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dc.contributor.authorKozik, Een_US
dc.contributor.authorBurovski, Een_US
dc.contributor.authorScarola, VWen_US
dc.contributor.authorTroyer, Men_US
dc.date.accessioned2017-02-20T19:45:12Z
dc.date.available2017-02-20T19:45:12Z
dc.date.issued2013-05-03en_US
dc.identifier.issn1098-0121en_US
dc.identifier.urihttp://hdl.handle.net/10919/75092
dc.format.extent? - ? (14) page(s)en_US
dc.languageEnglishen_US
dc.publisherAmer Physical Socen_US
dc.relation.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000318523700001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=930d57c9ac61a043676db62af60056c1en_US
dc.subjectPhysics, Condensed Matteren_US
dc.subjectPhysicsen_US
dc.subjectPHYSICS, CONDENSED MATTERen_US
dc.subjectOPTICAL LATTICEen_US
dc.subjectINFINITE DIMENSIONSen_US
dc.subjectGROUND-STATEen_US
dc.subjectSYSTEMSen_US
dc.subjectINSULATORen_US
dc.subjectPHYSICSen_US
dc.subjectATOMSen_US
dc.titleNeel temperature and thermodynamics of the half-filled three-dimensional Hubbard model by diagrammatic determinant Monte Carloen_US
dc.typeArticle - Refereed
dc.description.versionPublished (Publication status)en_US
dc.title.serialPHYSICAL REVIEW Ben_US
dc.identifier.doihttps://doi.org/10.1103/PhysRevB.87.205102
dc.identifier.volume87en_US
dc.identifier.issue20en_US
dc.identifier.orcidScarola, VW [0000-0002-8653-2723]en_US
pubs.organisational-group/Virginia Tech
pubs.organisational-group/Virginia Tech/All T&R Faculty
pubs.organisational-group/Virginia Tech/Science
pubs.organisational-group/Virginia Tech/Science/COS T&R Faculty
pubs.organisational-group/Virginia Tech/Science/Physics


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