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arXiv:hep-ph/9608311·v1·High Energy Physics — Phenomenology

Solar neutrinos: Near-far asymmetry and just-so oscillations

B. Faid (Algiers U.)🇩🇿 · G.L. Fogli (Bari U. & INFN, Bari)🇮🇹 · E. Lisi (Princeton, Inst. Advanced Study & Bari U. & INFN, Bari)🇺🇸 · D. Montanino (Bari U. & INFN, Bari)🇮🇹

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Abstract

We propose to study possible signals of just-so oscillations in new-generation solar neutrino experiments by separating the events detected when the earth is nearest to the sun (perihelion ~3~months) from those detected when the earth is farthest from the sun (aphelion ~3~months). We introduce a solar model independent near-far asymmetry, which is non-zero if just-so oscillations occur. We apply our calculations to the kinetic energy spectra of electrons induced by B solar neutrino interactions in the SuperKamiokande and Sudbury Neutrino Observatory experiments. We show that the sensitivity to the neutrino oscillation parameters can be increased by probing the near-far asymmetry in selected parts of the electron energy spectra.

Comments: RevTeX, 17 pages + 11 figures. Requires epsfig.sty

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