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dc.creatorMančić, Ana
dc.creatorBaronio, Fabio
dc.creatorHadžievski, Ljupčo
dc.creatorWabnitz, Stefan
dc.creatorMaluckov, Aleksandra
dc.date.accessioned2018-08-07T08:35:45Z
dc.date.available2018-08-07T08:35:45Z
dc.date.issued2018
dc.identifier.issn2470-0045
dc.identifier.urihttps://link.aps.org/doi/10.1103/PhysRevE.98.012209
dc.identifier.urihttps://vinar.vin.bg.ac.rs/handle/123456789/7797
dc.description.abstractWe present a statistical analysis based on the height and return-time probabilities of high-amplitude wave events in both focusing and defocusing Manakov systems. We find that analytical rational or semirational solutions, associated with extreme, rogue wave (RW) structures, are the leading high-amplitude events in this system. We define the thresholds for classifying an extreme wave event as a RW. Our results indicate that there is a strong relationship between the type of RW and the mechanism which is responsible for its creation. Initially, high-amplitude events originate from modulation instability. Upon subsequent evolution, the interaction among these events prevails as the mechanism for RW creation. We suggest a strategy for confirming the basic properties of different extreme events. This involves the definition of proper statistical measures at each stage of the RW dynamics. Our results point to the need for redefining criteria for identifying RW events.en
dc.relationinfo:eu-repo/grantAgreement/MESTD/Integrated and Interdisciplinary Research (IIR or III)/45010/RS//
dc.relationinfo:eu-repo/grantAgreement/EC/H2020/691051/EU//
dc.relationRussian Ministry of Science and Education (14.Y26.31.0017)
dc.rightsrestrictedAccess
dc.sourcePhysical Review E
dc.subjectmodulation instabilityen
dc.subjectSchrodinger-equationsen
dc.subjectmechanismsen
dc.subjecteventsen
dc.titleStatistics of vector Manakov rogue wavesen
dc.typearticleen
dc.rights.licenseARR
dcterms.abstractМанчић, Aна; Баронио, Фабио; Хаджиевски, Љупчо; Wабнитз, Стефан; Малуцков, Aлександра;
dc.rights.holder© 2018 American Physical Society
dc.citation.volume98
dc.citation.issue1
dc.citation.spage012209
dc.identifier.wos000438497500005
dc.identifier.doi10.1103/PhysRevE.98.012209
dc.citation.rankM21
dc.description.otherPeer-reviewed version of the article available here: [http://vinar.vin.bg.ac.rs/handle/123456789/7798]
dc.type.versionpublishedVersion
dc.identifier.scopus2-s2.0-85050128465


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