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We re-examine the interesting possibility of utilizing the Glashow resonance (GR) channel nu_ebar + e^- to W^- to anything to discriminate between the UHE cosmic neutrinos originating from p-gamma and pp collisions in an optically thin source of cosmic rays.
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The possibility of detecting the UHE cosmic ν ¯ e \overline{\nu}_{e} flux by means of the ν ¯ e + e − → W − + γ \overline{\nu}_{e}+e^{-}\to W^{-}+\gamma channel has been discussed in: H. Athar and G.L. Lin, Astropart. Phys. 19
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M. Maltoni and W. Winter, JHEP 0807
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See, e.g., Z.Z. Xing and S. Zhou, Neutrinos in Particle Physics, Astronomy and Cosmology
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T.A. Mueller et al
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