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We report recent results on the impact of asymmetric dark matter (DM)particles on low-mass stars. First, we found that the small convective coreexpected in stars with masses between 1.1 and 1.3 Msun is suppressed due to DMcooling. Moreover, stars with masses below 1 Msun have their centraltemperatures and densities more strongly influenced by DM than in the solarcase. We were able to put limits to the DM mass and spin-dependent DM-protonscattering cross section by comparing the modelling of the nearby star AlphaCen B with photometric, spectroscopic and asteroseismic observations.

Constraints on asymmetric dark matter from asteroseismology