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2014

Glashow resonance as a window into cosmic neutrino sources

Barger, V., Fu, Lingjun, Learned, J. G. et al.

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The Glashow resonance at E_\nu=6.3 PeV is a measure of the \bar\nu_e content of the astrophysical neutrino flux.

The fractional \bar\nu_e content depends on the neutrino production model at the cosmic neutrino source, and the environment at the source.
Thus, the strength of the Glashow resonance event rate is a potential window into astrophysical sources.
We quantify the "Glashow resonometer" and comment on the significance that no Glashow events are observed in the IceCube three-year data.

Glashow resonance as a window into cosmic neutrino sources · Around

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L. A. Anchordoqui, V. Barger, H. Goldberg, J. G. Learned, D. Marfatia, S. Pakvasa, T. C. Paul and T. J. Weiler, arXiv:1404.0622 [hep-ph]; J. G. Learned and T. J. Weiler, arXiv:1407.0739 [astro-ph.HE]

Cited in the paper.

L. A. Anchordoqui, T. C. Paul, L. H. M. da Silva, D. F. Torres and B. J. Vlcek, Phys. Rev. D 89

2014

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