The energy spectrum of tau leptons induced by the high energy Earth-skimming neutrinos
arXiv:astro-ph/0305507 · doi:10.1103/PhysRevD.68.063003
Abstract
We present a semi-analytic calculation of the tau-lepton flux emerging from the Earth, induced by the incident high energy neutrinos interacting inside the Earth for . We obtain results for the energy dependence of the tau-lepton flux coming from the Earth-skimming neutrinos, because of the neutrino-nucleon charged-current scattering as well as the resonant scattering. We illustrate our results for several anticipated high energy astrophysical neutrino sources such as the AGNs, the GRBs, and the GZK neutrino fluxes. The tau lepton fluxes resulting from rock-skimming and ocean-skimming neutrinos are compared. Such comparisons can render useful information for the spectral indices of incident neutrino fluxes.
23 pages, 6 figures
References in corpus (8)
- New Generation of Parton Distributions with Uncertainties from Global QCD Analysis
- Ultra-High Energy Neutrino Fluxes and Their Constraints
- Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector
- Photonuclear interaction of high energy muons and tau-leptons
- Large scale extragalactic jets powered by very-high energy gamma rays
- UHE and EHE neutrino induced taus inside the Earth
- Comparison of high-energy galactic and atmospheric tau neutrino flux
- High Energy Astrophysical Tau Neutrinos: The Expectations
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