Home > Research > Publications & Outputs > Evidence of electron neutrino appearance in a m...

Associated organisational unit

Electronic data

  • PhysRevD.88.032002

    Rights statement: © 2013 American Physical Society

    Final published version, 7 MB, PDF-document

    21/10/13

Links

Text available via DOI:

View graph of relations

Evidence of electron neutrino appearance in a muon neutrino beam

Research output: Contribution to journalJournal article

Published
Article number032002
<mark>Journal publication date</mark>5/08/2013
<mark>Journal</mark>Physical Review D
Issue number3
Volume88
Number of pages41
<mark>State</mark>Published
<mark>Original language</mark>English

Abstract

The T2K collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, |\Delta m_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy of 0.6 GeV at the Super-Kamiokande (SK) detector 295 km from the beam's origin. Signal and background predictions are constrained by data from near detectors located 280 m from the neutrino production target. We observe 11 electron neutrino candidate events at the SK detector when a background of 3.3\pm0.4(syst.) events is expected. The background-only hypothesis is rejected with a p-value of 0.0009 (3.1\sigma), and a fit assuming \nu_{\mu}->\nu_e oscillations with sin^2(2\theta_{23})=1, \delta_{CP}=0 and |\Delta m_{32}^2|=2.4x10^{-3} eV^2 yields sin^2(2\theta_{13})=0.088^{+0.049}_{-0.039}(stat.+syst.).

Bibliographic note

41 pages, 41 figures
© 2013 American Physical Society