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dc.contributor.authorBerger, Raphael Johann Friedrich
dc.contributor.authorRepisky, Michal
dc.contributor.authorKomorovsky, Stanislav
dc.date.accessioned2016-03-21T10:40:43Z
dc.date.available2016-03-21T10:40:43Z
dc.date.issued2015-07-23
dc.description.abstractMagnetically induced probability currents in molecules are studied in relativistic theory. Spin–orbit coupling (SOC) enhances the curvature and gives rise to a previously unobserved current cusp in AuH or small bulge-like distortions in HgH2 at the proton positions. The origin of this curvature is magnetically induced spin-density arising from SOC in the relativistic description.en_US
dc.descriptionPublished version. Source at <a href=http://doi.org/10.1039/c5cc05732a>http://doi.org/10.1039/c5cc05732a</a>.en_US
dc.identifier.citationChemical Communications 2015, 51(73):13961-13963en_US
dc.identifier.cristinIDFRIDAID 1286476
dc.identifier.doi10.1039/c5cc05732a
dc.identifier.issn1364-548X
dc.identifier.urihttps://hdl.handle.net/10037/9048
dc.identifier.urnURN:NBN:no-uit_munin_8611
dc.language.isoengen_US
dc.publisherRoyal Society of Chemistryen_US
dc.relation.projectIDNorges forskningsråd: 179568en_US
dc.rights.accessRightsopenAccess
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Kjemi: 440en_US
dc.subjectVDP::Mathematics and natural science: 400::Chemistry: 440en_US
dc.titleHow does relativity affect magnetically induced currents?en_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US
dc.typePeer revieweden_US


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