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Search for the Neutron Decay nrightarrow X+γ where X is a dark matter particle

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arxiv 1802.01595 v1 pith:S4QZUWCD submitted 2018-02-05 nucl-ex

Search for the Neutron Decay nrightarrow X+γ where X is a dark matter particle

classification nucl-ex
keywords darkmatterdecaygammaparticlediscrepancylifetimemethods
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In a recent paper submitted to Physical Review Letters, Fornal and Grinstein have suggested that the discrepancy between two different methods of neutron lifetime measurements, the beam and bottle methods can be explained by a previously unobserved dark matter decay mode, n$\rightarrow$ X+$\gamma$ where X is a dark matter particle. We have performed a search for this decay mode over the allowed range of energies of the monoenergetic gamma ray for X to be a dark matter particle. We exclude the possibility of a sufficiently strong branch to explain the lifetime discrepancy with greater than 4 sigma confidence.

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Cited by 1 Pith paper

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  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.