The moduli portal to dark matter particles

TL;DR

This paper explores how moduli fields in string-inspired models influence the freeze-in production of various dark matter particles, emphasizing the importance of early-universe contributions to accurately determine relic density.

Contribution

It introduces a detailed analysis of scalar, fermionic, and vector dark matter production via moduli exchange, highlighting the significance of pre-radiation era contributions.

Findings

High-temperature dependencies affect DM production rates.

Moduli masses at post-inflationary reheating scale are relevant.

Pre-radiation era contributions are crucial for relic density calculations.

Abstract

The out-of-equilibrium production of dark matter (DM) from standard model (SM) species in the early universe (freeze-in mechanism) is expected in many scenarios in which very heavy beyond the SM fields act as mediators. In this conference, I have talked about the freeze-in of scalar, fermionic and vector DM though the exchange of moduli fields \cite{chowdhury_moduli_2019}, which are in the low-energy spectrum of many extra-dimensions and string theory frameworks. We have shown that the high-temperature dependencies of the production rate densities in this model, as well as the possibility of having moduli masses at the post-inflationary reheating scale, make it crucial to consider the contribution of the freeze-in prior the start of the standard radiation era for a correct prediction of the DM relic density.