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Solitons in Nonlocal Media

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5.3 Constant Optical Amplification<br />

5.3 Constant Optical Amplification<br />

In the simplest case, γ can be approximated by a constant, i.e., <strong>in</strong>dependent from both<br />

the spatial coord<strong>in</strong>ates (the spatial distribution of the pump) and the <strong>in</strong>tensity I ∝ |A| 2<br />

(i.e., no ga<strong>in</strong> saturation). Fig. 5.2 shows a comparison between soliton propagation<br />

<strong>in</strong> undoped NLC [fig. 5.2(a)] and dye-doped NLC [fig. 5.2(a)]: <strong>in</strong> the latter case the<br />

power <strong>in</strong>creases with s; moreover, breath<strong>in</strong>g features are affected by the <strong>in</strong>cremented<br />

power. In this example, for γ = 100m −1 there are four maxima <strong>in</strong> <strong>in</strong>tensity along s,<br />

whereas for zero γ the maxima are only three. To better address this issue (i.e., the<br />

breath<strong>in</strong>g behavior versus ga<strong>in</strong>), fig. 5.3 displays the results at λ = 633nm for <strong>in</strong>itial<br />

beam powers of 0.5, 1.0, 1.5 and 2.0mW, respectively, plott<strong>in</strong>g the beam waist across<br />

t versus propagation s, wt(s) = 2<br />

It(t,s)t 2 dt<br />

It(t,s)dt , with It(t, s) = d<br />

0 |A|2 dx the <strong>in</strong>tensity<br />

averaged along x. The quantity wt is well suited to describe beam (soliton) breath<strong>in</strong>g<br />

dur<strong>in</strong>g amplification (or attenuation if γ < 0) along s. From the numerical simulations I<br />

f<strong>in</strong>d that wt(s) ∼ = wx(s) when w x/t are much smaller than d, wx be<strong>in</strong>g the waist across x<br />

(fig. 5.3). As predicted for highly nonlocal solitons <strong>in</strong> undoped media (γ = 0) (31; 51),<br />

the breath<strong>in</strong>g period decreases as the <strong>in</strong>itial power P<strong>in</strong> <strong>in</strong>creases. Therefore, for a fixed<br />

γ = 0, the propagation distance between two waist m<strong>in</strong>ima reduces (<strong>in</strong>creases) ow<strong>in</strong>g<br />

to amplification (attenuation). A f<strong>in</strong>ite γ affects the mean beam waist, which reduces<br />

(grows) with s for γ > 0 (γ < 0). I repeated the calculations at λ = 1064nm; fig. 5.4<br />

shows the computed waist wt(s) for P<strong>in</strong> = 0.5 and 2.0mW: self-conf<strong>in</strong>ement is obta<strong>in</strong>ed<br />

only when the power is large enough to <strong>in</strong>duce self-focus<strong>in</strong>g. Moreover, s<strong>in</strong>ce diffraction<br />

is stronger than <strong>in</strong> the red (for the same powers), waist oscillation periods are larger<br />

than <strong>in</strong> fig. 5.3 (see chapter 2 for details).<br />

Figure 5.5 shows the beam profile for λ = 633nm at s = 1.5mm with P<strong>in</strong> = 0.25mW<br />

and γ = 0 or γ = 1000m −1 , respectively. In the second case, the ga<strong>in</strong> suffices to en-<br />

hance the nonl<strong>in</strong>ear conf<strong>in</strong>ement and overcome diffraction: <strong>in</strong>deed, there is a region<br />

where the waist beg<strong>in</strong>s to decrease. Afterwards, beam width oscillates due to the <strong>in</strong>-<br />

terplay of nonl<strong>in</strong>ear self-focus<strong>in</strong>g and diffractive spread<strong>in</strong>g.<br />

After the <strong>in</strong>vestigation on beam breath<strong>in</strong>g, I discuss the amplification and its rela-<br />

tionship with the propagation coord<strong>in</strong>ate s. To this extent, I can def<strong>in</strong>e the beam<br />

power amplification at a fixed s as G(s) = P(s)/P<strong>in</strong>, i.e. the ratio between the power<br />

<strong>in</strong> s and <strong>in</strong> s = 0. I f<strong>in</strong>d that G(s) = exp(2γs) if the self-<strong>in</strong>duced waveguide has<br />

91

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