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zadetkov: 123
1.
  • Atmospheric neutrino oscill... Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV
    Haga, Y.; Ikeda, M.; Iyogi, K. ... Physical review. D, 04/2018, Letnik: 97, Številka: 7
    Journal Article
    Recenzirano
    Odprti dostop

    An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for Δm322, sin2θ23, ...
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2.
  • Search for neutrinos from a... Search for neutrinos from annihilation of captured low-mass dark matter particles in the sun by super-kamiokande
    Abe, K; Haga, Y; Iyogi, K ... Physical review letters, 04/2015, Letnik: 114, Številka: 14
    Journal Article
    Recenzirano
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    Super-Kamiokande (SK) can search for weakly interacting massive particles (WIMPs) by detecting neutrinos produced from WIMP annihilations occurring inside the Sun. In this analysis, we include ...
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3.
  • Sensitivity of Super-Kamiok... Sensitivity of Super-Kamiokande with Gadolinium to Low Energy Antineutrinos from Pre-supernova Emission
    Abe, K.; Hayato, Y.; Ikeda, M. ... Astrophysical journal/˜The œAstrophysical journal, 11/2019, Letnik: 885, Številka: 2
    Journal Article
    Recenzirano
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    Supernova detection is a major objective of the Super-Kamiokande (SK) experiment. In the next stage of SK (SK-Gd), gadolinium (Gd) sulfate will be added to the detector, which will improve the ...
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4.
  • First indication of terrest... First indication of terrestrial matter effects on solar neutrino oscillation
    Renshaw, A; Abe, K; Hayato, Y ... Physical review letters, 03/2014, Letnik: 112, Številka: 9
    Journal Article
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    We report an indication that the elastic scattering rate of solar B8 neutrinos with electrons in the Super-Kamiokande detector is larger when the neutrinos pass through Earth during nighttime. We ...
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5.
  • First measurement of radioa... First measurement of radioactive isotope production through cosmic-ray muon spallation in Super-Kamiokande IV
    Zhang, Y.; Abe, K.; Haga, Y. ... Physical review. D, 01/2016, Letnik: 93, Številka: 1
    Journal Article
    Recenzirano
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    Cosmic-ray-muon spallation-induced radioactive isotopes with beta decays are one of the major backgrounds for solar, reactor, and supernova relic neutrino experiments. Unlike in scintillator, ...
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6.
  • Evidence for the appearance... Evidence for the appearance of atmospheric tau neutrinos in super-Kamiokande
    Abe, K; Hayato, Y; Iida, T ... Physical review letters, 05/2013, Letnik: 110, Številka: 18
    Journal Article
    Recenzirano
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    Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscillation-generated tau ...
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7.
  • SEARCH FOR NEUTRINOS IN SUP... SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226
    Abe, K.; Haga, K.; Hayato, Y. ... Astrophysical journal. Letters, 10/2016, Letnik: 830, Številka: 1
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    ABSTRACT We report the results from a search in Super-Kamiokande for neutrino signals coincident with the first detected gravitational-wave events, GW150914 and GW151226, as well as LVT151012, using ...
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8.
  • Search for differences in o... Search for differences in oscillation parameters for atmospheric neutrinos and antineutrinos at Super-Kamiokande
    Abe, K; Iida, T; Ikeda, M ... Physical review letters, 12/2011, Letnik: 107, Številka: 24
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    We present a search for differences in the oscillations of antineutrinos and neutrinos in the Super-Kamiokande-I, -II, and -III atmospheric neutrino sample. Under a two-flavor disappearance model ...
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9.
  • Search for GUT monopoles at... Search for GUT monopoles at Super–Kamiokande
    Ueno, K.; Abe, K.; Hayato, Y. ... Astroparticle physics, August 2012, 2012-8-00, 20120801, Letnik: 36, Številka: 1
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    GUT monopoles captured by the Sun’s gravitation are expected to catalyze proton decays via the Callan–Rubakov process. In this scenario, protons, which initially decay into pions, will ultimately ...
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10.
  • Search for proton decay via... Search for proton decay via p→e+π0 and p→μ+π0 in 0.31  megaton·years exposure of the Super-Kamiokande water Cherenkov detector
    Abe, K Physical review. D, 01/2017, Letnik: 95, Številka: 1
    Journal Article
    Recenzirano

    We have searched for proton decay via p→e+π0 and p→μ+π0 using Super-Kamiokande data from April 1996 to March 2015, 0.306  megaton·years exposure in total. The atmospheric neutrino background rate in ...
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zadetkov: 123

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