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
- Authors: Knurenko S.P.1, Egorov Y.A.1, Petrov Z.E.1, Petrov I.S.1, Sleptsov I.Y.1
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Affiliations:
- Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- Issue: Vol 81, No 4 (2017)
- Pages: 474-477
- Section: 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
Cite item
Abstract
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.
About the authors
S. P. Knurenko
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Russian Federation, Yakutsk, 677980
Yu. A. Egorov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Russian Federation, Yakutsk, 677980
Z. E. Petrov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Russian Federation, Yakutsk, 677980
I. S. Petrov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Author for correspondence.
Email: igor.petrov@ikfia.sbras.ru
Russian Federation, Yakutsk, 677980
I. Ye. Sleptsov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Russian Federation, Yakutsk, 677980
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