English

Atmospheric Neutrino Status

High Energy Physics - Experiment 2016-05-03 v1 Instrumentation and Detectors

Abstract

This conference proceeding discusses new results arising from atmospheric neutrino detection in the Super-Kamiokande and IceCube experiments. Super-Kamiokande has measured atmospheric neutrinos in the energy range of 100 MeV-10 TeV and uses this data set to conclusively measure the east-west effect to 8.0 (6.0) σ\sigma for electron (muon) neutrinos. IceCube is ideal for measuring high energy atmospheric neutrinos and has explored how different production channels for atmospheric neutrinos contribute to the total overall observed flux. The measurement is consistent with the conventional spectrum, produced by the decay of pions and kaon, while the contribution from the prompt channel (due to charm decay) is consistent with zero.

Keywords

Cite

@article{arxiv.1605.00612,
  title  = {Atmospheric Neutrino Status},
  author = {E. O'Sullivan},
  journal= {arXiv preprint arXiv:1605.00612},
  year   = {2016}
}

Comments

Talk presented at NuPhys2015 (London, 16-18 December 2015). 8 pages, PDFLaTeX, 5 PDF figures

R2 v1 2026-06-22T13:47:01.301Z