the case<br />

P 0 > P cr . When input light is polariz<strong>ed</strong> close to the slow axis (left sphere), the situation<br />

is similar to the linear case. However, the behavior is qualitatively different when input<br />

light is polariz<strong>ed</strong> close to the fast axis (right sphere).<br />

To understand this asymmetry, let us find the fix<strong>ed</strong> points of Eqs. (6.3.17) and<br />

(6.3.18) by setting the z derivatives to zero. The location and number of fix<strong>ed</strong> points<br />

depend on the beam power P 0 launch<strong>ed</strong> inside the fiber. More specifically, the number<br />

of fix<strong>ed</strong> points changes from two to four at a critical power level P cr defin<strong>ed</strong> in Eq.<br />

(6.3.10). For P 0 < P cr , only two fix<strong>ed</strong> points, (S 0 ,0,0) and (−S 0 ,0,0), occur; these<br />

are identical to the low-power case. In contrast, when P 0 > P cr , two new fix<strong>ed</strong> points

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