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Non-thermal Dark Matter from Modified Early Matter Domination · Around

2018

Non-thermal Dark Matter from Modified Early Matter Domination

Allahverdi, Rouzbeh, Osiński, Jacek K.

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Thermal freeze-out or freeze-in during a period of early matter domination can give rise to the correct dark matter abundance for $\langle \sigma_{\rm ann} v \rangle_{\rm f} < 3 \times 10^{-26}$ cm$^3$ s$^{-1}$.

In the standard scenario, a single field that behaves like matter drives the early matter dominated era.
However, in realistic models, this epoch may involve more than one field.
In this paper, we study the effect of such a modification on the production of dark matter during early matter domination.

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