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Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars
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The Hawking evaporation of small black holes formed by the collapse of dark matter at the center of neutron stars plays a key role in loosing the constraint on the mass of asymmetric bosonic non-interacting dark matter particles. Different from previous works we show that such a kind of dark matter is viable in the mass range from 3.3 GeV to ~ 10 TeV, which covers the most 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.
Forward citations
Cited by 2 Pith papers
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Capture Driven Evolution of Asymmetric Dark Matter in Non-rotating Neutron Stars
Capture-driven accumulation of asymmetric dark matter in neutron stars stays gravitationally subdominant over a Hubble time and produces no detectable changes in tidal observables.
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Dynamical Boson Stars
Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.
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