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Nonlinear Fiber Optics - 4 ed. Agrawal

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506 Chapter 12. Novel <strong>Nonlinear</strong> Phenomena<br />

Figure 12.40: Measur<strong>ed</strong> THG spectra when 170-fs pulses at 1550 nm are launch<strong>ed</strong> along the (a)<br />

slow or (b) fast axis of a 20-cm-long microstructur<strong>ed</strong> fiber. (After Ref. [202]; c○2003 OSA.)<br />

two principal axes. Each peak appear<strong>ed</strong> as a doublet whose relative heights vari<strong>ed</strong> with<br />

the average power launch<strong>ed</strong> into the fiber. As in Figure 12.40, the longer-wavelength<br />

THG peak results from the Raman soliton that separates from the main pump pulse<br />

after a short distance into the fiber as a result of a large RIFS. The observ<strong>ed</strong> far-field<br />

patterns associat<strong>ed</strong> with the THG peaks were complex with eight lobes around a central<br />

dark spot and correspond<strong>ed</strong> to a fiber mode whose order was relatively high (>20). A<br />

theoretical model pr<strong>ed</strong>ict<strong>ed</strong> the observ<strong>ed</strong> patterns quite well. For a fiber with 1.5-μm<br />

core diameter, the mode order for which THG was phase-match<strong>ed</strong> was as high as 48.<br />

Problems<br />

12.1 Explain why the spectrum of an ultrashort pulse propagating as a soliton shifts<br />

toward longer wavelengths. Do you expect this shift to occur if the pulse were to<br />

propagate in the normal-dispersion regime of the fiber? Discuss the logic behind<br />

your answer.<br />

12.2 A short pulse with 100 W peak power propagates as a fundamental soliton inside<br />

a 10-m-long highly nonlinear fiber with γ = 100 W −1 /km and β 2 = −10 ps 2 /km.<br />

Calculate the pulse width (FWHM) and the dispersion and nonlinear lengths.<br />

Also estimate the Raman-induc<strong>ed</strong> spectral shift at the output of fiber assuming<br />

T R = 3 fs.<br />

12.3 A fourth-order soliton with 150-fs width (FWHM) undergoes fission inside a<br />

10-m-long fiber with γ = 100 W −1 /km and β 2 = −10 ps 2 /km. Calculate the<br />

widths, peak powers, and Raman-induc<strong>ed</strong> spectral shifts for the four fundamental<br />

solitons creat<strong>ed</strong>.<br />

12.4 Explain the FROG technique and sketch a typical experimental setup us<strong>ed</strong> for it.<br />

How would you extend this technique to make use of cross-correlation in place<br />

of autocorrelation?<br />

12.5 What is meant by the Cherenkov or nonsolitonic radiation? Under what conditions<br />

is this radiation emitt<strong>ed</strong> by a soliton? Derive an expression for the radiation<br />

frequency assuming that solitons are perturb<strong>ed</strong> only by the third-order dispersion.

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