Part VII — Cosmology

From Early Universe to Dark Sectors
← Back to Dual–Flux Homepage

Abstract

We apply the Dual–Flux (DF) framework—in which spacetime-like structure and matter-like excitations emerge from two primitive informational fluxes interacting with a single reactive substrate on a present surface P0—to cosmology. Working strictly within the DF long-memory dynamics (Parts I–VI), and without introducing an inflaton sector, additional dark fields, or phenomenological interpolation functions, we derive an effective FLRW background together with (i) a late-time dark-energy-like acceleration, (ii) a cold-dark-matter component, (iii) a MOND-like galactic regime, and (iv) a nonsingular strong-gravity completion.

In the DF compositional algebra, neutral 4π tripoles provide the dominant cold-dark-matter population, while charged 2π tripoles account for baryons. A single branching fraction y fixes their abundance ratio, Ωb/ΩDM = (1 − y)/y, yielding Ωb/ΩDM = 1/5 for the canonical DF value y = 5/6. The homogeneous long-memory component generates an effective cosmological constant scaling as ΛDF ∼ y H02, whereas the complementary inhomogeneous fraction (1 − y) produces a MOND-like acceleration scale a0 = (1 − y) c H0 and implies the baryonic Tully–Fisher relation.

Black holes are reinterpreted as memory-saturated regions of P0 with bounded curvature and standard Hawking thermodynamics, and the big-bang singularity is replaced by the formation of the present surface itself. We conclude with falsifiable predictions across galactic, cluster, cosmological, and strong-gravity regimes, and outline the bridge to Part VIII where the same DF substrate is used to organise quantum phenomenology via coheron differentiation.

Emergence of Spacetime at a glance
Figure 1 — Cosmology

PDF

Link to the Zenodo version:
Dual–Flux Part VII — Cosmology (Zenodo)
PDF download:
Download PDF