scispace - formally typeset
E

E. Sharkey

Researcher at Stony Brook University

Publications -  45
Citations -  14928

E. Sharkey is an academic researcher from Stony Brook University. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 37, co-authored 42 publications receiving 14402 citations. Previous affiliations of E. Sharkey include State University of New York System.

Papers
More filters
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.
Journal ArticleDOI

Measurements of the solar neutrino flux from Super-Kamiokande's first 300 days

Y. Fukuda, +131 more
TL;DR: The first results of the solar neutrino flux measurement from Super-Kamiokande are presented in this article, where the results are obtained from data taken between 31 May 1996, and 23 June 1997.
Journal ArticleDOI

Measurement of neutrino oscillation by the K2K experiment

M. H. Ahn, +220 more
- 12 Oct 2006 - 
TL;DR: In this article, measurements of {nu}{sub {mu}} disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment are presented.
Journal ArticleDOI

Tau neutrinos favored over sterile neutrinos in atmospheric muon neutrino oscillations.

S. Fukuda, +119 more
TL;DR: Using data recorded in 1100 live days of the Super-Kamiokande detector, three complementary data samples are used to study the difference in zenith angle distribution due to neutral currents and matter effects and find no evidence favoring sterile neutrinos, and reject the hypothesis at the 99% confidence level.
Journal ArticleDOI

Evidence for an Oscillatory Signature in Atmospheric Neutrino Oscillations

Y. Ashie, +139 more
TL;DR: A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation, which constrained nu(micro)<-->nu(tau) neutrinos oscillation parameters.