Response time structure of electrons and muons recorded by scintillation detectors in showers with energies higher than 5 × 10 18  eV at the Yakutsk EAS array: The search for neutrinos

S. P. Knurenko; Yu. A. Egorov; Z. E. Petrov; I. S. Petrov; I. Ye. Sleptsov

doi:10.3103/S1062873817040268

Response time structure of electrons and muons recorded by scintillation detectors in showers with energies higher than 5 × 10¹⁸ eV at the Yakutsk EAS array: The search for neutrinos

Авторлар: Knurenko S.P.¹, Egorov Y.A.¹, Petrov Z.E.¹, Petrov I.S.¹, Sleptsov I.Y.¹
Мекемелер:
1. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Шығарылым: Том 81, № 4 (2017)
Беттер: 474-477
Бөлім: Proceedings of the 34th National Conference on Cosmic Rays
URL: https://journals.rcsi.science/1062-8738/article/view/185046
DOI: https://doi.org/10.3103/S1062873817040268
ID: 185046

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Аннотация

The procedure for and results from a search for showers generated by such neutral particles as high energy gamma rays and astroneutrinos are presented. A comprehensive analysis of data on electrons, muons, and EAS Cherenkov light, and their response time in scintillation and Cherenkov detectors, is performed.