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The neutrino charge radius as a physical observable

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The neutrino charge radius as a physical observable

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dc.contributor.author Bernabeu Alberola, José
dc.contributor.author Papavassiliou, Joannis
dc.contributor.author Vidal Perona, Jorge
dc.date.accessioned 2014-01-16T12:22:02Z
dc.date.available 2014-01-16T12:22:02Z
dc.date.issued 2004
dc.identifier.citation Bernabeu Alberola, José; Papavassiliou, Joannis; Vidal Perona, Jorge (2004) The neutrino charge radius as a physical observable Nuclear Physics B 680 1-3 450 478
dc.identifier.uri http://hdl.handle.net/10550/32344
dc.description.abstract We present a method which allows, at least in principle, the direct extraction of the gauge-invariant and process-independent neutrino charge radius (NCR) from experiments. Under special kinematic conditions, the judicious combination of neutrino and anti-neutrino forward differential cross-sections allows the exclusion of all target-dependent contributions, such as gauge-independent box-graphs, not related to the NCR. We show that the remaining contributions contain universal, renormalization group invariant combinations, such as the electroweak effective charge and the running mixing angle, which must be also separated out. By considering the appropriate number of independent experiments we show that one may systematically eliminate these universal terms, and finally express the NCR entirely in terms of physical cross-sections. Even though the kinematic conditions and the required precision may render the proposed experiments unfeasible, at the conceptual level the analysis presented here allows for the promotion of the NCR into a genuine physical observable.
dc.relation.ispartof Nuclear Physics B, 2004, vol. 680, num. 1-3, p. 450-478
dc.subject Astrofísica
dc.title The neutrino charge radius as a physical observable
dc.type journal article es_ES
dc.date.updated 2014-01-16T12:22:02Z
dc.identifier.doi 10.1016/j.nuclphysb.2003.12.025
dc.identifier.idgrec 013973
dc.rights.accessRights open access es_ES
dc.identifier.url 10.1016/j.nuclphysb.2003.12.025

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