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Note that for k >4, the evolution of the inflaton is subject to the effects of fragmentation [13, 14] which cause the equation of state to evolve to k = 4

The overall scale of the potential, determined by λ, is fixed by the normalization of the cosmic microwave background (CMB) anisotropy spectrum, depends on k [4] · 1966

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Ultra-Relativistic Freeze-Out During Reheating

hep-ph · 2025-05-07 · conditional · novelty 6.0

Ultra-relativistic freeze-out during reheating produces the observed dark matter abundance across a far wider mass and coupling range than standard WIMP or freeze-in scenarios, with the light-mass region contingent on the cooling history.

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  • Ultra-Relativistic Freeze-Out During Reheating hep-ph · 2025-05-07 · conditional · none · ref 1

    Ultra-relativistic freeze-out during reheating produces the observed dark matter abundance across a far wider mass and coupling range than standard WIMP or freeze-in scenarios, with the light-mass region contingent on the cooling history.