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Nonlinear Fiber Optics - 4 ed. Agrawal

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5.5. Higher-Order Effects 157<br />

where a p , T p , C p , and φ p represent the amplitude, width, chirp, and phase of the pulse.<br />

We also allow for the temporal shift q p of the pulse envelope and the frequency shift Ω p<br />

of the pulse spectrum. All six parameters may change with z as the pulse propagates<br />

through the fiber.<br />

Using the definitions of moments in Sections 4.3.1 and 4.4.2 and the moment<br />

method, we obtain the following set of equations for the evolution of pulse parameters<br />

[167]:<br />

dT p<br />

dz =(β 2 + β 3 Ω p ) C p<br />

, (5.5.3)<br />

T p<br />

( )<br />

dC p 4<br />

dz = β2<br />

π 2 +C2 p + 4 ¯γP 0 T 0<br />

π 2 + 6Ω2 p<br />

T p π 2 (2β 2 + β 3 Ω p )<br />

+ β 3<br />

( 4<br />

π 2 + 3C2 p<br />

Tp<br />

2 )<br />

Ωp<br />

2T 2 p<br />

dq p<br />

dz = β 2Ω p + β 3<br />

2 Ω2 p + β 3<br />

6T 2 p<br />

+ 48 ¯γP 0 T 0<br />

π 2 , (5.5.4)<br />

ω 0 T p<br />

)<br />

(1 + π2<br />

4 C2 p + ¯γP 0 T 0<br />

, (5.5.5)<br />

ω 0 T p<br />

dΩ p<br />

dz<br />

= − 8T R ¯γP 0<br />

15<br />

T 0<br />

Tp<br />

3<br />

+ 2 ¯γP 0 T 0 C p<br />

, (5.5.6)<br />

3ω 0<br />

T 3 p<br />

where ¯γ = γ exp(−αz). As in Section 4.3.1, we have ignor<strong>ed</strong> the phase equation. The<br />

amplitude a p can be determin<strong>ed</strong> from the relation E 0 = 2P 0 T 0 = 2a 2 p(z)T p (z), where E 0<br />

is the input pulse energy.<br />

It is evident from Eqs. (5.5.3) through (5.5.6) that the pulse parameters are affect<strong>ed</strong><br />

considerably by the three higher-order terms in Eq. (5.5.1). Before considering their<br />

impact, we use these equations to determine the conditions under which a fundamental<br />

soliton can form. Equation (5.5.3) shows that pulse width will not change if the chirp<br />

C p remains zero for all z. The chirp equation (5.5.4) is quite complicat<strong>ed</strong>. However, if<br />

we neglect the higher-order terms and fiber losses (α = 0), this equation r<strong>ed</strong>uces to<br />

dC p<br />

dz = ( 4<br />

π 2 +C2 p<br />

)<br />

β2<br />

T 2 p<br />

+ 4γP 0<br />

π 2 T 0<br />

T p<br />

. (5.5.7)<br />

It is clear that if β 2 > 0, both terms on the right side are positive, and C p cannot remain<br />

zero even if C p = 0 initially. However, in the case of anomalous dispersion (β 2 < 0),<br />

the two terms cancel precisely when pulse parameters initially satisfy the condition<br />

γP 0 T0 2 = |β 2|. It follows from Eq. (5.2.3) that this condition is equivalent to setting<br />

N = 1.<br />

It is useful in the following discussion to normalize Eq. (5.5.1) using dimensionless<br />

variables ξ and τ defin<strong>ed</strong> in Eq. (5.2.1). The normaliz<strong>ed</strong> NLS equation takes the form<br />

i ∂u<br />

∂ξ + 1 ∂ 2 u<br />

2 ∂τ 2 + ∂ 3 u<br />

|u|2 u = iδ 3<br />

∂τ 3 − is ∂<br />

∂τ (|u|2 u)+τ R u ∂|u|2<br />

∂τ , (5.5.8)<br />

where the pulse is assum<strong>ed</strong> to propagate in the region of anomalous GVD (β 2 < 0) and<br />

fiber losses are neglect<strong>ed</strong> (α = 0). The parameters δ 3 , s, and τ R govern, respectively,

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