Terrestrial Effects of Nearby Supernovae: Updated Modeling
Brian C. Thomas (Washburn University), Alexander M. Yelland, (Washburn University, MIT)

TL;DR
This study reevaluates the impact of nearby supernovae on Earth by incorporating early-time suppression of cosmic rays, leading to revised estimates of atmospheric and biospheric effects, and suggests the lethal distance is closer than previously thought.
Contribution
The paper introduces an updated model of cosmic ray transport from supernovae, including early-time suppression, which refines estimates of their atmospheric and biological impacts.
Findings
Lower atmospheric ionization and ozone depletion at 100 pc compared to previous models.
Sea-level muon radiation doses are significantly smaller, especially at 50 pc.
The lethal supernova distance is revised to approximately 20 pc, closer than the traditionally assumed 8-10 pc.
Abstract
We have reevaluated recent studies of the effects on Earth by cosmic rays (CRs) from nearby supernovae (SNe) at 100 and 50 pc, in the diffusive transport CR case, here including an early-time suppression at lower CR energies neglected in the previous works. Inclusion of this suppression leads to lower overall CR fluxes at early times, lower atmospheric ionization, smaller resulting ozone depletion, and lower sea-level muon radiation doses. Differences in the atmospheric impacts are most pronounced for the 100 pc case with less significant differences in the 50 pc case. We find a greater discrepancy in the modeled sea-level muon radiation dose, with significantly smaller dose values in the 50 pc case; our results indicate it is unlikely that muon radiation is a significant threat to the biosphere for SNe beyond 20 pc, for the diffusive transport case. We have also performed new modeling…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Space Science and Extraterrestrial Life
