2002/12/16 by Alexander Kusenko · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Computer science #Dark Matter and Cosmic Phenomena #Neutrino #Neutrino Physics Research #Nuclear physics #Physics #hep-ph
paper · pdf · doi:10.1142/9789812704962_0075
published in Multiparticle Dynamics, 387-390 · talk presented at XXXII International Symposium on Multiparticle Dynamics, September 7-13, 2002, Ukraine
arxiv created 2002/12/16 · openalex publication_date 2003/07/01 · arxiv updated 2017/08/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Future detection of ultrahigh-energy neutrinos will open a new window on physics at center-of-mass energy 105 GeV and higher. In particular, observations of neutrino-initiated showers will help test the Standard Model predictions for the neutrino-nucleon cross section.