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EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors
Conference proceeding   Open access

EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors

Mary Hall Reno, Tonia M. Venters, John F. Krizmanic, Probe of Extreme MultiMessenger Astrophysics (POEMMA) and JEM-EUSO Collaboration
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021, Vol.395, 1201
01/01/2022
DOI: 10.22323/1.395.1201
url
https://doi.org/10.22323/1.395.1201View
Published (Version of record) Open Access

Abstract

Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.
Physical Sciences Physics Astronomy & Astrophysics Physics, Particles & Fields Science & Technology

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