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Mirror Neutron Stars
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The fundamental nature of dark matter is entirely unknown. A compelling candidate is Twin Higgs mirror matter, invisible hidden-sector cousins of the Standard Model particles and forces. This predicts mirror neutron stars made entirely of mirror nuclear matter. We find their structure using realistic equations of state, robustly modified based on first-principle quantum chromodynamic calculations, for the first time. This allows us to predict their gravitational wave signals, demonstrating an impressive discovery potential and ability to probe dark sectors connected to the hierarchy problem.
Forward citations
Cited by 3 Pith papers
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Gravitational Waves From Dark Binaries With Finite-Range Dark Forces
A finite-range dark force between dark-matter binaries sharpens and enhances the predicted gravitational wave background, adding knee features tied to the mediator mass.
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Dark Astronomy with Dark Matter Detectors
A proposal to detect the dark photon starlight from dissipative dark matter, with a new directional surface conversion mechanism in metals.
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Supernova Remnants with Mirror Dark Matter and Hyperons
Mirror dark matter inside proto-neutron stars reduces maximum mass, radius, and tidal deformability while heating the remnant and raising the speed of sound.
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