REVIEW 1 cited by
Secondary atmospheric tau neutrino production
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
abstract
We evaluate the flux of tau neutrinos produced from the decay of pair produced taus from incident muons using a cascade equation analysis. To solve the cascade equations, our numerical result for the tau production $Z$ moment is given. Our results for the flux of tau neutrinos produced from incident muons are compared to the flux of tau neutrinos produced via oscillations and the direct prompt atmospheric tau neutrino flux. Results are given for both downward and upward going neutrinos fluxes and higher zenith angles are discussed. We conclude that the direct prompt atmospheric tau neutrino flux dominates these other atmospheric sources of tau neutrinos for neutrino energies larger than a few TeV for upward fluxes, and over a wider range of energy for downward fluxes.
Forward citations
Cited by 1 Pith paper
-
Rare processes in ultrahigh-energy tau-lepton transport
Tau leptons at EeV energies produce muon pairs and neutral pions via rare processes, with energy-loss rates only ~0.6% and ~0.2% of electron pair production, yet muon pairs may yield detectable double-track signatures.
Discussion (0). Continue with ORCID to comment.