Published in

arXiv, 2013

DOI: 10.48550/arxiv.1304.5356

Links

Tools

Export citation

Search in Google Scholar

First observation of PeV-energy neutrinos with IceCube.

Journal article published in 2013 by IceCube Collaboration, S. de Ridder, Mg G. Aartsen, R. Abbasi, Yasser Abdou, Markus Ackermann ORCID, J. Adams, Ja A. Aguilar, M. Ahlers, D. Altmann, J. Auffenberg, X. Bai, M. Baker, Sw W. Barwick, V. Baum and other authors.
This paper is available in a repository.
This paper is available in a repository.

Full text: Download

Question mark in circle
Preprint: policy unknown
Question mark in circle
Postprint: policy unknown
Question mark in circle
Published version: policy unknown

Abstract

We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutral-current ν(e,μ,τ) (ν̅ (e,μ,τ)) or charged-current ν(e) (ν̅ e) interactions within the IceCube detector. The events were discovered in a search for ultrahigh energy neutrinos using data corresponding to 615.9 days effective live time. The expected number of atmospheric background is 0.082±0.004(stat)₋₀.₀₅₇⁺⁰.⁰⁴¹ (syst). The probability of observing two or more candidate events under the atmospheric background-only hypothesis is 2.9×10⁻³ (2.8σ) taking into account the uncertainty on the expected number of background events. These two events could be a first indication of an astrophysical neutrino flux; the moderate significance, however, does not permit a definitive conclusion at this time. ; M. G. Aartsen . G. C. Hill . et al. (IceCube Collaboration)