Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/4822
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dc.contributorDepartment of Electronic and Information Engineering-
dc.creatorChow, KW-
dc.creatorMerhasin, IM-
dc.creatorMalomed, BA-
dc.creatorNakkeeran, K-
dc.creatorSenthilnathan, K-
dc.creatorWai, PKA-
dc.date.accessioned2014-12-11T08:24:37Z-
dc.date.available2014-12-11T08:24:37Z-
dc.identifier.issn1539-3755-
dc.identifier.urihttp://hdl.handle.net/10397/4822-
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsPhysical Review E © 2008 The American Physical Society. The Journal's web site is located at http://pre.aps.org/en_US
dc.subjectComputer simulationen_US
dc.subjectEnergy gapen_US
dc.subjectLight propagationen_US
dc.subjectOptical Kerr effecten_US
dc.subjectSolitonsen_US
dc.subjectTime varying systemsen_US
dc.titlePeriodic waves in fiber Bragg gratingsen_US
dc.typeJournal/Magazine Articleen_US
dc.description.otherinformationAuthor name used in this publication: P. K. A. Waien_US
dc.identifier.spage1-
dc.identifier.epage8-
dc.identifier.volume77-
dc.identifier.issue2-
dc.identifier.doi10.1103/PhysRevE.77.026602-
dcterms.abstractWe construct two families of exact periodic solutions to the standard model of fiber Bragg grating (FBG) with Kerr nonlinearity. The solutions are named “sn” and “cn” waves, according to the elliptic functions used in their analytical representation. The sn wave exists only inside the FBG’s spectral bandgap, while waves of the cn type may only exist at negative frequencies (ω<0), both inside and outside the bandgap. In the long-wave limit, the sn and cn families recover, respectively, the ordinary gap solitons, and (unstable) antidark and dark solitons. Stability of the periodic solutions is checked by direct numerical simulations and, in the case of the sn family, also through the calculation of instability growth rates for small perturbations. Although, rigorously speaking, all periodic solutions are unstable, a subfamily of practically stable sn waves, with a sufficiently large spatial period and ω>0, is identified. However, the sn waves with ω<0, as well as all cn solutions, are strongly unstable.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationPhysical review. E, Statistical, nonlinear, and soft matter physics, Feb. 2008, v. 77, no. 2, 026602, p. 1-8-
dcterms.isPartOfPhysical review. E, Statistical, nonlinear, and soft matter physics-
dcterms.issued2008-02-07-
dc.identifier.isiWOS:000253763800060-
dc.identifier.scopus2-s2.0-38949174013-
dc.identifier.eissn1550-2376-
dc.identifier.rosgroupidr37561-
dc.description.ros2007-2008 > Academic research: refereed > Publication in refereed journal-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_IR/PIRAen_US
dc.description.pubStatusPublisheden_US
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