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Dark matter production via a non-minimal coupling to gravity

We study postinflationary scalar dark matter production via its non-minimal coupling to gravity. During the inflaton oscillation epoch, dark matter is produced resonantly for a sufficiently large non-minimal coupling ξ ≳ 5. We find that backreaction on the curvature and rescattering effects typicall...

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Bibliographic Details
Published in:Journal of cosmology and astroparticle physics 2023-02, Vol.2023 (2), p.35
Main Authors: Lebedev, Oleg, Solomko, Timofey, Yoon, Jong-Hyun
Format: Article
Language:English
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Summary:We study postinflationary scalar dark matter production via its non-minimal coupling to gravity. During the inflaton oscillation epoch, dark matter is produced resonantly for a sufficiently large non-minimal coupling ξ ≳ 5. We find that backreaction on the curvature and rescattering effects typically become important for the values of ξ above 30, which invalidate simple estimates of the production efficiency. At large couplings, the dark matter yield becomes almost independent of  ξ , signifying approximate quasi-equilibrium in the inflaton-dark matter system. Although the analysis gets complicated by the presence of apparent negative energy in the Jordan frame, this behaviour can be regularized by introducing mild dark matter self-interaction. Using lattice simulations, we delineate parameter space leading to the correct dark matter relic abundance.
ISSN:1475-7516
1475-7508
1475-7516
DOI:10.1088/1475-7516/2023/02/035