Thermal production of cold hot dark matter around eV

A very simple production mechanism of feebly interacting dark matter (DM) that rarely annihilates is thermal production, which predicts the DM mass around eV. This has been widely known as the hot DM scenario. Despite there are several observational hints from background lights suggesting a DM in this mass range, the hot DM scenario has been considered strongly in tension with the structure formation of our Universe because the free-streaming length of the DM produced from thermal reactions was thought to be too long. In this paper, I show that the previous conclusions are not always true depending on the reaction for bosonic DM because of the Bose-enhanced reaction at very low momentum. By utilizing a simple 1 <-> 2 decay/inverse decay process to produce DM, I demonstrate that eV range bosonic DM can be thermally produced in a cold manner from a hot plasma through a model-independent analysis applicable to axion, hidden photon, and other bosonic DM candidates. As a result, bosonic DM in the eV mass range may still be unique and theoretically well-motivated. I also discuss some caveats arising from this phenomenon in the freeze-in production of DM, and present a related system that can suppress the hot plasma with thermal reaction.

Automated summary

Thermal production is a simple mechanism for the production of feebly interacting dark matter (DM) with a mass around eV. Previous studies suggested that this hot DM scenario is inconsistent with the structure formation of our Universe due to the long free-streaming length of DM produced from thermal reactions. However, this paper demonstrates that bosonic DM in the eV range can still be thermally produced in a cold manner from a hot plasma through a Bose-enhanced reaction at very low momentum.