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Nonlinear Fiber Optics - 4 ed. Agrawal

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194 Chapter 6. Polarization Effects<br />

emerge. The components of the Stokes vector at the location of the new fix<strong>ed</strong> points<br />

on the Poincaré sphere are given by [47]<br />

√<br />

S 1 = −P cr , S 2 = 0, S 3 = ± P0 2 − P2 cr. (6.3.21)<br />

These two fix<strong>ed</strong> points correspond to elliptically polariz<strong>ed</strong> light and occur on the back<br />

of the Poincaré sphere in Figure 6.6 (lower right). At the same time, the fix<strong>ed</strong> point<br />

(−S 0 ,0,0), corresponding to light polariz<strong>ed</strong> linearly along the fast axis, becomes unstable.<br />

This is equivalent to the pitchfork bifurcation discuss<strong>ed</strong> earlier. If the input beam<br />

is polariz<strong>ed</strong> elliptically with its Stokes vector orient<strong>ed</strong> as indicat<strong>ed</strong> in Eq. (6.3.21), the<br />

polarization state will not change inside the fiber. When the polarization state is close<br />

to the new fix<strong>ed</strong> points, the Stokes vector forms a close loop around the elliptically<br />

polariz<strong>ed</strong> fix<strong>ed</strong> point. This behavior corresponds to the analytic solution discuss<strong>ed</strong> earlier.<br />

However, if the polarization state is close to the unstable fix<strong>ed</strong> point (−S 0 ,0,0),<br />

small changes in input polarization can induce large changes at the output. This issue<br />

is discuss<strong>ed</strong> next.<br />

6.3.3 Polarization Instability<br />

The polarization instability manifests as large changes in the output state of polarization<br />

when the input power or the polarization state of a CW beam is chang<strong>ed</strong> slightly<br />

[33]–[35]. The presence of polarization instability shows that slow and fast axes of a<br />

polarization-preserving fiber are not entirely equivalent.<br />

The origin of polarization instability can be understood from the following qualitative<br />

argument [34]. When the input beam is polariz<strong>ed</strong> close to the slow axis (x axis if<br />

n x > n y ), nonlinear birefringence adds to intrinsic linear birefringence, making the fiber<br />

more birefringent. By contrast, when the input beam is polariz<strong>ed</strong> close to the fast axis,<br />

nonlinear effects decrease total birefringence by an amount that depends on the input<br />

power. As a result, the fiber becomes less birefringent, and the effective beat length<br />

increases. At a critical value of the input power nonlinear birefringence can cancel<br />

LB<br />

eff<br />

intrinsic birefringence completely, and LB<br />

eff becomes infinite. With a further increase<br />

in the input power, the fiber again becomes birefringent but the roles of the slow and<br />

fast axes are revers<strong>ed</strong>. Clearly large changes in the output polarization state can occur<br />

when the input power is close to the critical power necessary to balance the linear and<br />

nonlinear birefringences. Roughly speaking, the polarization instability occurs when<br />

the input peak power is large enough to make the nonlinear length L NL comparable to<br />

the intrinsic beat length L B .<br />

The period of the elliptic function in Eq. (6.3.11) determines the effective beat<br />

length as [34]<br />

L eff<br />

B<br />

= 2K(m)<br />

π √ |q| L B, (6.3.22)<br />

where L B is the low-power beat length, K(m) is the quarter-period of the elliptic function,<br />

and m and q are given by Eq. (6.3.13) in terms of the normaliz<strong>ed</strong> input power<br />

defin<strong>ed</strong> as p = P 0 /P cr . In the absence of nonlinear effects, p = 0, q = 1, and we recover<br />

L eff<br />

B = L B = 2π/|Δβ|. (6.3.23)

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