Gamma Rays from UltraCompact Minihaloes: Effects on the Earth's Atmosphere and Links to Mass Extinction Events
M. Sarkis, G. Beck, B. C. Thomas

TL;DR
This study investigates how gamma rays from dark matter mini-halo annihilation could deplete Earth's ozone, potentially impacting life, but such events are rare compared to other astrophysical sources.
Contribution
It models gamma-ray emissions from UCMHs and assesses their potential atmospheric effects and occurrence rates, linking dark matter to Earth's historical mass extinctions.
Findings
UCMHs can cause significant ozone depletion similar to extinction-linked levels.
The probability of Earth encountering such UCMHs is low.
Other astrophysical phenomena are more likely to impact Earth's atmosphere.
Abstract
Recent studies of the effects on the Earth's atmosphere by astrophysical sources, such as nearby gamma-ray bursts or supernovae, have shown that these events could lead to severe changes in atmospheric composition. Depletion of ozone, the most notable of these changes, is extremely dangerous to living organisms as any decrease in ozone levels leads to an increase in the irradiance of harmful solar radiation at the Earth's surface. In this work we consider dark matter as an astrophysical source of gamma rays, by the annihilation and decay of WIMPs found within dark compact halo objects known as UltraCompact Minihaloes (UCMHs). We calculate the fluence of gamma rays produced in this way and simulate the resulting changes to terrestrial ozone levels using the Goddard Space Flight Center 2D Atmospheric Model. We also calculate the rate at which such events would occur, using estimates for…
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