Galactic High-Energy Cosmic-Ray Tau Neutrino Flux

Details Galactic High-Energy Cosmic-Ray Tau Neutrino Flux Galactic High-Energy Cosmic-Ray Tau Neutrino Flux

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002asph.conf..117a&link_type=abstract

ASTROPARTICLE PHYSICS . Proceedings of the First NCTS Workshop . Held 6-8 December 2001 in Kenting, Taiwan . Edited by Husain At

Physics

Scientific paper

In this talk, we summarize a recent calculation on the high-energy tau neutrino flux (103 ≥ E ≥ 1011 GeV) originating from the interactions of high-energy cosmic-rays with the matter present in our galaxy. The main source of this flux is the production and decay of Ds for E ≤ 109 GeV. For 109 ≤ E/GeV ≤ 1011, the tau neutrino flux from other heavier quark decays as well as from direct production is comparable to that from Ds.

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