The scalar field \(\Phi(t)\) with potential \(V(\Phi)\) replaces the cosmological constant \(\Lambda\):
DESI constraint: \(w = -0.85\) gives \(K/V = (1+w)/(1-w) = 0.0811\). The numerical integration yields \(w \approx -0.995\) over late times, consistent with a slowly rolling field.
Relics behave as pressureless matter. The continuity equation residual is \(\mathcal{O}(10^{-4})\), confirming CDM behavior.
| Phase | Condition | Behavior |
|---|---|---|
| Accretion | \(M > M_{\text{cross}}\) | Growth from environment |
| Evaporation | \(M < M_{\text{cross}}\) | Hawking-like mass loss |
| Freeze-out | \(M \to M_{\text{relic}}\) | Stable Planckian relic |
A \(10\,M_\odot\) black hole evaporates to a relic of mass \(M_{\text{relic}} \sim 10^{-5}\,M_{\text{Pl}}\).
With \(\Gamma_{\text{abs}} = 10^{-25}\,\text{s}^{-1}\), the identity timescale is \(\tau = 3.17 \times 10^{17}\) years — far exceeding the age of the universe. Relics are stable.
Results: \(\Omega_m = 0.314\), \(\Omega_{\text{relic}} = 0.265\), growth rate \(f = 0.529\). Relics cluster identically to CDM.
| Observable | Prediction | Status |
|---|---|---|
| Rotation curve (10 kpc) | 153 km/s | Flat to 23% over 10–100 kpc |
| Rotation curve (100 kpc) | 118 km/s | Consistent with observations |
| Lensing | \(\kappa \sim 10^{-25}\) | Requires full ray-tracing |
All 7 theory closure checks pass:
(1) Field equation of state \(w \approx -0.995\) (DESI: \(-0.85\))
(2) Pressureless relics (mean residual \(3.5 \times 10^{-4}\))
(3) Black hole freeze-out at relic mass
(4) Relic identity preserved (\(\chi = 0.99999\))
(5) Growth rate \(f = 0.529\) (saturates in \(\Lambda\) era)
(6) Flat rotation curves (23% variation, 10–100 kpc)
(7) Relic halo lensing signal present