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Nonlinear Fiber Optics - 4 ed. Agrawal

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284 Chapter 8. Stimulat<strong>ed</strong> Raman Scattering<br />

Figure 8.4: Five Stokes lines S 1 to S 5 generat<strong>ed</strong> simultaneously using 1.06-μm pump pulses.<br />

Vertical line corresponds to residual pump. Powers were measur<strong>ed</strong> through a monochromator<br />

with 1.5-nm resolution. (After Ref. [37]; c○1978 IEEE.)<br />

line shape of the first-order Stokes line, generat<strong>ed</strong> by launching in a 100-m-long fiber<br />

pump pulses of about 1-ns duration, obtain<strong>ed</strong> from a mode-lock<strong>ed</strong> argon laser (λ p =<br />

514.5 nm). Figure 8.5 shows the observ<strong>ed</strong> spectra at three pump powers. The spectra<br />

exhibit a broad peak at 440 cm −1 (13.2 THz) and a narrow peak at 490 cm −1<br />

(14.7 THz). As pump power is increas<strong>ed</strong>, the peak power of the broad peak saturates<br />

while that of the narrow peak keeps increasing.<br />

The appearance of the double-peak Stokes spectrum can be understood by noting<br />

from Figure 8.2 that the dominant peak in the Raman-gain spectrum actually consists<br />

of two peaks whose locations exactly coincide with the two peaks in the Stokes spectra<br />

of Figure 8.5. A detail<strong>ed</strong> numerical model, in which the shape of the Raman-gain spectrum<br />

is includ<strong>ed</strong> and each spectral component of the Stokes line is propagat<strong>ed</strong> along<br />

the fiber including both the Raman gain and spontaneous Raman scattering, pr<strong>ed</strong>icts<br />

line shapes in agreement with the experimentally observ<strong>ed</strong> spectra [45].<br />

The features seen in Figure 8.5 can be understood qualitatively as follows. Spontaneous<br />

Raman scattering generates Stokes light across the entire frequency range of<br />

the Raman-gain spectrum. After a short length of fiber, these weak signals are amplifi<strong>ed</strong><br />

with the appropriate gain coefficients while more spontaneous light is add<strong>ed</strong>. At<br />

low pump powers, the observ<strong>ed</strong> Stokes spectrum looks like exp[g R (Ω)] because of the<br />

exponential amplification process. As pump power is increas<strong>ed</strong>, the high-frequency<br />

peak at 440 cm −1 can pump the low-frequency peak at 490 cm −1 through the Ramanamplification<br />

process. This is precisely what is seen in Figure 8.5. Eventually, the<br />

Stokes power becomes high enough to generate a second-order Stokes line. Even<br />

though this model is bas<strong>ed</strong> on the CW theory of SRS, it is able to explain the qual-

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