The Sun Can Strongly Constrain Spin-Dependent Dark Matter Nucleon Scattering Below the Evaporation Limit
This paper demonstrates that by accounting for the competitive dynamics of dark matter evaporation and annihilation, solar observations can significantly constrain spin-dependent dark matter-nucleon scattering cross-sections for masses below the traditional 4 GeV evaporation limit, outperforming terrestrial direct detection constraints by up to five orders of magnitude.