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Level density of spin chains of Haldane-Shastry type

dc.contributor.authorEnciso, Alberto
dc.contributor.authorFinkel Morgenstern, Federico
dc.contributor.authorGonzález López, Artemio
dc.date.accessioned2023-06-20T03:55:22Z
dc.date.available2023-06-20T03:55:22Z
dc.date.issued2010-11-15
dc.description©2010 The American Physical Society. This work was supported in part by the MICINN and the UCM–Banco Santander under Grants No. FIS2008-00209 and No. GR58/08-910556. The authors would also like to thank Gabriel Álvarez for some useful discussions, and the anonymous referees of a previous version of this paper for their helpful suggestions.
dc.description.abstractWe provide a rigorous proof of the fact that the level density of all known su (m) spin chains of Haldane-Shastry type associated with the A(N-1) root system approaches a Gaussian distribution as the number of spins N tends to infinity. Our approach is based on the study of the large-N limit of the characteristic function of the level density, using the description of the spectrum in terms of motifs and the asymptotic behavior of the transfer matrix.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMICINN
dc.description.sponsorshipUCM–Banco Santander
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31279
dc.identifier.doi10.1103/PhysRevE.82.051117
dc.identifier.issn1539-3755
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevE.82.051117
dc.identifier.relatedurlhttp://journals.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44673
dc.issue.number5
dc.journal.titlePhysical review E
dc.language.isoeng
dc.page.initialPart 1
dc.publisherAmerican Physical Society
dc.relation.projectIDFIS2008-00209
dc.relation.projectIDGR58/08-910556
dc.rights.accessRightsopen access
dc.subject.cdu51-73
dc.subject.ucmFísica-Modelos matemáticos
dc.subject.ucmFísica matemática
dc.titleLevel density of spin chains of Haldane-Shastry type
dc.typejournal article
dc.volume.number82
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relation.isAuthorOfPublication.latestForDiscovery207092a4-0443-4336-a037-15936f8acc25

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