Final-state interactions and superscaling in the semi-relativistic approach to quasielastic electron and neutrino scattering

dc.creatorAmaro, J. E.
dc.creatorBarbaro, M. B.
dc.creatorCaballero, J. A.
dc.creatorDonnelly, T. W.
dc.creatorUdias, J. M.
dc.date2006-12-13
dc.date.accessioned2026-07-07T11:03:26Z
dc.date.available2026-07-07T11:03:26Z
dc.descriptionThe semi-relativistic approach to electron and neutrino quasielastic scattering from nuclei is extended to include final-state interactions. Starting with the usual non-relativistic continuum shell model, the problem is relativized by using the semi-relativistic expansion of the current in powers of the initial nucleon momentum and relativistic kinematics. Two different approaches are considered for the final-state interactions: the Smith-Wambach 2p-2h damping model and the Dirac-equation-based potential extracted from a relativistic mean-field plus the Darwin factor. Using the latter the scaling properties of $(e,e')$ and $(ν_μ,μ^-)$ cross sections for intermediate momentum transfers are investigated.
dc.description36 pages, 17 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0612056
dc.identifierhttp://arxiv.org/abs/nucl-th/0612056
dc.identifierPhys.Rev.C75:034613,2007
dc.identifierdoi:10.1103/PhysRevC.75.034613
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188594
dc.subjectNuclear Theory
dc.titleFinal-state interactions and superscaling in the semi-relativistic approach to quasielastic electron and neutrino scattering
dc.typetext

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