Towards a fast and precise forward model for air shower radio simulation
David Butler, Tim Huege, Olaf Scholten

TL;DR
This paper introduces a semi-analytical model for air shower radio emission that significantly reduces computation time while maintaining accuracy, enhancing the efficiency of cosmic ray detection methods.
Contribution
It presents a novel semi-analytical framework that maps template simulations to radio event specifications, enabling faster and more direct modeling of air shower radio signals.
Findings
Model reduces simulation time compared to Monte Carlo methods.
Allows direct input of shower maximum depth in simulations.
Potential to improve air shower reconstruction accuracy.
Abstract
The radio detection method for cosmic rays relies on coherent emission from electrons and positrons which is beamed in a narrow cone along the shower axis. Currently the only mod- els to reproduce this emission with sufficient accuracy are Monte Carlo based simulations of the particle and radio emission physics, which require large investments of computation time. The work presented here focuses on condensing the simulation results into a semi-analytical model. This relies on building a framework based on theoretical predictions of radio emission, but instead of calculating the radio signal directly these models are used to map template simu- lations to the specifications of a given radio event. Our current approach slices the radio signal based on atmospheric depth of origin and weights these slices based on a shower parameter such as electron number or an effective dipole moment. One…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
