Elsevier

Physics Letters B

Volume 299, Issues 1–2, 21 January 1993, Pages 94-98
Physics Letters B

Solar neutrino data, solar model uncertainties and neutrino oscillations

https://doi.org/10.1016/0370-2693(93)90888-OGet rights and content

Abstract

We incorporate all existing solar neutrino flux measurements and take solar model flux uncertainties into account in deriving global fits to parameter space for the MSW and vacuum solutions of the solar neutrino problem.

References (22)

  • P Anselmann

    Phys. Lett. B

    (1992)
    P Anselmann

    Phys. Lett. B

    (1992)
  • M White et al.

    Phys. Rev. Lett.

    (1992)
  • K Hirata

    Phys. Rev. Lett.

    (1990)
  • J.N Bahcall

    Neutrino astrophysics

    (1989)
  • P.I Krastev et al.

    Phys. Lett. B

    (1988)
  • G.T Ewan

    Sudbury neutrino observatory proposal

    report SNO-87-12

    (October 1987)
  • R Davis
  • A.I Abazov

    Phys. Rev. Lett.

    (1991)
  • E Gates et al.

    Phys. Rev. D

    (1992)
  • S.P Mikheyev et al.

    Sov. J. Nucl. Phys.

    (1985)
    L Wolfenstein

    Phys. Rev. D

    (1987)
  • S.L Glashow et al.

    Phys. Lett. B

    (1987)
  • Cited by (38)

    • Neutrino masses and mixing

      1999, Nuclear Physics B - Proceedings Supplements
    • Anomalous diffusion modifies solar neutrino fluxes

      1998, Physica A: Statistical Mechanics and its Applications
    • A neutrino apparatus with improved capabilities for a short baseline ν<inf>μ</inf>(ν<inf>e</inf>) ↔ ν<inf>τ</inf> search

      1996, Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
    • Results from SAGE

      1996, Nuclear Physics B - Proceedings Supplements
    View all citing articles on Scopus
    1

    Also at Department of Astronomy, Yale University, New Haven,USA.

    2

    Research supported in part by the DOE, the NSF and the TNRLC.

    4

    Supported in part by the DOE.

    View full text