Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4
Alexander Broberg Skeltved, Nikolai {\O}stgaard, Brant Carlson, Thomas, Gjesteland, and Sebastien Celestin

TL;DR
This study uses GEANT4 simulations to model relativistic runaway electron avalanches and feedback mechanisms in thunderstorms, validating the tool's effectiveness and exploring photon-electron ratios and physics list impacts.
Contribution
It is the first to employ GEANT4 for detailed quantitative modeling of RREAs and feedback in electric fields, comparing physics lists and analyzing photon-electron ratios.
Findings
Electron multiplication during RREAs aligns with previous estimates.
Photon-to-electron ratio depends on electric field and avalanche time.
Physics list choice significantly affects simulation results.
Abstract
This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modelling results related to the production of Terrestrial Gamma-ray Flashes (TGFs) and high-energy particle emission from thunderstorms. We will study the Relativistic Runaway Electron Avalanche (RREA) and the relativistic feedback process, as well as the production of bremsstrahlung photons from Runaway Electrons (REs). The Monte Carlo (MC) simulations take into account the effects of electron ionisation, electron by electron (M{\o}ller) and electron by positron (Bhabha) scattering as well as the bremsstrahlung process and pair-production, in the eV GeV energy range. Our results indicate that the multiplication of electrons during the development of RREAs and under the influence of feedback, are consistent with previous estimates. This is…
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