Speaker
Prof.
Mary Hall Reno
(University of Iowa)
Description
The high energy atmospheric neutrino flux is dominated by charm production by cosmic ray interactions in the atmosphere, followed by their prompt decays. Using next-to-leading order QCD and several cosmic ray flux parameterizations, the prompt atmospheric neutrino flux is discussed, along with uncertainties associated with the perturbative evaluation.
Primary authors
Prof.
Anna Stasto
(Pennsylvania State University)
Dr
Atri Bhattacharya
(University of Arizona)
Prof.
Ina Sarcevic
(University of Arizona)
Prof.
Mary Hall Reno
(University of Iowa)
Prof.
Rikard Enberg
(University of Uppsala)
