3D simulation for Cherenkov emissions in Extensive Air Showers

TL;DR

This paper introduces BinTheSky, a 3D simulation framework for Cherenkov light emissions in Extensive Air Showers, addressing computational challenges of existing methods at ultra high energies.

Contribution

It presents a novel framework that simulates Cherenkov light emissions using Monte Carlo data, enabling detailed spatial and temporal analysis at ground level.

Findings

Efficient simulation of Cherenkov light distributions at ground level.

Reduced computational resources compared to traditional methods.

Accurate modeling of light propagation and attenuation.

Abstract

The development of a 3-dimensional simulation for Cherenkov photon emissions in Extensive Air Showers (EAS) is reported in this paper. CORSIKA is the most widely used Monte-Carlo generator for the description of EAS, but it is not recommended to calculate Cherenkov light emissions for EAS at ultra high energies due to the enormous amount of data storage and running time required. The presented BinTheSky is a framework to simulate the Cherenkov light emissions using the spatial information produced by Monte-Carlo generators. The light is emitted in the shower, propagated and attenuated to the ground. The framework enables one to calculate the light spatial, timing and directional distributions at the ground or at a given altitude, whereas the usual approach of Ultra High Energy Cosmic Ray experiments relies on the simulation of the longitudinal shower development and on parametrizations of the transverse shower distributions.