Publication:
The Radar Echo Telescope for Cosmic Rays: Pathfinder experiment for a next-generation neutrino observatory

Дата
2021
Авторы
Prohira, S.
De, Vries, K. D.
Allison, P.
Beatty, J.
Besson, D.
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Научные группы
Организационные подразделения
Организационная единица
Институт ядерной физики и технологий
Цель ИЯФиТ и стратегия развития - создание и развитие научно-образовательного центра мирового уровня в области ядерной физики и технологий, радиационного материаловедения, физики элементарных частиц, астрофизики и космофизики.
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Аннотация
© 2021 American Physical Society.The Radar Echo Telescope for Cosmic Rays (RET-CR) is a recently funded experiment designed to detect the englacial cascade of a cosmic ray-initiated air shower via in-ice radar, toward the goal of a full-scale, next-generation experiment to detect ultrahigh energy neutrinos in polar ice. For cosmic rays with a primary energy greater than 10 PeV, roughly 10% of an air shower's energy reaches the surface of a high elevation ice sheet (≳2 k˙m) concentrated into a radius of roughly 10 cm. This penetrating shower core creates an in-ice cascade orders of magnitude more dense than the preceding in-air cascade. This dense cascade can be detected via the radar echo technique, where transmitted radio waves are reflected from the ionization deposit left in the wake of the cascade. RET-CR will test the radar echo method in nature, with the in-ice cascade of a cosmic ray-initiated air shower serving as a test beam. We present the projected event rate and sensitivity based upon a three part simulation using corsika, geant4, and radioscatter. RET-CR expects ∼1 radar echo event per day.
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Цитирование
The Radar Echo Telescope for Cosmic Rays: Pathfinder experiment for a next-generation neutrino observatory / Prohira, S. [et al.] // Physical Review D. - 2021. - 104. - № 10. - 10.1103/PhysRevD.104.102006
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