完整後設資料紀錄
DC 欄位語言
dc.contributor.authorVasala, Samien_US
dc.contributor.authorSaadaoui, Hassanen_US
dc.contributor.authorMorenzoni, Elvezioen_US
dc.contributor.authorChmaissem, Omaren_US
dc.contributor.authorChan, Ting-Shanen_US
dc.contributor.authorChen, Jin-Mingen_US
dc.contributor.authorHsu, Ying-Yaen_US
dc.contributor.authorYamauchi, Hisaoen_US
dc.contributor.authorKarppinen, Maariten_US
dc.date.accessioned2014-12-08T15:35:50Z-
dc.date.available2014-12-08T15:35:50Z-
dc.date.issued2014-04-21en_US
dc.identifier.issn1098-0121en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevB.89.134419en_US
dc.identifier.urihttp://hdl.handle.net/11536/24230-
dc.description.abstractIn this work we examine the low-temperature magnetic properties of the two double-perovskite compounds Sr2CuWO6 and Sr2CuMoO6 using magnetic susceptibility, muon spin rotation and relaxation, and neutron powder diffraction measurements. Additionally, the most relevant spin exchange interaction constants are derived from ab initio electronic structure calculations, aided by x-ray absorption spectroscopy. The compounds exhibit quasi-two-dimensional magnetic properties, with broad maxima at T-max = 83 and 95 K for Sr2CuWO6 and Sr2CuMoO6, respectively. However, three-dimensional long-range order takes place below T-N = 24(1) and 28(2) K for Sr2CuWO6 and Sr2CuMoO6, respectively. Our results show that the low-dimensional magnetic correlations are mainly due to the significant next-nearest-neighbor interactions in the ab plane of the double-perovskite structure, whereas three-dimensional long-range magnetic order is caused by weaker next-nearest-neighbor interactions along the c axis. Next-nearest-neighbor interactions are also slightly frustrated by weaker nearest-neighbor interactions within the ab plane. Based on these results we predict the low-temperature magnetic structure in these compounds to be type-II antiferromagnetic order of the double-perovskite lattice.en_US
dc.language.isoen_USen_US
dc.titleCharacterization of magnetic properties of Sr2CuWO6 and Sr2CuMoO6en_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevB.89.134419en_US
dc.identifier.journalPHYSICAL REVIEW Ben_US
dc.citation.volume89en_US
dc.citation.issue13en_US
dc.citation.spageen_US
dc.citation.epageen_US
dc.contributor.department加速器光源科技與應用學位學程zh_TW
dc.contributor.departmentMaster and Ph.D. Program for Science and Technology of Accelrrator Light Sourceen_US
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