Glashow resonance as a window into cosmic neutrino sources
Barger, V. · Fu, Lingjun · Learned, J. G. · Marfatia, D. · Pakvasa, S. · Weiler, T. J.
الأصل · EN
The Glashow resonance at Eν=6.3 PeV is a measure of the νₑ content of the astrophysical neutrino flux. The fractional νₑ 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.
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