• Solar neutrino oscillation phenomenology

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    • Keywords


      Solar neutrino; reactor neutrino

    • Abstract


      This article summarises the status of the solar neutrino oscillation phenomenology at the end of 2002 in the light of the SNO and KamLAND results. We first present the allowed areas obtained from global solar analysis and demonstrate the preference of the solar data towards the large-mixing-angle (LMA) MSW solution. A clear confirmation in favour of the LMA solution comes from the KamLAND reactor neutrino data. The KamLAND spectral data in conjunction with the global solar data further narrows down the allowed LMA region and splits it into two allowed zones a low Δm2 region (low-LMA) and high Δm2 region (high-LMA). We demonstrate through a projected analysis that with an exposure of 3 kton-year (kTy) KamLAND can remove this ambiguity.

    • Author Affiliations


      Srubabati Goswami1

      1. Harish-Chandra Research Institute, Chhatnag Road, Jhusi, Allahabad - 211 019, India
    • Dates

  • Pramana – Journal of Physics | News

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