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2016

Solar Neutrino Measurements in Super-Kamiokande-IV

Kamiokande Collaboration, Abe, K., Haga, Y. et al.

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Upgraded electronics, improved water system dynamics, better calibration and analysis techniques allowed Super-Kamiokande-IV to clearly observe very low-energy 8B solar neutrino interactions, with recoil electron kinetic energies as low as 3.49 MeV.

Super-Kamiokande-IV data-taking began in September of 2008; this paper includes data until February 2014, a total livetime of 1664 days.
The measured solar neutrino flux is (2.308+-0.020(stat.) + 0.039-0.040(syst.)) x 106/(cm2sec) assuming no oscillations.
The observed recoil electron energy spectrum is consistent with no distortions due to neutrino oscillations.

Solar Neutrino Measurements in Super-Kamiokande-IV · Around

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