2013/07/09 by Jan Ebr, Petr Nečesal · 2 citations
Physics and Astronomy · #Air shower #Astrophysics and Cosmic Phenomena #Bremsstrahlung #Cosmic ray #Dark Matter and Cosmic Phenomena #Electron #Monte Carlo method #Muon #Nuclear physics #Optics #Particle physics #Particle physics theoretical and experimental studies #Photon #Physics #Production (economics) #Statistics #Unobservable #astro-ph.HE #hep-ph
paper · pdf · doi:10.1016/j.physletb.2013.07.007
published in Physics Letters B 725(4-5), 185-189 (Elsevier BV) · Accepted for publication in Physics Letters B on 9 July 2013
openalex publication_date 2013/07/09 · arxiv created 2013/07/15 · arxiv updated 2013/07/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Inspired by recent astrophysical observations of leptonic excesses measured by satellite experiments, we consider the impact of some general models of the dark sector on the muon production in extensive air showers. We present a compact approximative expression for the bremsstrahlung of a massive photon from an electron and use it within Monte Carlo simulations to estimate the amount of weakly interacting photon-like massive particles that could be produced in an extensive air shower. We find that the resulting muon production is by many orders of magnitude below the average muon count in a shower and thus unobservable.