Please use this identifier to cite or link to this item: http://localhost/handle/Hannan/656638
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dc.contributor.authorYang Heen_US
dc.contributor.authorShaofei Wangen_US
dc.contributor.authorXianglong Zengen_US
dc.date.accessioned2020-05-20T10:28:59Z-
dc.date.available2020-05-20T10:28:59Z-
dc.date.issued2016en_US
dc.identifier.issn1943-0655en_US
dc.identifier.other10.1109/JPHOT.2016.2626004en_US
dc.identifier.urihttp://localhost/handle/Hannan/169746en_US
dc.identifier.urihttp://localhost/handle/Hannan/656638-
dc.descriptionen_US
dc.description.abstractTaking advantage of an extended Lugiato-Lefever equation with third-order dispersion, we numerically show that dark cavity solitons formed in normal dispersion of microresonators are capable of emitting dispersive waves in both normal and anomalous dispersion regions with two different methods, resembling the behavior of the commonly encountered bright cavity solitons. The generated dispersive waves can be accurately predicted by the dissipative radiation theory. In addition, we demonstrate the stability enhancement of Kerr frequency combs in the normal dispersion regime in case the dispersive wave is emitted by dark solitons in the presence of third-order dispersion.en_US
dc.publisherIEEEen_US
dc.relation.haspart7740022.pdfen_US
dc.subjectmicroresonators|Dark cavity soliton|dispersive wave.en_US
dc.titleDynamics of Dispersive Wave Emission From Dark Solitons in Kerr Frequency Combsen_US
dc.typeArticleen_US
dc.journal.volume8en_US
dc.journal.issue6en_US
dc.journal.titleIEEE Photonics Journalen_US
Appears in Collections:2016

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Full metadata record
DC FieldValueLanguage
dc.contributor.authorYang Heen_US
dc.contributor.authorShaofei Wangen_US
dc.contributor.authorXianglong Zengen_US
dc.date.accessioned2020-05-20T10:28:59Z-
dc.date.available2020-05-20T10:28:59Z-
dc.date.issued2016en_US
dc.identifier.issn1943-0655en_US
dc.identifier.other10.1109/JPHOT.2016.2626004en_US
dc.identifier.urihttp://localhost/handle/Hannan/169746en_US
dc.identifier.urihttp://localhost/handle/Hannan/656638-
dc.descriptionen_US
dc.description.abstractTaking advantage of an extended Lugiato-Lefever equation with third-order dispersion, we numerically show that dark cavity solitons formed in normal dispersion of microresonators are capable of emitting dispersive waves in both normal and anomalous dispersion regions with two different methods, resembling the behavior of the commonly encountered bright cavity solitons. The generated dispersive waves can be accurately predicted by the dissipative radiation theory. In addition, we demonstrate the stability enhancement of Kerr frequency combs in the normal dispersion regime in case the dispersive wave is emitted by dark solitons in the presence of third-order dispersion.en_US
dc.publisherIEEEen_US
dc.relation.haspart7740022.pdfen_US
dc.subjectmicroresonators|Dark cavity soliton|dispersive wave.en_US
dc.titleDynamics of Dispersive Wave Emission From Dark Solitons in Kerr Frequency Combsen_US
dc.typeArticleen_US
dc.journal.volume8en_US
dc.journal.issue6en_US
dc.journal.titleIEEE Photonics Journalen_US
Appears in Collections:2016

Files in This Item:
File Description SizeFormat 
7740022.pdf1.33 MBAdobe PDFThumbnail
Preview File
Full metadata record
DC FieldValueLanguage
dc.contributor.authorYang Heen_US
dc.contributor.authorShaofei Wangen_US
dc.contributor.authorXianglong Zengen_US
dc.date.accessioned2020-05-20T10:28:59Z-
dc.date.available2020-05-20T10:28:59Z-
dc.date.issued2016en_US
dc.identifier.issn1943-0655en_US
dc.identifier.other10.1109/JPHOT.2016.2626004en_US
dc.identifier.urihttp://localhost/handle/Hannan/169746en_US
dc.identifier.urihttp://localhost/handle/Hannan/656638-
dc.descriptionen_US
dc.description.abstractTaking advantage of an extended Lugiato-Lefever equation with third-order dispersion, we numerically show that dark cavity solitons formed in normal dispersion of microresonators are capable of emitting dispersive waves in both normal and anomalous dispersion regions with two different methods, resembling the behavior of the commonly encountered bright cavity solitons. The generated dispersive waves can be accurately predicted by the dissipative radiation theory. In addition, we demonstrate the stability enhancement of Kerr frequency combs in the normal dispersion regime in case the dispersive wave is emitted by dark solitons in the presence of third-order dispersion.en_US
dc.publisherIEEEen_US
dc.relation.haspart7740022.pdfen_US
dc.subjectmicroresonators|Dark cavity soliton|dispersive wave.en_US
dc.titleDynamics of Dispersive Wave Emission From Dark Solitons in Kerr Frequency Combsen_US
dc.typeArticleen_US
dc.journal.volume8en_US
dc.journal.issue6en_US
dc.journal.titleIEEE Photonics Journalen_US
Appears in Collections:2016

Files in This Item:
File Description SizeFormat 
7740022.pdf1.33 MBAdobe PDFThumbnail
Preview File