Asymmetric dark matter interactions at high density can extend main-sequence lifetimes of ~1 solar-mass stars by several Gyr and quench core convection in stars up to 1.5 solar masses.
G., Garc´ ıa, A., Robertson, R
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Asymmetric Dark Matter Imprint on Low-mass Main-sequence Stars in the Milky Way Nuclear Star Cluster
Asymmetric dark matter interactions at high density can extend main-sequence lifetimes of ~1 solar-mass stars by several Gyr and quench core convection in stars up to 1.5 solar masses.