dc.creatorde Siervo, A
dc.creatorLanders, R
dc.creatorKleiman, GG
dc.date2001
dc.dateFEB 12
dc.date2014-11-16T10:44:49Z
dc.date2015-11-26T17:24:31Z
dc.date2014-11-16T10:44:49Z
dc.date2015-11-26T17:24:31Z
dc.date.accessioned2018-03-29T00:11:49Z
dc.date.available2018-03-29T00:11:49Z
dc.identifierPhysical Review Letters. American Physical Soc, v. 86, n. 7, n. 1362, n. 1365, 2001.
dc.identifier0031-9007
dc.identifierWOS:000166907600055
dc.identifier10.1103/PhysRevLett.86.1362
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/56341
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/56341
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/56341
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1284099
dc.descriptionMVV spectra of ph, Pd, and Ag were measured with and without ionization of their L-3 levels. Extra (MMMVV) structure corresponds to the M45M45 --> M45VV transition following the L3M45M45 transition. We interpret the MMMVV structure for Pd as quasiatomic in nature from its similarity to the corresponding Ag spectral shape and from its agreement with atomic calculations. The Pd quasiatomic MMMVV spectrum arises from a two final-state hole bound state in the Pd d band filled by screening of the core holes. These findings represent the first unambiguous observation of the influence of complete screening on spectral features.
dc.description86
dc.description7
dc.description1362
dc.description1365
dc.languageen
dc.publisherAmerican Physical Soc
dc.publisherCollege Pk
dc.publisherEUA
dc.relationPhysical Review Letters
dc.relationPhys. Rev. Lett.
dc.rightsaberto
dc.sourceWeb of Science
dc.subjectHartree-fock Calculation
dc.subjectInner-shell Ionization
dc.subjectBinding-energy Shifts
dc.subjectMetallic Elements
dc.subjectVacancy Cascades
dc.subject4d Metals
dc.subjectSpectra
dc.subjectSatellite
dc.subjectTransitions
dc.subjectValence
dc.titleComplete screening and quasiatomic MVV auger line shapes due to double core ionization
dc.typeArtículos de revistas


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