arXiv:hep-ph/0111432·v2·High Energy Physics — Phenomenology
On the Effect of theta_{13} on the Determination of Solar Oscillation Parameters at KamLAND
M.C.Gonzalez-Garcia🇨🇭 · C. Peña-Garay🇪🇸
Abstract
If the solution to the solar neutrino puzzle falls in the LMA region, KamLAND should be able to measure with good precision the corresponding oscillation parameters after a few years of data taking. Assuming a positive signal, we study their expected sensitivity to the solar parameters (theta_{12},Delta m^2_{21}) when considered in the framework of three-neutrino mixing after taking into account our ignorance on the mixing angle theta_{13}. We find a simple ``scaling'' dependence of the reconstructed theta_{12} range with the value of theta_{13} while the Delta m^2_{12} range is practically unaffected. Our results show that the net effect is approximately equivalent to an uncertainty on the overall neutrino flux normalization of up to sim 10 %.
Comments: 6 pages, 2 figures. Typos corrected and reference added. Final version to appear in PLB