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
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.