1989
DOI: 10.1364/ol.14.000703
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Propagation properties of dark solitons

Abstract: We numerically study the initial-value problem of the nonlinear Schrödinger equation in the normal-dispersion regime of an optical fiber. A nonchirped hyperbolic tangent input pulse having arbitrary amplitude is found to evolve into a primary dark soliton having a constant amplitude and speed. The effect of the input amplitude is to alter the pulse width of the primary dark soliton. In addition, a set of secondary dark solitons of smaller amplitude moving away from the primary pulse is also generated. It is al… Show more

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Cited by 139 publications
(34 citation statements)
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“…We also show that spectral width of the plasmonic absorption resonance that is linked to the plasmon relaxation time in gold does not allow generation of pulses shorter than 11fs using this type of absorbers. We argue that such pulse could enable the generation of short dark solitons which can propagate large distances in dispersive media without broadening [22] with high stability, low loss and low noise compared with bright solitons [16,23]. Dark pulses also can be used in spectroscopy enabling direct measurement of ultra-short excitation dynamics [4].…”
Section: Discussionmentioning
confidence: 99%
“…We also show that spectral width of the plasmonic absorption resonance that is linked to the plasmon relaxation time in gold does not allow generation of pulses shorter than 11fs using this type of absorbers. We argue that such pulse could enable the generation of short dark solitons which can propagate large distances in dispersive media without broadening [22] with high stability, low loss and low noise compared with bright solitons [16,23]. Dark pulses also can be used in spectroscopy enabling direct measurement of ultra-short excitation dynamics [4].…”
Section: Discussionmentioning
confidence: 99%
“…However, the non-vanishing boundary of dark solitons introduces serious complications when applying the perturbative methods developed for bright solitons. In early work, the particular case of linear loss was studied both numerically (Zhao & Bourkoff 1989) and analytically (Giannini & Joseph 1990). The analysis was specifically for black solitons and solved explicitly for higher order correction terms.…”
mentioning
confidence: 99%
“…This is indeed what we numerically observed. For the case ω = 0, using the Inverse Scattering Transform, one can predict that out of an initial profile of the form ψ(x, t = 0) = b tanh(cx), one black soliton and a number N 0 of pairs of grey solitons (with N 0 = n − 1, n being the integer part of the ratio b/c) [15,16], should be generated. By denoting with γ 1 and γ 2 the initial and final values of γ, one can write the initial condition for the equation:…”
Section: Numerical Resultsmentioning
confidence: 99%