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W. Wang

Researcher at Boston University

Publications -  35
Citations -  6270

W. Wang is an academic researcher from Boston University. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 28, co-authored 34 publications receiving 5996 citations. Previous affiliations of W. Wang include University of Wisconsin-Madison.

Papers
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Journal ArticleDOI

Solar neutrino results in Super-Kamiokande-III

K. Abe, +134 more
- 24 Mar 2011 - 
TL;DR: The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results in this article, where improved detector calibrations, a full detector simulation, and improved analysis methods are estimated to be approximately 2.1%, which is about two thirds of the systematic uncertainty for the first phase.
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Evidence for Muon Neutrino Oscillation in an Accelerator-Based Experiment

E. Aliu, +159 more
TL;DR: The energy-dependent disappearance of nu(mu), which the authors presume have oscillated to nu(tau), is observed in the KEK to Kamioka (K2K) long-baseline neutrino oscillation experiment.
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Search for dark matter WIMPs using upward through-going muons in Super-Kamiokande

Shantanu Desai, +138 more
- 15 Oct 2004 - 
TL;DR: The results of indirect searches for Weakly Interacting Massive Particles (WIMPs) with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced upward through-going muons are presented in this paper.
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Atmospheric neutrino oscillation analysis with subleading effects in Super-Kamiokande I, II, and III

R. A. Wendell, +128 more
- 20 May 2010 - 
TL;DR: In this article, a search for nonzero {theta}{sub 13} and deviations of sin{sup 2{theta}}{sub 23} from 0.04(0.09) and 1.9(1.5) was conducted.
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Observation of the anisotropy of 10 TeV primary cosmic ray nuclei flux with the Super-Kamiokande-I detector

G. Guillian, +119 more
- 23 Mar 2007 - 
TL;DR: In this article, the first 2D celestial map of primary cosmic-ray flux was obtained from 2.10 10 8 8 cosmic ray muons accumulated in 1662.0 days of Super-Kamiokande, which indicated an (0:104 0:020)% excess region in the constellation of Taurus and a ( 0:094 0:014)% deficit region toward Virgo.