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arxiv: 1806.00903 · v2 · pith:2OWED5S4new · submitted 2018-06-04 · ⚛️ nucl-th

Neutron to Dark Matter Decay in Neutron Stars

classification ⚛️ nucl-th
keywords neutrondarkdecaymatterparticleastro-physicalcomponentconcerning
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Recent proposals have suggested that a previously unknown decay mode of the neutron into a dark matter particle could solve the long lasting measurement problem of the neutron decay width. We show that, if the dark particle in neutron decay is the major component of the dark matter in the universe, this proposal is in disagreement with modern astro-physical data concerning neutron star masses.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Bulk viscosity from neutron decays to dark baryons in neutron star matter

    astro-ph.HE 2025-09 conditional novelty 5.0

    Neutron dark decays modify the equation of state and either mildly suppress or strongly enhance bulk viscosity in neutron star merger conditions, depending on the in-medium decay rate.