DFH Cosmology: Unifying Inflation, CMB, and Dark Energy via a Time-Varying Coupling g(t)
Authors/Creators
Description
We extend the DFH framework of expansion without cosmological constant to
the linear perturbation regime. A canonical field ϕ with scale function g(t) unifies
the background dynamics from the Big Bang to today. Here we show that the same
scaling law governs matter perturbation growth, without introducing independent
dark energy components. We derive the modified growth equation ¨δ + 2H(t)
˙δ =
4πGeff(t)ρmδ, where Geff(t) inherits the evolution of g(t). The model predicts a
growth rate fσ8(z) consistent with RSD data, suppresses power at sub-Mpc scales
solving the missing satellites problem, and generates flat rotation curves without
additional cold dark matter. With a single free parameter f∗, DFH reproduces
the structure formation history from recombination to z = 0, offering a complete
cosmology of background + perturbations with a single physical cause.
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Cosmologia_Big_Bang__Presente_en_V5 (1).pdf
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Additional details
Related works
- Cites
- Data paper: 10.5281/zenodo.20510142 (DOI)
- Data paper: 10.5281/zenodo.20074279 (DOI)