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dc.contributor.authorCheng, Szu-Chengen_US
dc.contributor.authorChen, Ting-Weien_US
dc.contributor.authorJheng, Shih-Daen_US
dc.contributor.authorHsieh, Wen-Fengen_US
dc.date.accessioned2016-03-28T00:04:25Z-
dc.date.available2016-03-28T00:04:25Z-
dc.date.issued2016-01-19en_US
dc.identifier.issn0038-1098en_US
dc.identifier.urihttp://dx.doi.org/10.1016/j.ssc.2015.11.022en_US
dc.identifier.urihttp://hdl.handle.net/11536/129664-
dc.description.abstractWe model the superfluid properties of a trapped exciton-polariton condensate under non-resonant excitation subjected to a rotating defect. With increasing the linear velocity of rotating defect, the density modulation can be classified into superfluid-like regime, parabolic-like regime, Cherenkov regime and over-Cherenkov regime. The threshold-like behavior of drag force and the onset of turbulent fringes can define the critical velocity for the superfluidity. Based on the perturbative drag force in the Bogoliubov-type analysis, the rigid modes with gapped excitation spectrum have higher critical velocity than that of the soft modes. (C) 2015 Elsevier Ltd. All rights reserved.en_US
dc.language.isoen_USen_US
dc.subjectCritical velocityen_US
dc.subjectDrag forceen_US
dc.subjectExciton-polariton condensateen_US
dc.subjectsuperfluiden_US
dc.titleDrag and critical velocities in a nonresonantly pumped trapped polariton condensate with a rotating defecten_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.ssc.2015.11.022en_US
dc.identifier.journalSOLID STATE COMMUNICATIONSen_US
dc.citation.volume227en_US
dc.citation.spage45en_US
dc.citation.epage50en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.department光電工程學系zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.contributor.departmentDepartment of Photonicsen_US
dc.identifier.wosnumberWOS:000368956600009en_US
dc.citation.woscount0en_US
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