scispace - formally typeset
M

M. B. Smy

Researcher at University of California, Irvine

Publications -  114
Citations -  11847

M. B. Smy is an academic researcher from University of California, Irvine. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 41, co-authored 90 publications receiving 10265 citations. Previous affiliations of M. B. Smy include Institute for the Physics and Mathematics of the Universe & University of Tokyo.

Papers
More filters
Journal ArticleDOI

Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam

K. Abe, +416 more
TL;DR: The T2K experiment observes indications of ν (μ) → ν(e) appearance in data accumulated with 1.43×10(20) protons on target, and under this hypothesis, the probability to observe six or more candidate events is 7×10(-3), equivalent to 2.5σ significance.
Journal ArticleDOI

Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data

Y. Fukuda, +117 more
TL;DR: Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented and the recoil electron energy spectrum is consistent with no spectral distortion.
Journal ArticleDOI

The T2K Experiment

K. Abe, +536 more
TL;DR: The T2K experiment as discussed by the authors is a long-baseline neutrino oscillation experiment whose main goal is to measure the last unknown lepton sector mixing angle by observing its appearance in a particle beam generated by the J-PARC accelerator.
Journal ArticleDOI

The Super-Kamiokande detector

S. Fukuda, +186 more
TL;DR: Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons as discussed by the authors, which collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency.
Journal ArticleDOI

Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data

S. Fukuda, +126 more
- 18 Jul 2002 - 
TL;DR: In this paper, a number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar NE data.