A branching model for hadronic air showers
High Energy Astrophysical Phenomena
2015-09-02 v1
Abstract
We introduce a simple branching model for the development of hadronic showers in the Earth's atmosphere. Based on this model, we show how the size of the pionic component followed by muons can be estimated. Several aspects of the subsequent muonic component are also discussed. We focus on the energy evolution of the muon production depth. We also estimate the impact of the primary particle mass on the size of the hadronic component. Even though a precise calculation of the development of air showers must be left to complex Monte Carlo simulations, the proposed model can reveal qualitative insight into the air shower physics.
Keywords
Cite
@article{arxiv.1509.00364,
title = {A branching model for hadronic air showers},
author = {Vladimir Novotny and Dalibor Nosek and Jan Ebr},
journal= {arXiv preprint arXiv:1509.00364},
year = {2015}
}
Comments
In Proceedings of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands