2001/05/25 by C. G. S. Costa, Costa, C. G. S., C. Salles +1
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Radio Astronomy Observations and Technology #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0105271
16 pages, 8 figures, Talk given at PHENO 2001 (Madison, WI)
arxiv created 2001/05/25 · openalex publication_date 2001/05/25 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present an overview of the phenomenology of prompt neutrinos produced in the atmosphere by the decay of charmed particles. In face of the great activity involving operational and proposed large scale neutrino telescopes, we discuss the implications of different scenarios in calculating the prompt flux, upon the detectable signals in these experiments.