Determining the flavour content of the low-energy solar neutrino flux

André De Gouvêa*, Hitoshi Murayama

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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 languageEnglish (US)
Pages (from-to)14-21
Number of pages8
JournalJournal of High Energy Physics
Volume4
Issue number8 PART A
StatePublished - Dec 1 2000

Keywords

  • Neutrino Physics
  • Solar and Atmospheric Neutrinos

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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