Capability of the HAWC Gamma-Ray Observatory for the Indirect Detection of Ultrahigh-Energy Neutrinos

Table 4

Tau charged lepton fluxes () produced by neutrino-nucleon interactions in “standard rock” with average width . The astrophysical flux is obtained from the extrapolation of the measured neutrino flux by IceCube. See the text for details.

Neutrino energy []
	Astrophysical	Model A	Model B	Model C
10 PeV–100 PeV	10.7471	0.4732	0.8269	0.1008
100 PeV–10 EeV	11.0342	0.0233	0.4251	0.3690