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Nonlinear Fiber Optics - 4 ed. Agrawal

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4.4. Higher-Order <strong>Nonlinear</strong> Effects 107<br />

where L D , L ′ D , and L NL are the three length scales defin<strong>ed</strong> as<br />

L D = T 0<br />

2<br />

|β 2 | , L′ D = T 0<br />

3<br />

|β 3 | , L NL = 1 . (4.4.2)<br />

γP 0<br />

The parameters s and τ R govern the effects of self-steepening and intrapulse Raman<br />

scattering, respectively, and are defin<strong>ed</strong> as<br />

s = 1<br />

ω 0 T 0<br />

,<br />

τ R = T R<br />

T 0<br />

. (4.4.3)<br />

Both of these effects are quite small for picosecond pulses but must be consider<strong>ed</strong> for<br />

ultrashort pulses with T 0 < 1 ps.<br />

4.4.1 Self-Steepening<br />

Self-steepening results from the intensity dependence of the group velocity [84]–[87].<br />

Its effects on SPM were first consider<strong>ed</strong> in liquid nonlinear m<strong>ed</strong>ia [2] and later extend<strong>ed</strong><br />

to optical fibers [88]–[92]. Self-steepening leads to an asymmetry in the SPMbroaden<strong>ed</strong><br />

spectra of ultrashort pulses [93]–[99].<br />

Before solving Eq. (4.4.1) numerically, it is instructive to consider the dispersionless<br />

case by setting β 2 = β 3 = 0. Equation (4.4.1) can be solv<strong>ed</strong> analytically in this<br />

specific case if we also set τ R = 0 [86]. Defining a normaliz<strong>ed</strong> distance as Z = z/L NL<br />

and neglecting fiber losses (α = 0), Eq. (4.4.1) becomes<br />

∂U<br />

∂Z + s ∂<br />

∂τ (|U|2 U)=i|U| 2 U. (4.4.4)<br />

Using U = √ I exp(iφ) in Eq. (4.4.4) and separating the real and imaginary parts, we<br />

obtain the following two equations:<br />

∂I ∂I<br />

+ 3sI = 0, (4.4.5)<br />

∂Z ∂τ<br />

∂φ ∂φ<br />

+ sI = I. (4.4.6)<br />

∂Z ∂τ<br />

Since the intensity equation (4.4.5) is decoupl<strong>ed</strong> from the phase equation (4.4.6), it<br />

can be solv<strong>ed</strong> easily using the method of characteristics. Its general solution is given<br />

by [88]<br />

I(Z,τ)= f (τ − 3sIZ), (4.4.7)<br />

where we us<strong>ed</strong> the initial condition I(0,τ)= f (τ) and f (τ) describes the pulse shape<br />

at z = 0. Equation (4.4.7) shows that each point τ moves along a straight line from its<br />

initial value, and the slope of the line is intensity dependent. This feature leads to pulse<br />

distortion. As an example, consider the case of a Gaussian pulse for which<br />

I(0,τ) ≡ f (τ)=exp(−τ 2 ). (4.4.8)<br />

From Eq. (4.4.7), the pulse shape at a distance Z is obtain<strong>ed</strong> by using<br />

I(Z,τ)=exp[−(τ − 3sIZ) 2 ]. (4.4.9)

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