Low Energy Asymptotics of the Spectral Shift Function for Pauli Operators with Nonconstant Magnetic Fields

dc.creatorRaikov, Georgi D.
dc.date.accessioned2024-01-10T13:50:06Z
dc.date.accessioned2024-05-02T18:01:24Z
dc.date.available2024-01-10T13:50:06Z
dc.date.available2024-05-02T18:01:24Z
dc.date.created2024-01-10T13:50:06Z
dc.date.issued2010
dc.identifier10.2977/PRIMS/18
dc.identifier0034-5318
dc.identifierhttps://doi.org/10.2977/PRIMS/18
dc.identifierhttps://repositorio.uc.cl/handle/11534/79505
dc.identifierWOS:000284859700005
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9269613
dc.description.abstractWe consider the 3D Pauli operator with nonconstant magnetic field B of constant direction, perturbed by a symmetric matrix-valued electric potential V whose coefficients decay fast enough at infinity We investigate the low-energy asymptotes of the corresponding spectral shift function As a corollary, for generic negative V, we obtain a generalized Levinson formula, relating the low-energy asymptotes of the eigenvalue counting function and of the scattering phase of the perturbed operator
dc.languageen
dc.publisherKYOTO UNIV
dc.rightsregistro bibliográfico
dc.subjectPauli operators
dc.subjectspectral shift function
dc.subjectlow-energy asymptotes
dc.subjectLevinson formula
dc.subjectDENSITY-OF-STATES
dc.subjectH-LAMBDA-W
dc.subjectSCHRODINGER-OPERATORS
dc.subjectEIGENVALUE BRANCHES
dc.subjectLANDAU-LEVELS
dc.subjectPOTENTIALS
dc.subjectUNIQUENESS
dc.subjectGAPS
dc.titleLow Energy Asymptotics of the Spectral Shift Function for Pauli Operators with Nonconstant Magnetic Fields
dc.typeartículo


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