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Nonlinear Fiber Optics - 4 ed. Agrawal

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2.3. Pulse-Propagation Equation 39<br />

Figure 2.2: Temporal variation of the Raman response function h R (t) obtain<strong>ed</strong> by using the<br />

actual Raman-gain spectrum of silica fibers. (After Ref. [15]; c○1989 OSA.)<br />

and τ 2 = 32 fs were us<strong>ed</strong> [16]. The fraction f R can also be estimat<strong>ed</strong> from Eq. (2.3.39).<br />

Using the known numerical value of peak Raman gain, f R is found to be about 0.18<br />

[15]–[17]. One should be careful in using Eq. (2.3.40) for h R (t) because it approximates<br />

the actual Raman gain spectrum with a single Lorentzian profile, and thus fails<br />

to reproduce the hump seen in Figure 8.2 at frequencies below 5 THz. This feature<br />

contributes to the Raman-induc<strong>ed</strong> frequency shift. As a result, Eq. (2.3.40) generally<br />

underestimates this shift. A different form of h R (t) was propos<strong>ed</strong> recently to address<br />

this issue [27].<br />

Equation (2.3.36) together with the response function R(t) given by Eq. (2.3.38)<br />

governs evolution of ultrashort pulses in optical fibers. Its accuracy has been verifi<strong>ed</strong><br />

by showing that it preserves the number of photons during pulse evolution if fiber loss<br />

is ignor<strong>ed</strong> by setting α = 0 [17]. The pulse energy is not conserv<strong>ed</strong> in the presence<br />

of intrapulse Raman scattering because a part of the pulse energy is taken by silica<br />

molecules. Equation (2.3.36) includes this source of nonlinear loss. It is easy to see that<br />

it r<strong>ed</strong>uces to the simpler equation (2.3.28) for optical pulses much longer than the time<br />

scale of the Raman response function h R (t). Noting that h R (t) becomes nearly zero for<br />

t > 1 ps (see Figure 2.2), R(t) for such pulses can be replac<strong>ed</strong> by δ(t). As the higherorder<br />

dispersion term involving β 3 , the loss term involving α 1 , and the nonlinear term<br />

involving γ 1 are also negligible for such pulses, Eq. (2.3.36) r<strong>ed</strong>uces to Eq. (2.3.28).<br />

For pulses wide enough to contain many optical cycles (pulse width >100 fs), we<br />

can simplify Eq. (2.3.36) considerably by setting α 1 = 0 and γ 1 = γ/ω 0 and using the<br />

following Taylor-series expansion:<br />

|A(z,t −t ′ )| 2 ≈|A(z,t)| 2 −t ′ ∂<br />

∂t |A(z,t)|2 . (2.3.41)<br />

This approximation is reasonable if the pulse envelope evolves slowly along the fiber.

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