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Given the lack of empirical evidence of weakly interacting dark matter, it isreasonable to look to other candidates such as a confining dark sector with asimilar number of particles as the standard model. Twin Higgs mirror matter isone such model that is a twin of the standard model with particles masses 3--6times heavier than the standard model that solves the hierarchy problem. Thisgenerically predicts mirror neutron stars, degenerate objects made entirely ofmirror nuclear matter. We find their structure using a realistic equation ofstate from crust (nuclei) to core (relativistic mean-field model) and scale theparticle masses using lattice QCD results. We find that mirror neutron starshave unique signatures that are detectable via gravitational waves and binarypulsars, that provides an intriguing possibility for probing dark matter.

Mirror Neutron Stars: How QCD can be used to study dark matter through gravitational waves