Cosmological and astrophysical probes of dark baryons

We examine the cosmological and astrophysical signatures of a dark baryon, a neutral fermion that mixes with the neutron. As the mixing is through a higher-dimensional operator at the quark level, production of the dark baryon at high energies is enhanced so that its abundance in the early universe may be significant. Treating its initial abundance as a free parameter, we derive new, powerful limits on the properties of the dark baryon. Primordial nucleosynthesis and the cosmic microwave background provide strong constraints due to the interconversion of neutrons to dark baryons through their induced transition dipole, and due to late decays of the dark baryon. Additionally, neutrons in a neutron star could decay slowly to dark baryons, providing a novel source of heat that is constrained by measurements of pulsar temperatures. Taking all the constraints into account, we identify parameter space where the dark baryon can be a viable dark matter candidate and discuss promising avenues for probing it.

Automated summary

This study examines the cosmological and astrophysical signatures of a dark baryon that mixes with neutrons, discussing enhanced production at high energies and constraints from various sources such as primordial nucleosynthesis, the cosmic microwave background, and neutron decays in neutron stars. The research identifies parameter space where the dark baryon can be a viable dark matter candidate and explores potential avenues for further investigation.