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Title: Solar neutrino measurements in Super-Kamiokande-IV

Journal Article · · Physical Review D
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We report that upgraded electronics, improved water system dynamics, better calibration and analysis techniques allowed Super-Kamiokande-IV to clearly observe very low-energy B 8 solar neutrino interactions, with recoil electron kinetic energies as low as ~ 3.5 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 ) - 0.040 + 0.039 ( syst ) ) × 1 0 6 / ( cm 2 sec ) assuming no oscillations. The observed recoil electron energy spectrum is consistent with no distortions due to neutrino oscillations. An extended maximum likelihood fit to the amplitude of the expected solar zenith angle variation of the neutrino-electron elastic scattering rate in SK-IV results in a day/night asymmetry of ( - 3.6 ± 1.6 ( stat ) ± 0.6 ( syst ) ) % . The SK-IV solar neutrino data determine the solar mixing angle as sin 2 θ 12 = 0.327 - 0.031 + 0.026 , all SK solar data (SK-I, SK-II, SK III and SK-IV) measures this angle to be sin 2 θ 12 = 0.334 - 0.023 + 0.027 , the determined mass-squared splitting is Δ m 21 2 = 4.8 - 0.8 + 1.5 × 10 - 5 eV 2 .

Research Organization:
Univ. of Hawaii, Honolulu, HI (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
Super-Kamiokande Collaboration
Grant/Contract Number:
SC0010504
OSTI ID:
1598644
Alternate ID(s):
OSTI ID: 1325610
Journal Information:
Physical Review D, Vol. 94, Issue 5; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 172 works
Citation information provided by
Web of Science

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Cited By (19)

Solar neutrinos as a probe of dark matter-neutrino interactions journal July 2017
Comprehensive measurement of pp-chain solar neutrinos journal October 2018
Neutrino versus antineutrino oscillation parameters at DUNE and Hyper-Kamiokande experiments journal November 2017
Sensitivity of Super-Kamiokande with Gadolinium to Low Energy Antineutrinos from Pre-supernova Emission journal November 2019
Effects of a revised 7 Be e -capture rate on solar neutrino fluxes journal March 2019
Coherent two-photon emission from hydrogen molecules excited by counter-propagating laser pulses journal January 2019
Long-Baseline Oscillation Experiments as a Tool to Probe High Energy Flavor Symmetry Models journal July 2018
Neutrino Oscillations and Non-standard Interactions journal February 2018
Pinpointing astrophysical bursts of low-energy neutrinos embedded into the noise journal August 2018
CNO neutrino Grand Prix: the race to solve the solar metallicity problem journal April 2018
Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger journal April 2018
Highlight Talk from Super-Kamiokande journal January 2019
Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s journal August 2019
Measurement of neutrino and antineutrino neutral-current quasielasticlike interactions on oxygen by detecting nuclear deexcitation gamma rays text January 2019
Constraints on neutrino lifetime from the Sudbury Neutrino Observatory text January 2019
Measurement of neutrino and antineutrino neutral-current quasielasticlike interactions on oxygen by detecting nuclear deexcitation $\gamma$ rays text January 2019
Neutrino oscillations and Non-Standard Interactions preprint January 2017
Search for Neutrinos in Super-Kamiokande associated with the GW170817 neutron-star merger text January 2018
Coherent two-photon emission from hydrogen molecules excited by counter-propagating laser pulses text January 2018

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