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dc.date.accessioned 2019-10-09T18:04:07Z
dc.date.available 2019-10-09T18:04:07Z
dc.date.issued 2007
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82981
dc.description.abstract Pion-photoproduction amplitude is calculated within a consistent isobar model already used to fix the Δ+ + (1232   MeV) parameters in pion-nucleon scattering and bremsstrahlung. This amplitude is expressed in terms of (physical) on-shell quantities and off-shell contributions coming from final state interactions. These latter are isolated in principal value integrals on the non-polar part of the pion-nucleon K-matrix, being the main effect of them to dress the bare form factors present in the γ N → Δ vertex. First, we hide the dressing into effective form factors getting at kγ2 = 0, GM = 2.97 ± 0.08 and GE = 0.055 ± 0.010 in full consistence with recent chiral effective field theory calculations. Then, different models to regularize the mentioned integrals are analyzed. We choose those better describing the non-resonant multipoles, in order to get model independent results for the resonant ones. Finally, we try to predict the bare form factors getting GM0 = 1.69 ± 0.02 and GE0 = 0.028 ± 0.008, which are consistent with recent lattice quark calculations and other more sophisticated dynamical models. en
dc.format.extent 253-261 es
dc.language en es
dc.subject Pion-photoproduction es
dc.subject isobar model es
dc.title A consistent dynamical model for pion-photoproduction en
dc.type Articulo es
sedici.identifier.other doi:10.1016/j.physletb.2007.02.006 es
sedici.identifier.other eid:2-s2.0-33947306740 es
sedici.identifier.issn 0370-2693 es
sedici.creator.person Mariano, Alejandro Edgardo es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 3.0 Unported (CC BY 3.0)
sedici.rights.uri http://creativecommons.org/licenses/by/3.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physics Letters B es
sedici.relation.journalVolumeAndIssue vol. 647, no. 4 es


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Creative Commons Attribution 3.0 Unported (CC BY 3.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 3.0 Unported (CC BY 3.0)