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


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Resumo

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.

Sobre autores

S. Knurenko

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: igor.petrov@ikfia.sbras.ru
Rússia, Yakutsk, 677980

Yu. Egorov

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: igor.petrov@ikfia.sbras.ru
Rússia, Yakutsk, 677980

Z. Petrov

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: igor.petrov@ikfia.sbras.ru
Rússia, Yakutsk, 677980

I. Petrov

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Autor responsável pela correspondência
Email: igor.petrov@ikfia.sbras.ru
Rússia, Yakutsk, 677980

I. Sleptsov

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: igor.petrov@ikfia.sbras.ru
Rússia, Yakutsk, 677980

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