Warm Higgs-Starobinsky inflation can produce the observed dark matter abundance for 1 MeV and 100 GeV masses through dimension-8 and dimension-9 freeze-in operators, with production concentrated at the inflation-to-radiation transition.
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Scalaron-driven Dark Matter during Warm Inflation via UV Freeze--in
Warm Higgs-Starobinsky inflation can produce the observed dark matter abundance for 1 MeV and 100 GeV masses through dimension-8 and dimension-9 freeze-in operators, with production concentrated at the inflation-to-radiation transition.