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Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

M. G. Aartsen et al. (IceCube Collaboration)
Phys. Rev. Lett. 114, 171102 – Published 28 April 2015
Physics logo See Synopsis: IceCube Neutrinos Pass Flavor Test

Abstract

A diffuse flux of astrophysical neutrinos above 100 TeV has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to 35 TeV and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for showerlike events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the (fefμfτ)(111) flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sources. Limits are placed on nonstandard flavor compositions that cannot be produced by averaged neutrino oscillations but could arise in exotic physics scenarios. A maximally tracklike composition of (010) is excluded at 3.3σ, and a purely showerlike composition of (100) is excluded at 2.3σ.

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  • Received 13 February 2015

DOI:https://doi.org/10.1103/PhysRevLett.114.171102

© 2015 American Physical Society

Synopsis

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IceCube Neutrinos Pass Flavor Test

Published 28 April 2015

The highest energy neutrinos ever recorded have a flavor distribution of neutrinos that is consistent with the particles having a cosmic origin.

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See Also

What is the Flavor of the Cosmic Neutrinos Seen by IceCube?

A. Palladino, G. Pagliaroli, F. L. Villante, and F. Vissani
Phys. Rev. Lett. 114, 171101 (2015)

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Vol. 114, Iss. 17 — 1 May 2015

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