Hadrophilic Light Dark Matter from the Atmosphere

TL;DR

This paper explores the production and detection of hadrophilic light dark matter from atmospheric cosmic-ray interactions, providing new limits and projections for experimental searches in the sub-GeV mass range.

Contribution

It introduces the first detailed analysis of meson decay channels including η, η′, and K+ for dark matter production, improving constraints for DM masses above a few hundred MeV.

Findings

New limits for DM masses above a few hundred MeV from atmospheric meson decays.

Inclusion of nuclear form factor effects significantly alters the detectable DM parameter space.

Projections for upcoming experiments like DARWIN extend the search for sub-GeV dark matter.

Abstract

Light sub-GeV dark matter (DM) constitutes an underexplored target, beyond the optimized sensitivity of typical direct DM detection experiments. We comprehensively investigate hadrophilic light DM produced from cosmic-ray collisions with the atmosphere. The resulting relativistic DM, originating from meson decays, can be efficiently observed in variety of experiments, such as XENON1T. We include for the first time decays of $\eta$, $\eta^{\prime}$ and $K^+$ mesons, leading to improved limits for DM masses above few hundred MeV. We incorporate an exact treatment of the DM attenuation in Earth and demonstrate that nuclear form factor effects can significantly impact the resulting testable DM parameter space. Further, we establish projections for upcoming experiments, such as DARWIN, over a wide range of DM masses below the GeV scale.