Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5653
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dc.contributor.authorMandal, Prithwijiten_US
dc.contributor.authorPatel, Ranjan Kumaren_US
dc.contributor.authorROUT, DIBYATAen_US
dc.contributor.authorBanerjee, Rajdeepen_US
dc.contributor.authorBAG, RABINDRANATHen_US
dc.contributor.authorKARMAKAR, KOUSHIKen_US
dc.contributor.authorNarayan, Awadheshen_US
dc.contributor.authorFreeland, John W.en_US
dc.contributor.authorSINGH, SURJEETen_US
dc.contributor.authorMiddey, Srimantaen_US
dc.date.accessioned2021-02-23T08:40:44Z
dc.date.available2021-02-23T08:40:44Z
dc.date.issued2021-02en_US
dc.identifier.citationPhysical Review B, 103(6), L060504.en_US
dc.identifier.issn2469-9969en_US
dc.identifier.issn2469-9950en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5653
dc.identifier.urihttps://doi.org/10.1103/PhysRevB.103.L060504en_US
dc.description.abstractFinding large orbital polarization in Ni-based oxides has become a topic of paramount interest in recent years due to the prospect of finding superconductivity. In this work, we investigate the electronic structure of single-crystalline samples of Sr2CuO3 and Ni-doped Sr 2 CuO3 containing Cu/NiO4 square planar units. Our polarization-dependent x-ray absorption spectroscopy experiments reveal extremely large orbital polarization (∼63%)for Ni2+. Cluster calculations and ab initio calculations find that the giant orbital polarization arises due to the low-spin (S=0) configuration with two holes in the Ni 3dx2−y2 orbital, contrary to the expected high-spin ( S=1) state from Hund's first rule.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectImpurities in superconductorsen_US
dc.subjectMagnetic susceptibilityen_US
dc.subjectSuperconducting phase transitionen_US
dc.subject2021-FEB-WEEK3en_US
dc.subjectTOC-FEB-2021en_US
dc.subject2021en_US
dc.titleGiant orbital polarization of Ni 2+ in a square planar environmenten_US
dc.typeLetteren_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review B en_US
dc.publication.originofpublisherForeignen_US
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