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dc.contributor.authorChen, J. M.en_US
dc.contributor.authorHaw, S. C.en_US
dc.contributor.authorLee, J. M.en_US
dc.contributor.authorChou, T. L.en_US
dc.contributor.authorChen, S. A.en_US
dc.contributor.authorLu, K. T.en_US
dc.contributor.authorLiang, Y. C.en_US
dc.contributor.authorLee, Y. C.en_US
dc.contributor.authorHiraoka, N.en_US
dc.contributor.authorIshii, H.en_US
dc.contributor.authorTsuei, K. D.en_US
dc.contributor.authorHuang, Eugeneen_US
dc.contributor.authorYang, T. J.en_US
dc.date.accessioned2019-04-03T06:35:37Z-
dc.date.available2019-04-03T06:35:37Z-
dc.date.issued2011-09-09en_US
dc.identifier.issn1098-0121en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevB.84.125117en_US
dc.identifier.urihttp://hdl.handle.net/11536/150367-
dc.description.abstractPressure dependence of electronic structures and spin states of iron-chalcogenide Fe1.01Se superconductors up to similar to 66 GPa has been investigated with x-ray emission spectra and x-ray absorption spectra with partial-fluorescence yield. The intensity of the pre-edge peak at energy of similar to 7112.7 eV of the Fe K-edge x-ray absorption spectrum of Fe1.01Se decreases progressively with pressure up to similar to 10 GPa. A new prepeak at energy of similar to 7113.7 eV develops for pressure above similar to 13 GPa, indicating formation of a new phase. The experimental and the calculated Fe K-edge absorption spectra of Fe1.01Se using the FDMNES code agree satisfactorily. The larger compression accompanied by significant distortion around the Fe atoms along the c axis in Fe1.01Se upon applying pressure suppresses the Fe 3d-Se 4p and Fe 4p-Se 4d hybridization. The applied pressure suppresses the nearest-neighbor ferromagnetic superexchange interaction and enhances spin fluctuations on the Fe sites in Fe1.01Se. A discontinuous variation of the integrated absolute difference values of the K beta emission line was observed, originating from a phase transition of Fe1.01Se for a pressure >12 GPa. Fe1.01Se shows a small net magnetic moment of Fe-2 broken vertical bar at ambient pressure, probably arising from strong Fe-Fe spin fluctuations. The satellite line K beta' was reduced in intensity upon applying pressure and became absent for pressure >52 GPa, indicating a continuous reduction of the spin moment of Fe in Fe1.01Se superconductors. The experimental results provide insight into the spin state of Fe1.01Se superconductors under pressure.en_US
dc.language.isoen_USen_US
dc.titlePressure dependence of the electronic structure and spin state in Fe1.01Se superconductors probed by x-ray absorption and x-ray emission spectroscopyen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevB.84.125117en_US
dc.identifier.journalPHYSICAL REVIEW Ben_US
dc.citation.volume84en_US
dc.citation.issue12en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department電子物理學系zh_TW
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.identifier.wosnumberWOS:000294777400011en_US
dc.citation.woscount13en_US
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