# Making dark matter out of light: freeze-in from plasma effects

## TL;DR

This paper refines the calculation of dark matter relic abundance produced via freeze-in through a light vector mediator, highlighting the importance of plasma effects like plasmon decay, which significantly influence detection prospects.

## Contribution

It introduces an additional production channel via plasmon decay and updates relic abundance calculations, emphasizing plasma effects in freeze-in dark matter models.

## Key findings

- Plasmon decay is a dominant production channel for sub-MeV dark matter.
- Including plasma effects reduces the expected signals in dark matter searches.
- Dark matter exhibits a non-thermal phase space distribution affecting cosmology.

## Abstract

Dark matter (DM) could couple to particles in the Standard Model (SM) through a light vector mediator. In the limit of small coupling, this portal could be responsible for producing the observed DM abundance through a mechanism known as freeze-in. Furthermore, the requisite DM-SM couplings provide a concrete benchmark for direct and indirect searches for DM. In this paper, we present updated calculations of the relic abundance for DM produced by freeze-in through a light vector mediator. We identify an additional production channel: the decay of photons that acquire an in-medium plasma mass. These plasmon decays are a dominant channel for DM production for sub-MeV DM masses, and including this channel leads to a significant reduction in the predicted signal strength for DM searches. Accounting for production from both plasmon decays and annihilations of SM fermions, the DM acquires a highly non-thermal phase space distribution which impacts the cosmology at later times; these cosmological effects will be explored in a companion paper.