Rogue wave formation by accelerated solitons at an optical event horizon

dc.bibliographicCitation.seriesTitleWIAS Preprintseng
dc.bibliographicCitation.volume1807
dc.contributor.authorDemircan, Ayhan
dc.contributor.authorAmiranashvili, Shalva
dc.contributor.authorBrée, Carsten
dc.contributor.authorMahnke, Christoph
dc.contributor.authorMitschke, Fedor
dc.contributor.authorSteinmeyer, Günter
dc.date.accessioned2016-03-24T17:37:45Z
dc.date.available2019-06-28T08:19:25Z
dc.date.issued2013
dc.description.abstractRogue waves, by definition, are rare events of extreme amplitude, but at the same time they are frequent in the sense that they can exist in a wide range of physical contexts. While many mechanisms have been demonstrated to explain the appearance of rogue waves in various specific systems, there is no known generic mechanism or general set of criteria shown to rule their appearance. Presupposing only the existence of a nonlinear Schrödinger-type equation together with a concave dispersion profile around a zero dispersion wavelength we demonstrate that solitons may experience acceleration and strong reshaping due to the interaction with continuum radiation, giving rise to extreme-value phenomena. The mechanism is independent of the optical Raman effect. A strong increase of the peak power is accompanied by a mild increase of the pulse energy and carrier frequency, whereas the photon number of the soliton remains practically constant. This reshaping mechanism is particularly robust and is naturally given in optics in the supercontinuum generation process.
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.issn0946-8633
dc.identifier.urihttps://doi.org/10.34657/3098
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/3211
dc.language.isoengeng
dc.publisherBerlin : Weierstraß-Institut für Angewandte Analysis und Stochastik
dc.relation.issn0946-8633eng
dc.rights.licenseDieses Dokument darf im Rahmen von § 53 UrhG zum eigenen Gebrauch kostenfrei heruntergeladen, gelesen, gespeichert und ausgedruckt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden.ger
dc.rights.licenseThis document may be downloaded, read, stored and printed for your own use within the limits of § 53 UrhG but it may not be distributed via the internet or passed on to external parties.eng
dc.subject.ddc510
dc.subject.otherRogue waveeng
dc.subject.otherOptical solitoneng
dc.subject.otherUltrashort pulseeng
dc.subject.otherOptical event horizoneng
dc.titleRogue wave formation by accelerated solitons at an optical event horizon
dc.typeReporteng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorWIASeng
wgl.contributorMBIeng
wgl.subjectMathematikeng
wgl.typeReport / Forschungsbericht / Arbeitspapiereng
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