Three-neutrino mixing after the first results from K2K and KamLAND
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Three-neutrino mixing after the first results from K2K and KamLAND

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Three-neutrino mixing after the first results from K2K and KamLAND

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González García, Mª Concepción; Peña Garay, Carlos
Aquest document és un/a article, creat/da en: 2003
We analyze the impact of the data on long-baseline nu(mu) disappearance from the K2K experiment and reactor (nu) over bar (e) disappearance from the KamLAND experiment on the determination of the leptonic three-generation mixing parameters. Performing an up-to-date global analysis of solar, atmospheric, reactor, and long-baseline neutrino data in the context of three-neutrino oscillations, we determine the presently allowed ranges of masses and mixing and we consistently derive the allowed magnitude of the elements of the leptonic mixing matrix. We also quantify the maximum allowed contribution of Deltam(21)(2) oscillations to CP-odd and CP-even observables at future long-baseline experiments.

    González García, Mª Concepción Peña Garay, Carlos 2003 Three-neutrino mixing after the first results from K2K and KamLAND Physical Review D 68 9 093003
http://dx.doi.org/10.1103/PhysRevD.68.093003
distribuït sota llicència Creative Commons de Reconeixement-NoComercial 3.0 No adaptada

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