Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2001-11-29
Phys.Lett. B527 (2002) 199-205
Physics
High Energy Physics
High Energy Physics - Phenomenology
6 pages, 2 figures. Typos corrected and reference added. Final version to appear in PLB
Scientific paper
10.1016/S0370-2693(02)01178-4
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 %.
Gonzalez-Garcia M. C.
Pena-Garay Carlos
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