Article - post-print
In the TeV energy region and above, the uncertainty in the level of prompt atmospheric neutrinos would limit the search for diffuse astrophysical neutrinos. We suggest that neutrino telescopes may provide an empirical determination of the flux of prompt atmospheric electron and muon neutrinos by measuring the flux of prompt down-going muons. Our suggestion is based on the consideration that prompt neutrino and prompt muon fluxes at sea level are almost identical.
This is an author-manuscript of an article accepted for publication in Physical Review D - Particles and Fields following peer review. The version of record is available online at: DOI:https://doi.org/10.1103/PhysRevD.67.017301.
Gelmini, G., P. Gondolo, and G. Varieschi, Phys. Rev. D 67, 017301 (2003). https://doi.org/10.1103/PhysRevD.67.017301