Solar neutrino oscillation phenomenology

Goswami, Srubabati (2004) Solar neutrino oscillation phenomenology Pramana - Journal of Physics, 62 (2). pp. 241-253. ISSN 0304-4289

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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.

Item Type:Article
Source:Copyright of this article belongs to Indian Academy of Sciences.
Keywords:Solar Neutrino; Reactor Neutrino
ID Code:108828
Deposited On:01 Feb 2018 04:48
Last Modified:01 Feb 2018 04:48

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