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Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4

This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes and high‐energy particle emission from thunderstorms. We will study the relativistic runawa...

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Published in:Journal of geophysical research. Space physics 2014-11, Vol.119 (11), p.9174-9191
Main Authors: Skeltved, Alexander Broberg, Østgaard, Nikolai, Carlson, Brant, Gjesteland, Thomas, Celestin, Sebastien
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container_issue 11
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container_title Journal of geophysical research. Space physics
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creator Skeltved, Alexander Broberg
Østgaard, Nikolai
Carlson, Brant
Gjesteland, Thomas
Celestin, Sebastien
description This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes 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. The Monte Carlo simulations take into account the effects of electron ionization, electron by electron (Møller), and electron by positron (Bhabha) scattering as well as the bremsstrahlung process and pair production, in the 250 eV to 100 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 important to validate GEANT4 as a tool to model RREAs and feedback in homogeneous electric fields. We also determine the ratio of bremsstrahlung photons to energetic electrons Nγ/Ne. We then show that the ratio has a dependence on the electric field, which can be expressed by the avalanche time τ(E) and the bremsstrahlung coefficient α(ϵ). In addition, we present comparisons of GEANT4 simulations performed with a “standard” and a “low‐energy” physics list both validated in the 1 keV to 100 GeV energy range. This comparison shows that the choice of physics list used in GEANT4 simulations has a significant effect on the results. Key Points Testing the feedback mechanism with GEANT4Validating the GEANT4 programming toolkitStudy the ratio of bremsstrahlung photons to electrons at TGF source altitude
doi_str_mv 10.1002/2014JA020504
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In addition, we present comparisons of GEANT4 simulations performed with a “standard” and a “low‐energy” physics list both validated in the 1 keV to 100 GeV energy range. This comparison shows that the choice of physics list used in GEANT4 simulations has a significant effect on the results. 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subjects Bremsstrahlung
Computer simulation
Electric fields
Electron avalanche
Energy
Feedback
Gamma rays
Ionization
lightning
Lists
Monte Carlo simulation
Photons
Physics
Relativism
RREA
runaway relativistic electron avalanche
Sciences of the Universe
terrestrial gamma ray flashes
TGF
Thunderstorms
title Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4
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