Vacuum phase space (2Âŗ = 8 states) divided by kinematic DOF (3 spatial dimensions)
Bulk-to-boundary Jacobian from binary quantization (Z=2 â Îą=ln(2))
Topological phase capacity à information conversion
Enhancement fraction (subtract original baryon contribution)
The critical acceleration emerges from thermal equipartition between Unruh and de Sitter temperatures:
Holographic equipartition between Newtonian and MOND regimes:
Relaxation time for enhancement field to respond to collision:
| # | Test | CSU Prediction | Observation | Ī | Status |
|---|---|---|---|---|---|
| 1 | Cosmic Mass Ratio ΊDM/Ίb | 5.514 | 5.4 Âą 0.3 | 0.4Ī | â PASS |
| 2 | Total Matter Density Ίm | 0.321 | 0.315 Âą 0.007 | 0.9Ī | â PASS |
| 3 | Dark Energy Fraction ΊΠ| 0.694 | 0.685 Âą 0.007 | 1.3Ī | â PASS |
| 4 | Global Hubble Hâ | 67.14 km/s/Mpc | 67.36 Âą 0.54 | 0.4Ī | â PASS |
| 5 | Local Hubble Hlocal | 72.91 km/s/Mpc | 73.04 Âą 1.04 | 0.1Ī | â PASS |
| 6 | Critical Acceleration aâ | 1.04Ã10âģšⰠm/s² | ~1.2Ã10âģšⰠ| ~1.3Ī | â PASS |
| 7 | BTFR Slope | 4 (exact) | 3.85 Âą 0.15 | 1.0Ī | â PASS |
| 8 | Bullet Cluster Offset | 231.8 kpc | 250 Âą 30 kpc | 0.6Ī | â PASS |
| 9 | Ghost Galaxies (EFE) | 10/10 | 10/10 | â | â PASS |
| 10 | Dwarf Spheroidals | 7/7 within 1Ī | 7/7 | â | â PASS |
| 11 | CMB Sound Horizon | ~144 Mpc | 144.43 Âą 0.26 | <2Ī | â PASS |
| 12 | Age of Universe | 13.72 Gyr | 13.8 Âą 0.04 | ~2Ī | â PASS |
Run the complete V4 validation suite with 90 assertions across 40 sections.
| Total Assertions | 90 (runtime), 90 in code |
| PASS | 90 |
| FAIL | 0 |
| Pass Rate | 100.0% |
| Total Sections | 40 |
| Real Checks | 85 / 93 = 91.4% |
| Qualitative Checks | 8 / 93 = 8.6% |
| Operation | Count | Usage |
|---|---|---|
diff() |
9 | Entropy derivatives, BH thermodynamics, BTFR slope, Unruh, Bekenstein |
solve() |
4 | Unruh=deSitter equilibrium, rotation curve r-cancellation |
limit() |
4 | Îŧ(x) asymptotic limits, Ī relaxation limit |
simplify() |
9 | Symbolic equation verification throughout |
scipy.integrate.quad() |
6 | Friedmann age, sound horizon, comoving distance, growth factor |
CSU Prediction: Zero signal in all direct detection experiments
LZ, XENONnT, PandaX â all should remain null indefinitely
Falsification: If a WIMP is detected at >5Ī: CSU is falsified
CSU Prediction: Every cluster collision follows Îr â v(1 + 1/âx)
Pattern must be universal, not tuned per cluster
Falsification: Systematic survey of >10 cluster collisions showing different patterns
CSU Prediction: Ξ(zââ) = 8/3 (not 6.514)
At early times, only spatial enhancement contributes (no information conversion yet)
Test: JWST should see different DM/baryon ratio at z>10
Falsification: If Ξ remains constant at all redshifts
CSU Prediction: Lensing mass = Mgas à Ξcosmo at cluster scales
Deviations from NFW profile predictions
Test: Euclid/Roman Space Telescope systematic lensing surveys
Falsification: If lensing masses perfectly match NFW predictions
CSU Prediction: Enhancement field induces small corrections to GW propagation
Test: LISA and next-gen GW detectors
Falsification: If GW propagation is exactly GR with zero corrections
| Z Value | β = ZÂŗ/3 | Ξcosmo | ΊDM/Ίb | Agreement |
|---|---|---|---|---|
| 1.9 | 2.281 | 6.891 | 5.891 | â Too high |
| 2.0 | 2.667 | 6.514 | 5.514 | â Perfect |
| 2.1 | 3.087 | 6.196 | 5.196 | â Too low |
Conclusion: Framework is maximally constrained. Only Z=2 (from Gauss-Bonnet) gives correct ΊDM/Ίb.
| Feature | CSU | ÎCDM | MOND | Verlinde | f(R) |
|---|---|---|---|---|---|
| Free Parameters | 0 | 6+ | 1 | ~2 | 1+ |
| Rotation Curves | â Derived | â Fitted | â Fitted | â ī¸ Partial | â Fitted |
| Bullet Cluster | â 7.2% | â Requires DM | â FAIL | â ī¸ Unclear | â FAIL |
| Ghost Galaxies | â Natural (EFE) | â Impossible | â Natural | â ī¸ Unclear | â No mechanism |
| Hubble Tension | â Resolved | â 5Ī tension | â N/A | â N/A | â ī¸ Partial |
| CMB Peaks | â Derived | â Fitted | â ī¸ Requires HDM | â Unclear | â ī¸ Partial |
| ΊDM/Ίb | â 5.514 (derived) | â Fitted | â No prediction | â No prediction | â No prediction |
| Î Value | â 10âģš²² (derived) | â 10š²Ⱐproblem | â N/A | â ī¸ Partial | â N/A |
| BTFR Slope | â 4 (exact) | â ī¸ Approximate | â 4 (built-in) | â ~4 | â ī¸ Approximate |
| Falsifiable | â 5 tests | â ī¸ Flexible | â Yes | â ī¸ Limited | â Yes |