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On the non-detection of Glashow resonance in IceCube

High Energy Physics - Phenomenology 2018-07-31 v2 High Energy Astrophysical Phenomena

Abstract

Electron anti-neutrinos at the Glashow resonance (GR, at Eνˉe6.3E_{\bar \nu_e} \sim 6.3 PeV) have an enhanced probability to be detected. With three neutrinos detected by IceCube in the (1-2) PeV energy range at present, one would expect that about 1 to 4 GR νˉe\bar\nu_e should have been detected. The high-energy 8.7\sim 8.7 PeV muon neutrino detected by IceCube may not be a GR event. If so, we expect to detect 50 to 70 GR νˉe\bar\nu_e, then one would have a "missing Glashow-resonance problem". This would suggest (1) that pγp\gamma interaction rather than pppp interaction is the dominant channel to produce the observed IceCube high-energy neutrinos, (2) that multi-pion pγp\gamma interactions are suppressed, and (3) that the magnetic field and photon energy density in the pγp\gamma emission region is such that significant μ+\mu^+ cooling occurs before decaying, yet π+\pi^+'s essentially do not cool before decaying.

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Cite

@article{arxiv.1612.09043,
  title  = {On the non-detection of Glashow resonance in IceCube},
  author = {Sarira Sahu and Bing Zhang},
  journal= {arXiv preprint arXiv:1612.09043},
  year   = {2018}
}

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single column, 11 pages