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Dark matter in compact stars
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White dwarfs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark matter. We review detection prospects of wave-like, particulate, macroscopic and black hole dark matter that make use of several exceptional properties of compact stars, such as ultra-high densities, deep fermion degeneracies, low temperatures, nucleon superfluidity, strong magnetic fields, high rotational regularity, and significant gravitational wave emissivity. Foundational topics first made explicit in this document include the effect of the ``propellor phase" on neutron star baryonic accretion, and the contribution of Auger and Cooper pair breaking effects to neutron star heating by dark matter capture.
Forward citations
Cited by 10 Pith papers
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Dark matter scattering with pre-supernova neutrinos
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Complementary Planetary Spectroscopy Probes of Dark Matter
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A self-consistent Higgs-portal framework for dark matter--admixed neutron stars: Collider-motivated benchmarks meet multimessenger constraints
Adding heavy dark matter to neutron stars via nχ=FχnB softens the equation of state and lowers the maximum mass, but the vector interaction invoked is numerically negligible.
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Stability Boundary of Neutron-Dark Matter Mixed Stars
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Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO
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Gravitational Waves as a Probe of Particle Dark Matter
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