Abstract

Studying energy deposition by space radiation at the cellular scale provides insights on health risks to astronauts. Using the Monte Carlo track structure code RITRACKS, and the chromosome aberrations code RITCARD, we performed a modeling study of single-ion energy deposition spectra and chromosome aberrations for high-energy (>250 MeV/n) ion beams with linear energy transfer (LET) varying from 0.22 to 149.2 keV/µm. The calculations were performed using cells irradiated directly by mono-energetic ion beams, and by poly-energetic beams after particle transport in a digital mouse model, representing the radiation exposure of a cell in a tissue. To discriminate events from ion tracks directly traversing the nucleus, to events from δ-electrons emitted by distant ion tracks, we categorized ion contributions to microdosimetry or chromosome aberrations into direct and indirect contributions, respectively. The ions were either ions of the mono-energetic beam or secondary ions created in the digital mouse due to interaction of the beam with tissues. For microdosimetry, the indirect contribution is largely independent of the beam LET and minimally impacted by the beam interactions in mice. In contrast, the direct contribution is strongly dependent on the beam LET and shows increased probabilities of having low and high-energy deposition events when considering beam transport. Regarding chromosome aberrations, the indirect contribution induces a small number of simple exchanges, and a negligible number of complex exchanges. The direct contribution is responsible for most simple and complex exchanges. The complex exchanges are significantly increased for some low-LET ion beams when considering beam transport.

Highlights

  • Galactic cosmic rays are composed of approximately 87% protons, 12% helium nuclei, and 1% high-charge and energy (HZE) ions [1]

  • This work investigated the effect of radiation quality and beam transport on both cell nucleus microdosimetry and chromosome aberrations by means of Monte Carlo (MC) simulation with the radiation transport code RITRACKS/RITCARD

  • The effect of beam quality was assessed by considering mono-energetic ion beams of various linear energy transfer (LET) and high energy and simulating their transport within a digital mouse to replicate experimental conditions of ground-based studies

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Summary

Introduction

Galactic cosmic rays are composed of approximately 87% protons, 12% helium nuclei, and 1% high-charge and energy (HZE) ions [1]. This pattern is responsible for the induction of complex DNA damages that can lead to chromosomal aberrations, which are positively correlated with carcinogenesis [3,4] Biological endpoints such as chromosome aberrations are instigated by direct energy depositions from tracks that intersect the cell nucleus and energy depositions from δ-electrons ejected from tracks that crossed neighboring cells. Such mechanisms are relevant to space radiation exposures from galactic cosmic rays and help in determining relative biological effectiveness factors extrapolated from dose–response curves at low dose. The ability to separate such energy contributions to different endpoints provides clear means of studying the track interactions

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