Freezing-in Cannibal Dark Sectors

Self-Interacting Dark Matter models can successfully explain dark matter (DM) production through interactions confined within the dark sector.

However, they often lack measurable experimental signals due to their secluded nature.

Including a feeble interaction with the visible sector through a Higgs portal leads not only to potential detection avenues and richer thermal production dynamics, but also to a possible explanation of the initial dark sector population through the freeze-in mechanism.

In this work we study, by solving the full system of coupled Boltzmann equations for the number densities and temperatures of all the involved states, three scenarios of this type where the DM is: a real scalar with broken $\mathbb{Z}_2$, a complex scalar with unbroken $\mathbb{Z}_3$, and a $\mathbb{Z}_3$ scalar with an additional scalar mediator.

All of these models have viable dark matter candidates in a cannibal phase while having different detection profiles.

We show that cosmological bounds can be either exacerbated or evaded by changing the dark sector interactions, leading to potential signatures in long-lived particle and indirect detection experiments.

;Comment: 47 pages, 18 figures.

Figure 1 has been updated to align with Planck constraints on the DM lifetime.

Minor corrections and additional references have been included.

This version matches the published version in JHEP