arXiv · 2208.11072
Evaluation of the potential of a gamma-ray observatory to detect astrophysical neutrinos through inclined showers
Abstract
We assess the capabilities of a ground-based gamma-ray observatory to detect astrophysical neutrinos with energies in the $100\,{\rm TeV}$ to $100\,{\rm PeV}$ range. The identification of these events would be done through the measurement of very inclined extensive air showers induced by downward-going and upward-going neutrinos. The discrimination of neutrino-induced showers in the overwhelming cosmic-ray background is achieved by analysing the balance of the total electromagnetic and muonic signals of the shower at the ground. We demonstrate that a ${\rm km^2}$-scale wide field-of-view ground-based gamma-ray observatory could detect a couple of Very-High to Ultra-High energy (VHE-UHE) neutrino events per year with a reasonable pointing accuracy, making it an interesting facility for multi-messenger studies with both photons and neutrinos.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jaime Alvarez-Muñiz, Ruben Conceição, Pedro J. Costa, Mário Pimenta, Bernardo Tomé. 2022-09-25. Evaluation of the potential of a gamma-ray observatory to detect astrophysical neutrinos through inclined showers. https://doi.org/10.1103/physrevd.106.102001
Cite the original work for its findings. Save a collection to share your selection of sources.