Pqcd Analysis of Atmospheric Tau Neutrino

Details Pqcd Analysis of Atmospheric Tau Neutrino Pqcd Analysis of Atmospheric Tau Neutrino

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cpa..conf..190y&link_type=abstract

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS (CosPA 02). Held 31 May ?2 June 2002 in T

Astronomy and Astrophysics

Astrophysics

Scientific paper

We calculate the flux of ντ produced in the atmosphere by cosmic ray-air collisions. The production channels of ντ from the process pA -> X -> ν τ (bar ν τ )Y with X = Ds ,W±, Z, hb, tbar t , are considered. The calculations are performed by employing perturbative QCD (PQCD). The predicted ντ flux ϕντ is given for energy range 103GeV ≤ E ≤ 108GeV.

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