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Spectral density and magnetic susceptibility for the asymmetric degenerate Anderson model

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dc.contributorVirginia Techen
dc.contributor.authorZhang, F. C.en
dc.contributor.authorLee, T. K.en
dc.contributor.departmentPhysicsen
dc.date.accessed2014-04-23en
dc.date.accessioned2014-05-07T15:37:06Zen
dc.date.available2014-05-07T15:37:06Zen
dc.date.issued1984-08en
dc.description.abstractWith the use of a new diagrammatic formulation, two coupled integral equations for the self-energy functions of the f hole and f particle in the asymmetric degenerate Anderson model are solved numerically. All the diagrams are included in the equations except the cross terms (or the vertex correction). The results for the spectral density function and the magnetic susceptibility show the scaling property described by the renormalization-group theory.en
dc.description.sponsorshipMicorelectronic Information Science Center of University of Minnesotaen
dc.identifier.citationZhang, F. C.; Lee, T. K., "Spectral density and magnetic susceptibility for the asymmetric degenerate Anderson model," Phys. Rev. B 30, 1556 DOI: http://dx.doi.org/10.1103/PhysRevB.30.1556en
dc.identifier.doihttps://doi.org/10.1103/PhysRevB.30.1556en
dc.identifier.issn0163-1829en
dc.identifier.urihttp://hdl.handle.net/10919/47889en
dc.identifier.urlhttp://journals.aps.org/prb/abstract/10.1103/PhysRevB.30.1556en
dc.language.isoen_USen
dc.publisherAmerican Physical Societyen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectphysics, condensed matteren
dc.titleSpectral density and magnetic susceptibility for the asymmetric degenerate Anderson modelen
dc.title.serialPhysical Review Ben
dc.typeArticle - Refereeden

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