Monte-Carlo modeling of the experiment on ultrahigh-energy cosmic ray and neutrino detection using circumlunar orbital radio detector

A mathematical model of ultrahigh-energy cosmic ray and neutrino detection by radio method is elaborated. Algorithms of solving a problem of revealing by a lunar orbital radio detector of radio pulses emitted by hadronic and electromagnetic cascades initiated by high-energy particles in near-surface layer of lunar regolith are considered. These algorithms can be used for modeling of experiments which utilize radio-transparent media (ice, salt, sand, etc.) as a target of interaction.