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The Hawking evaporation of small black holes formed by the collapse of darkmatter at the center of neutron stars plays a key role in loosing theconstraint on the mass of asymmetric bosonic non-interacting dark matterparticles. Different from previous works we show that such a kind of darkmatter is viable in the mass range from 3.3 GeV to ~ 10 TeV, which covers themost attractive regions, including the preferred asymmetric dark matter mass ~5.7 GeV as well as the 5-15 GeV range favored by DAMA and CoGeNT.

Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars