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Probing In-Medium Neutron-to-Dark-Fermion Conversion with Multimessenger Neutron Star Observations
Neutron stars provide a natural environment for probing in-medium neutron-to-dark-fermion conversion and its impact on the dense-matter equation of state (EOS). We use multimessenger neutron star observations to map excluded and not-excluded regions of dark-sector parameter space for an EOS ensemble
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