Comments on the physics potential of ultra-high-energy neutrino interactions with OWL

Details Comments on the physics potential of ultra-high-energy neutrino interactions with OWL Comments on the physics potential of ultra-high-energy neutrino interactions with OWL

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..433..262c&link_type=abstract

Workshop on observing giant cosmic ray air showers from >1020 eV particles from space. AIP Conference Proceedings, Volume 433, p

Physics

Cosmic Rays, Elementary Particle Processes

Scientific paper

The study of neutrino interactions and sources for energies >=1019 eV is discussed. The OWL NASA project could play a very important role in this field. We make a simple estimate of the neutrino rate in OWL and find a small value. It is essential to design OWL with either a larger target volume or a planned upgrade to larger target volume.

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