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Nonlinear Fiber Optics - 4 ed. Agrawal

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4.2. Effect of Group-Velocity Dispersion 95<br />

Figure 4.11: (a) Temporal and (b) spectral evolution of an initially unchirp<strong>ed</strong> Gaussian pulse<br />

with N = 30 at a distance z = 0.1L D in the normal-dispersion regime of an optical fiber.<br />

travels down the fiber. However, as seen from Eqs. (3.2.14) and (4.1.9), although the<br />

GVD-induc<strong>ed</strong> chirp is linear in time, the SPM-induc<strong>ed</strong> chirp is far from being linear<br />

across the entire pulse. Because of the nonlinear nature of the composite chirp, different<br />

parts of the pulse propagate at different spe<strong>ed</strong>s [52]. In particular, in the case of normal<br />

GVD (β 2 > 0), the r<strong>ed</strong>-shift<strong>ed</strong> light near the leading <strong>ed</strong>ge travels faster and overtakes<br />

the unshift<strong>ed</strong> light in the forward tail of the pulse. The opposite occurs for the blueshift<strong>ed</strong><br />

light near the trailing <strong>ed</strong>ge. In both cases, the leading and trailing regions of<br />

the pulse contain light at two different frequencies that interfere. Oscillations near the<br />

pulse <strong>ed</strong>ges in Figure 4.11 are a result of such interference.<br />

The phenomenon of optical wave breaking can also be understood as a four-wave<br />

mixing process (see Chapter 10). <strong>Nonlinear</strong> mixing of two different frequencies ω 1<br />

and ω 2 in the pulse tails creates new frequencies at 2ω 1 − ω 2 and 2ω 2 − ω 1 . The<br />

spectral sidelobes in Figure 4.12 represent these new frequency components. Temporal<br />

oscillations near pulse <strong>ed</strong>ges and the spectral sidelobes are manifestations of the same<br />

phenomenon. It is interesting to note that optical wave breaking does not occur in the<br />

case of anomalous GVD. The reason is that the r<strong>ed</strong>-shift<strong>ed</strong> part of the pulse cannot take<br />

over the fast-moving forward tail. Instead, the energy in the pulse tail spreads out, and<br />

the pulse acquires a p<strong>ed</strong>estal [52].<br />

The results shown in Figures 4.11 and 4.12 are obtain<strong>ed</strong> for an unchirp<strong>ed</strong> pulse<br />

(C = 0). Pulses emitt<strong>ed</strong> from practical laser sources are often chirp<strong>ed</strong> and may follow<br />

quite a different evolution pattern depending on the sign and magnitude of the chirp<br />

parameter C [49]. Figure 4.13 shows the pulse shape and the spectrum for a chirp<strong>ed</strong>

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