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Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
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Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
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Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
Journal Article

Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection

2024
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Overview
Λ -Cold Dark Matter ( Λ CDM) has been successful at explaining the large-scale structures in the universe but faces severe issues on smaller scales when compared to observations. Introducing self-interactions between dark matter particles claims to provide a solution to the small-scale issues in the Λ CDM simulations while being consistent with the observations at large scales. The existence of the energy region in which these self-interactions between dark matter particles come close to saturating the S-wave unitarity bound can result in the formation of dark matter bound states called darkonium. In this scenario, all the low energy scattering properties are determined by a single parameter, the inverse scattering length γ . In this work, we set bounds on γ by studying the impact of darkonium on the observations at direct detection experiments using data from CRESST-III and XENON1T. The exclusion limits on γ are then subsequently converted to exclusion limits on the self-interaction cross-section and compared with the constraints from astrophysics and N-body simulations.