Abstract
We study the sensitivity of the HELLAZ and Borexino solar neutrino experiments on discriminating the neutrino species νe, ν̄e, νμ,τ, ν̄μ,τ, and νs using the difference in the recoil electron kinetic energy spectra in elastic neutrino-electron scattering. We find that one can observe a non-vanishing νμ,τ component in the solar neutrino flux, especially when the νe survival probability is low. Also, if the data turn out to be consistent with νe ↔ νμ,τ oscillations, a ν̄e component can be excluded effectively.
Original language | English (US) |
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Pages (from-to) | 14-21 |
Number of pages | 8 |
Journal | Journal of High Energy Physics |
Volume | 4 |
Issue number | 8 PART A |
State | Published - Dec 1 2000 |
Keywords
- Neutrino Physics
- Solar and Atmospheric Neutrinos
ASJC Scopus subject areas
- Nuclear and High Energy Physics