Thermal production of cold “hot dark matter” around eV

Abstract

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.

Misalignment production of vector boson dark matter from axion-SU(2) inflation

“…One of the candidates is a dark photon, which is a gauge boson associated with a hidden U(1) gauge symmetry. There are various known scenarios to produce dark photon particles or excitations as dark matter: gravitational production [1][2][3][4][5][6][7], gravitational thermal scattering [8,9], production through axion-like couplings [10][11][12][13], Higgs dynamics [14,15], kinetic couplings [16][17][18][19], thermal production with the bose-enhancement effect [20], and cosmic strings [21,22]. Moreover, a coherent oscillation of a dark photon field can also account for dark matter.…”