Speaker
Prof.
Reno, Mary Hall Reno
(University of Iowa)
Description
Theoretical evaluations of the high energy atmospheric neutrino and muon fluxes from cosmic ray interactions with air nuclei rely on calculations of charmed particle production and decay. Presented here is a review of approaches to charm contributions to the atmospheric lepton fluxes, including dipole models and the parton model with QCD.
Primary author
Prof.
Reno, Mary Hall Reno
(University of Iowa)
Co-authors
Ina Sarcevic
(University of Arizona)
Rikard Enberg
(Uppsala University)
