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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.identifier16837172
dc.identifierdb2cdac8-6066-438d-98ed-d0dc4d439afc
dc.identifier84860309347
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.otherArXiv: http://arxiv.org/abs/1201.3916v2
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.format.extent548676
dc.language.isoeng
dc.relation.ispartofPhysical Review. B, Condensed matter and materials physicsen
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.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1103/PhysRevB.85.165111
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H049584/1en
dc.identifier.grantnumberEP/I031014/1en


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