Speeding Up the Search for Dark Matter

The calculation of the thermally averaged effective cross section for a scalar particle-specifically one mirroring the quantum properties of up-type quarks-demonstrates that incorporating bound state formation, decay, and transitions among those states significantly alters predictions, a difference most pronounced when considering scenarios involving color-charged but electrically neutral particles at masses around [latex]10^6[/latex] GeV and employing running QCD and QED couplings.

A new computational tool dramatically accelerates calculations of how dark matter particles interacted in the early universe, paving the way for more comprehensive cosmological modeling.