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Nonlinear Fiber Optics - 4 ed. Agrawal

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26 Chapter 2. Pulse Propagation in <strong>Fiber</strong>s<br />

relations given by [1]<br />

D = ε 0 E + P, (2.1.5)<br />

B = μ 0 H + M, (2.1.6)<br />

where ε 0 is the vacuum permittivity, μ 0 is the vacuum permeability, and P and M are<br />

the induc<strong>ed</strong> electric and magnetic polarizations. For a nonmagnetic m<strong>ed</strong>ium such as<br />

optical fibers, M = 0.<br />

Maxwell’s equations can be us<strong>ed</strong> to obtain the wave equation that describes light<br />

propagation in optical fibers. By taking the curl of Eq. (2.1.1) and using Eqs. (2.1.2),<br />

(2.1.5), and (2.1.6), one can eliminate B and D in favor of E and P and obtain<br />

∇ × ∇ × E = − 1 ∂ 2 E<br />

c 2 ∂t 2 − μ ∂ 2 P<br />

0<br />

∂t 2 , (2.1.7)<br />

where c is the spe<strong>ed</strong> of light in vacuum and the relation μ 0 ε 0 = 1/c 2 was us<strong>ed</strong>. To<br />

complete the description, a relation between the induc<strong>ed</strong> polarization P and the electric<br />

field E is ne<strong>ed</strong><strong>ed</strong>. In general, the evaluation of P requires a quantum-mechanical<br />

approach. Although such an approach is often necessary when the optical frequency is<br />

near a m<strong>ed</strong>ium resonance, a phenomenological relation of the form (1.3.1) can be us<strong>ed</strong><br />

to relate P and E far from m<strong>ed</strong>ium resonances. This is the case for optical fibers in the<br />

wavelength range 0.5–2 μm that is of interest for the study of nonlinear effects. If we<br />

include only the third-order nonlinear effects govern<strong>ed</strong> by χ (3) , the induc<strong>ed</strong> polarization<br />

consists of two parts such that<br />

P(r,t)=P L (r,t)+P NL (r,t), (2.1.8)<br />

where the linear part P L and the nonlinear part P NL are relat<strong>ed</strong> to the electric field by<br />

the general relations [2]–[4]<br />

P L (r,t) =ε 0<br />

∫ t<br />

−∞<br />

P NL (r,t) =ε 0<br />

∫ t<br />

−∞<br />

χ (1) (t −t ′ ) · E(r,t ′ )dt ′ , (2.1.9)<br />

dt 1<br />

∫ t<br />

−∞<br />

dt 2<br />

∫ t<br />

−∞<br />

dt 3<br />

× χ (3) (t −t 1 ,t −t 2 ,t −t 3 ) . E(r,t 1 )E(r,t 2 )E(r,t 3 ). (2.1.10)<br />

These relations are valid in the electric-dipole approximation and assume that the<br />

m<strong>ed</strong>ium response is local.<br />

Equations (2.1.7)–(2.1.10) provide a general formalism for studying the third-order<br />

nonlinear effects in optical fibers. Because of their complexity, it is necessary to make<br />

several simplifying approximations. In a major simplification, the nonlinear polarization<br />

P NL in Eq. (2.1.8) is treat<strong>ed</strong> as a small perturbation to the total induc<strong>ed</strong> polarization.<br />

This is justifi<strong>ed</strong> because the nonlinear effects are relatively weak in silica fibers.<br />

The first step therefore consists of solving Eq. (2.1.7) with P NL = 0. Because Eq.<br />

(2.1.7) is then linear in E, it is useful to write in the frequency domain as<br />

∇ × ∇ × Ẽ(r,ω)=ε(ω) ω2<br />

Ẽ(r,ω), (2.1.11)<br />

c2

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