activity
19952025
most citedIndication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam

1.4k citations · 14.3k across the 154 of their papers we have counts for

collaborators
Showing 2013 · hep-exShow all

6 papers · 2 filters

hep-ex2013★ 98 cited

First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation

A. Renshaw, K. Abe, Y. Hayato +112

We report an indication that the elastic scattering rate of solar B neutrinos with electrons in the Super-Kamiokande detector is larger when the neutrinos pass through the Eart…

hep-ex2013★ 521 cited

Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

K. Abe, J. Adam, H. Aihara +336

The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28…

hep-ex2013★ 132 cited

Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV

Kamiokande Collaboration

A search for Supernova Relic Neutrinos 's is first conducted via inverse-beta-decay by tagging neutron capture on hydrogen at Super-Kamiokande-IV. The neutron tagging effi…

hep-ex2013★ 98 cited

Measurement of Neutrino Oscillation Parameters from Muon Neutrino Disappearance with an Off-axis Beam

T2K collaboration, K. Abe, N. Abgrall +335

The T2K collaboration reports a precision measurement of muon neutrino disappearance with an off-axis neutrino beam with a peak energy of 0.6 GeV. Near detector measurements are us…

hep-ex2013★ 81 cited

A Search for Nucleon Decay via and in Super-Kamiokande

Kamiokande Collaboration, K. Abe, Y. Hayato +111

We present the results of searches for nucleon decay via bound neutron to antineutrino plus pizero and proton to antineutrino plus piplus using data from a combined 172.8 kiloton-y…

hep-ex2013★ 170 cited

Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam

T2K Collaboration, K. Abe, N. Abgrall +356

The T2K collaboration: reports evidence for electron neutrino appearance at the atmospheric mass splitting, |Δm_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interaction…