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dc.contributor.authorKarahasanovic, Una
dc.contributor.authorKruger, Frank
dc.contributor.authorGreen, Andrew
dc.date.accessioned2014-06-05T15:31:01Z
dc.date.available2014-06-05T15:31:01Z
dc.date.issued2012-04-06
dc.identifier.citationKarahasanovic , U , Kruger , F & Green , A 2012 , ' Quantum order-by-disorder driven phase reconstruction in the vicinity of ferromagnetic quantum critical points ' , Physical Review. B, Condensed matter and materials physics , vol. 85 , no. 16 , 165111 . https://doi.org/10.1103/PhysRevB.85.165111en
dc.identifier.issn1098-0121
dc.identifier.otherPURE: 16837172
dc.identifier.otherPURE UUID: db2cdac8-6066-438d-98ed-d0dc4d439afc
dc.identifier.otherArXiv: http://arxiv.org/abs/1201.3916v2
dc.identifier.otherScopus: 84860309347
dc.identifier.urihttps://hdl.handle.net/10023/4857
dc.descriptionThis work was supported by EPSRC under Grant No. EP/I 004831/1.en
dc.description.abstractThe formation of new phases close to itinerant electron quantum critical points has been observed experimentally in many compounds. We present a unified analytical model that explains the emergence of new types of order around itinerant ferromagnetic quantum critical points. The central idea of our analysis is that certain Fermi-surface deformations associated with the onset of the competing order enhance the phase-space available for low-energy quantum fluctuations and so self-consistently lower the free energy. We demonstrate that this quantum order-by-disorder mechanism leads to instabilities towards the formation of spiral and d-wave spin nematic phases close to itinerant ferromagnetic quantum critical points in three spatial dimensions.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofPhysical Review. B, Condensed matter and materials physicsen
dc.rights© 2012 American Physical Societyen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleQuantum order-by-disorder driven phase reconstruction in the vicinity of ferromagnetic quantum critical pointsen
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.contributor.sponsorEPSRCen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1103/PhysRevB.85.165111
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H049584/1en
dc.identifier.grantnumberEP/I031014/1en


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