Dark decay of the neutron

Abstract

New decay channels for the neutron into dark matter plus other particles have been suggested for explaining a long-standing discrepancy between the neutron lifetime measured from trapped neutrons versus those decaying in flight. Many such scenarios are already ruled out by their effects on neutron stars, and the decay into dark matter plus photon has been experimentally excluded. Here we explore the decay into a dark Dirac fermion $\chi$ and a dark photon $A^{\prime }$, which can be consistent with all constraints if $\chi$ is a subdominant component of the dark matter. Neutron star constraints are evaded if the dark photon mass to coupling ratio is $m_{A^{\prime }}/g^{\prime }\lesssim (45-60)$MeV, depending upon the nuclear equation of state. $g^{\prime }$ and the kinetic mixing between U(1)${}^{\prime }$ and electromagnetism are tightly constrained by direct and indirect dark matter detection, supernova constraints, and cosmological limits.

arXiv comment10 pages, 2 figures. v2: Clarifications and references added. Submitted to JHEP. v3: Dark matter self scattering cross section and constraints from direct detection corrected, additional constraints added. v4: Typos corrected. Matches published version

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