Using three new nuclear equation-of-state models, the authors derive model-dependent bounds on the dark matter self-interaction strength in the neutron decay anomaly scenario from neutron star mass, radius, and tidal deformability data combined with galaxy cluster cross-section limits.
Search for the Neutron Decay n→ X + γ, Where X is a Dark Matter Particle
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Neutron Decay Anomaly and Its Effects on Neutron Star Properties
Using three new nuclear equation-of-state models, the authors derive model-dependent bounds on the dark matter self-interaction strength in the neutron decay anomaly scenario from neutron star mass, radius, and tidal deformability data combined with galaxy cluster cross-section limits.