Documentdetail
ID kaart
oai:arXiv.org:1606.03629
Onderwerp
Astrophysics - Instrumentation and... Astrophysics - High Energy Astroph...Auteur
Neronov, A. Semikoz, D. V. Anchordoqui, L. A. Adams, J. Olinto, A. V.Categorie
wetenschappen: astrofysica
Jaar
2016
vermelding datum
09-03-2021
Trefwoorden
study astrophysicsBeschrijving
Neutrinos with energies in the PeV to EeV range produce upgoing extensive air showers when they interact underground close enough to the surface of the Earth.
We study the possibility for detection of such showers with a system of very wide field-of-view imaging atmospheric Cherenkov telescopes, named CHANT for CHerenkov from Astrophysical Neutrinos Telescope, pointing down to a strip below the Earth's horizon from space.
We find that CHANT provides sufficient sensitivity for the study of the astrophysical neutrino flux in a wide energy range, from 10 PeV to 10 EeV.
A space-based CHANT system can discover and study in detail the cosmogenic neutrino flux originating from interactions of ultra-high-energy cosmic rays in the intergalactic medium.
;Comment: 15 pages, 8 figures, accepted to Phys.
Rev. D
Neronov, A.,Semikoz, D. V.,Anchordoqui, L. A.,Adams, J.,Olinto, A. V., 2016, Sensitivity of a proposed space-based Cerenkov astrophysical-neutrino telescope (CHANT)
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