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

Table 5

Muon 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	1.0816	0.0476	0.0832	0.0101
100 PeV–1 EeV	0.4685	0.0015	0.0267	0.0185