Accelerated star and galaxy formation in fractal overdensity nodes,
Natural emergence of mature galaxies with high metallicity as early as z12z \sim 12, matching recent JWST observations.
2. Large-Scale Anisotropic Voids from Layered Topology
The multilayered void-Hubble architecture (Sec. II.2 and III.1) predicts that spacetime expansion is not uniform, but instead varies radially and angularly depending on layered boundary conditions and local topological curvature. In particular:
Adjacent spacetime layers with differing Hubble parameters H(r)H(r) produce anisotropic expansion profiles,
These anisotropies manifest observationally as elliptical or directionally biased voids on scales of hundreds of Mpc to several Gpc.
This prediction aligns with:
The CMB cold spot and large-angle alignment anomalies,
Observed bulk flows and hemispherical asymmetries,
Discrepancies in cosmic dipole anisotropy beyond what peculiar motion accounts for.
Numerical simulations (Sec. IV.1 and IV.3) show that when topological interference between layers is included, the resulting void orientations and anisotropic shells resemble features seen in SDSS and Planck data.
3. Galactic Spin and Angular Momentum Alignment
Conventional inflationary cosmology assumes random phase initial conditions leading to uncorrelated spin orientations for galaxies. However, under our fractal-topological model:
The initial matter distribution exhibits directionally coherent filaments and nodes, inherited from the blink event's non-trivial boundary topology,
These lead to preferred angular momentum axes across cosmic structures---especially in regions where the fractal dimension is locally high (i.e., near bifurcation points of nested layers).
From Sec. IV.2 simulations, the galactic spin vector Lg\vec{L}_g shows a statistical bias:
Lgn^layer>0\langle \vec{L}_g \cdot \hat{n}_{\text{layer}} \rangle > 0
where n^layer\hat{n}_{\text{layer}} is the normal vector to a dominant local layer interface. This bias naturally explains:
Observed alignments in galaxy spins over tens to hundreds of Mpc (as seen in SDSS and 2dF),
Statistical correlations between spin direction and large-scale structure orientation,
The planarity and alignment of satellite galaxies around hosts, challenging isotropic collapse models.
4. No Inflation Required for Horizon or Structure Problems
Critically, all of the above emerge without invoking inflation. The key reasons include:
