Calculations of electric fields for radio detection of Ultra-High Energy particles
Daniel Garc\'ia-Fern\'andez, Jaime Alvarez-Mu\~niz, Washington R., Carvalho Jr, Andr\'es Romero-Wolf, Enrique Zas

TL;DR
This paper evaluates the accuracy of the ZHS algorithm, a key computational method for simulating radio pulses from high-energy particle showers, confirming its validity for detecting Ultra-High Energy cosmic rays and neutrinos.
Contribution
It provides a detailed comparison between the ZHS algorithm and exact solutions, clarifying the conditions for its validity in simulating electromagnetic pulses in dense media.
Findings
ZHS algorithm accurately models Cherenkov radiation in dense media.
The algorithm is valid for most Ultra-High Energy neutrino detection scenarios.
Comparison with exact solutions confirms the algorithm's reliability.
Abstract
The detection of electromagnetic pulses from high energy showers is used as a means to search for Ultra-High Energy cosmic ray and neutrino interactions. An approximate formula has been obtained to numerically evaluate the radio pulse emitted by a charged particle that instantaneously accelerates, moves at constant speed along a straight track and halts again instantaneously. The approximate solution is applied to the particle track after dividing it in smaller subintervals. The resulting algorithm (often referred to as the ZHS algorithm) is also the basis for most of the simulations of the electric field produced in high energy showers in dense media. In this work, the electromagnetic pulses as predicted with the ZHS algorithm are compared to those obtained with an exact solution of the electric field produced by a charged particle track. The precise conditions that must apply for the…
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