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dc.contributor.authorFellows, J. M.
dc.contributor.authorCarr, S. T.
dc.contributor.authorHooley, C. A.
dc.contributor.authorSchmalian, J.
dc.date.accessioned2014-06-04T16:01:02Z
dc.date.available2014-06-04T16:01:02Z
dc.date.issued2012-10-10
dc.identifier.citationFellows , J M , Carr , S T , Hooley , C A & Schmalian , J 2012 , ' Unbinding of giant vortices in states of competing order ' , Physical Review Letters , vol. 109 , no. 15 , 155703 . https://doi.org/10.1103/PhysRevLett.109.155703en
dc.identifier.issn0031-9007
dc.identifier.otherPURE: 38400688
dc.identifier.otherPURE UUID: 08e26e01-451b-4194-b3a8-f4e6f8fd9448
dc.identifier.otherWOS: 000309658300017
dc.identifier.otherScopus: 84867322152
dc.identifier.otherORCID: /0000-0002-9976-2405/work/27144568
dc.identifier.urihttps://hdl.handle.net/10023/4855
dc.descriptionFunding: EPSRC (UK) via Grants No. EP/I031014/1 and No. EP/H049584/1.en
dc.description.abstractWe consider a two-dimensional system with two order parameters, one with O(2) symmetry and one with O(M), near a point in parameter space where they couple to become a single O(2+M) order. While the O(2) sector supports vortex excitations, these vortices must somehow disappear as the high symmetry point is approached. We develop a variational argument which shows that the size of the vortex cores diverges as 1/root Delta and the Berezinskii-Kosterlitz-Thouless transition temperature of the O(2) order vanishes as 1/1n(1/Delta), where Delta denotes the distance from the high-symmetry point. Our physical picture is confirmed by a renormalization group analysis which gives further logarithmic corrections, and demonstrates full symmetry restoration within the cores.
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofPhysical Review Lettersen
dc.rights© 2012 American Physical Societyen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleUnbinding of giant vortices in states of competing orderen
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.contributor.sponsorEPSRCen
dc.description.versionPublisher PDFen
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/PhysRevLett.109.155703
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H049584/1en
dc.identifier.grantnumberEP/I031014/1en


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