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dc.contributor.authorKeeling, Jonathan Mark James
dc.contributor.authorKirton, Peter George
dc.date.accessioned2018-05-09T11:30:06Z
dc.date.available2018-05-09T11:30:06Z
dc.date.issued2018-05-29
dc.identifier.citationKeeling , J M J & Kirton , P G 2018 , ' Orientational alignment in cavity quantum electrodynamics ' , Physical Review. A, Atomic, molecular, and optical physics , vol. 97 , no. 5 , 053836 . https://doi.org/10.1103/PhysRevA.97.053836en
dc.identifier.issn1050-2947
dc.identifier.otherPURE: 253035252
dc.identifier.otherPURE UUID: 1fcfe3ad-a640-4218-b716-0b5a6daa325f
dc.identifier.otherScopus: 85047756710
dc.identifier.otherORCID: /0000-0002-4283-552X/work/45366211
dc.identifier.otherWOS: 000433286200017
dc.identifier.urihttps://hdl.handle.net/10023/13316
dc.description.abstractWe consider the orientational alignment of dipoles due to strong matter-light coupling, for a non-vanishing density of excitations. We compare various approaches to this problem in the limit of large numbers of emitters, and show that direct Monte Carlo integration, mean-field theory, and large deviation methods match exactly in this limit. All three results show that orientational alignment develops in the presence of a macroscopically occupied polariton mode, and that the dipoles asymptotically approach perfect alignment in the limit of high density or low temperature.
dc.language.isoeng
dc.relation.ispartofPhysical Review. A, Atomic, molecular, and optical physicsen
dc.rights© 2018, American Physical Society. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1103/PhysRevA.97.053836en
dc.subjectQC Physicsen
dc.subjectTK Electrical engineering. Electronics Nuclear engineeringen
dc.subjectDASen
dc.subject.lccQCen
dc.subject.lccTKen
dc.titleOrientational alignment in cavity quantum electrodynamicsen
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. Condensed Matter Physicsen
dc.identifier.doihttps://doi.org/10.1103/PhysRevA.97.053836
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/1803.05877en
dc.identifier.urlhttps://journals.aps.org/pra/accepted/87078Nf2Ef319218d4e35492b8ffdebc935443b33en
dc.identifier.grantnumberEP/M025330/1en


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