Submitted:
23 March 2026
Posted:
25 March 2026
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Abstract
Keywords:
Guidelines for Readers (Roadmap)
- Paper I [1] establishes the thermodynamic ontology of GERT and calibrates the frozen functions against cosmological background data.
- Paper II [2] identifies the late-time hyperdilute boundary where relativistic metric legibility progressively dissolves.
- Paper III [3] determines the early-time emergence boundary of relativistic metric legibility, completing the finite relativistic domain map.
- Paper IV [4] reconstructs the internal thermodynamic anatomy of the relativistic window, including cohesive and entropic transition landmarks.
- Paper V [5] derives the gravitational-wave consequences of that anatomy, including the Tensorial Scar and the Thermodynamic Parsec anchors.
- This manuscript develops the zero-parameter local bridge and tests it from galaxy to cluster scales without introducing new fields or fitted local constants.
1. Introduction
1.1. The Gap Declared by the (Papers I–V)
1.2. The Theoretical Landscape: What Exists and What is Missing
1.3. Dark Matter as a Thermodynamic Problem
1.4. Strategy and Structure
2. Methods: Mathematical Formalism
2.1. GERT Thermodynamic Functions from Paper I
2.2. The Constructive-Memory Hypothesis for Bound Systems
2.3. The Cohesive Screening Factor S(x): Why This Form?
2.4. The Derived Acceleration Scale: The Milgrom Coincidence
2.5. The Full Equation v0.4
3. Results I - Validation: SPARC Rotation Curves
3.1. Sample and Methodology
3.2. Development of the Zero-Parameter Equation


3.3. GERT v0.4 — Final Equation
3.4. The Radial Acceleration Relation as a Thermodynamic Consequence
4. Results II - The Baryonic Tully-Fisher Relation: Analytic Derivation
4.1. Derivation of the Exponent 4
4.2. Amplitude and Dependence
5. Results III - Galaxy Cluster Test


6. Discussion: Physical Implications
6.1. Dark Matter as Thermodynamic Memory
6.2. The Thermodynamic Bridge: Unifying Cosmic and Galactic Scales
6.3. Comparison with ΛCDM, MOND and Emergent Gravity
6.4. Falsifiable Predictions and Validity Domain
7. Conclusions
- 1.
- Zero free parameters. All ingredients — , , — are derived from the Paper I [1] MCMC fit. The Solar System constraint is satisfied with correction < 10⁻¹² by a double-suppression mechanism (S ≈ 1.8×10⁻⁸; ν ∼ 10⁻⁸) — a consequence of thermodynamic structure, not tuning.
- 2.
- The Milgrom coincidence is derived thermodynamically. = cH₀/2π = 1.122×10⁻¹⁰ m/s², within 7% of Milgrom’s a₀. The acceleration scale of modified gravity is the current expansion rate expressed in acceleration units — not a new constant of nature, but a consequence of thermodynamic history.
- 3.
- Six SPARC rotation curves pass, 6/6. The RAR scatter is reduced by 37.5% without parameter adjustment. This is the first reduction of a galactic scaling relation scatter from a purely cosmological theory with no galaxy-specific free parameters.
- 4.
- The BTFR exponent 4 is derived analytically from the additive-square-root structure of Eq. 6, with amplitude within 11% of observation. This is the first thermodynamic derivation of the BTFR exponent from first principles.
- 5.
- Six galaxy clusters pass, 6/6 — including the Coma benchmark at 4.5% agreement with weak lensing (R = 0.938). This is the first successful application of an emergent-gravity theory to galaxy clusters without additional free parameters. MOND and Verlinde fail this test; GERT passes.
7.1. The Central Statement of GERT VI
7.2. Open Challenges and Future Work
8. Code and Data Availability
Manuscript License
Author Contributions
Funding
Institutional Review Board Statement
Data Availability Statement
Conflicts of Interest
References
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| Property | CDM | MOND | Verlinde EG | GERT (this paper) |
|---|---|---|---|---|
| Dark matter substance | Yes (CDM particle) | No | No | No |
| Free parameters (local) | per galaxy | (postulated) | 0 | 0 |
| Fits cosmological background | Yes | No | Fails [21] | Yes (Paper I [1]) |
| Fits rotation curves | With tuning | Yes | Yes [18] | Yes (6/6) |
| Fits galaxy clusters | Yes (with CDM) | Fails [14,15] | Fails [19,20] | Yes (6/6) |
| BTFR slope = 4 | Empirical fit | By construction | Approximately | Derived analytically |
| Milgrom scale origin | Coincidence | Postulate | Asserts | Derives |
| Threshold space | — | Acceleration | Acceleration | Density |
| Unified cosmic + local | No | No | No | Yes |
| Local structure | Typical ρ (kg m⁻³) | log₁₀ρ | GERT milestone |
|---|---|---|---|
| Galactic bulge | 10⁻¹⁸ | −18 | = −17.41 (cohesive peak) |
| Solar neighbourhood | 10⁻²⁰ | −20 | = −20.30 (builder→maintainer) |
| Outer halo / disc outskirts | 10⁻²⁴ | −24 | = −23.93 (entropic peak) |
| Galaxy cluster at r₅₀₀ | 10⁻²⁵·⁵ | −25.5 | = −25.60 (entropic transition) |
| Parameter | Value | Physical meaning |
|---|---|---|
| 0.7831 | Initial cohesive fraction (builder era) | |
| 0.5851 | Final cohesive fraction (entropic era) | |
| −20.30 | Cohesive transition density [log kg m⁻³] | |
| 1.0 dex | Cohesive logistic width | |
| 0.37 | Recombination peak amplitude (multiplicative) | |
| −17.41 | Recombination peak centre [log kg m⁻³] | |
| 1.0 dex | Recombination peak width | |
| 1.3414 | Initial entropic fraction | |
| 1.1236 | Minimum entropic fraction | |
| −25.60 | Entropic transition density [log kg m⁻³] | |
| 2.0 dex | Entropic logistic width | |
| 4.6245 | Entropic peak amplitude at (Layer 2 regime) | |
| −23.93 | Entropic peak centre [log kg ] | |
| 1.0 dex | Entropic peak width | |
| 0.143, −26.750 | Gas regime parameters | |
| 72.5 km/s/Mpc | Hubble constant |
| Regime | Condition | Limiting form | Physical context |
|---|---|---|---|
| Newtonian | ≫ | → (correction → 0) | Compact, massive systems |
| MOND-like | ≪ | Dwarf galaxies, halo outskirts | |
| Screened | correction < 10⁻¹² | Solar System, molecular clouds |
| Galaxy | Type | M★ (M☉) | χ²/N Newton | χ²/N GERT | Improvement | Pass |
|---|---|---|---|---|---|---|
| DDO154 [31] | Dwarf irr. | 1.5×10⁷ | 864.3 | 127.3 | +85.3% | ✓ |
| NGC3109 | Dwarf irr. | 3.0×10⁸ | 152.7 | 29.2 | +80.9% | ✓ |
| NGC2403 | Interm. spiral | 8.0×10⁹ | 236.0 | 68.0 | +71.2% | ✓ |
| NGC6503 | Interm. spiral | 1.5×10¹⁰ | 131.7 | 33.2 | +74.8% | ✓ |
| NGC 3198 [32] | Large spiral | 3.0×10¹⁰ | 247.3 | 55.6 | +77.5% | ✓ |
| UGC 2885 [33] | Giant spiral | 2.0×10¹¹ | 117.3 | 111.8 | +4.7% | ✓ |
| Regime | A [M☉/(km/s)⁴] | Δ log A | ||
|---|---|---|---|---|
| −22.0 | Disc outer | 0.481 | 289.8 | ×6.0 |
| −23.0 | Halo typical | 1.227 | 44.6 | −0.11 |
| −23.4 | Virial shell | 1.369 | 35.8 | −0.28 |
| −23.93 | L2 peak | 1.767 | 21.5 | −0.57 |
| −25.0 | Cluster inner | 1.129 | 52.7 | +0.06 |
| Cluster | T (keV) | (10¹³ M☉) | (10¹³ M☉) | (10¹³ M☉) | / | / | Δ | Pass |
|---|---|---|---|---|---|---|---|---|
| Coma | 8.2 | 95.5 | 679 | 650 | 7.11 | 6.80 | 4.5% | ✓✓ |
| Perseus | 6.8 | 20.6 | 97.0 | 60.0 | 4.70 | 2.91 | 62% | ✓ |
| Virgo | 2.4 | 38.6 | 253 | 120 | 6.55 | 3.11 | 111% | ✓ |
| A2029 | 8.5 | 28.4 | 128 | 80.0 | 4.49 | 2.81 | 60% | ✓ |
| A2142 | 9.1 | 38.6 | 152 | 90.0 | 3.94 | 2.33 | 69% | ✓ |
| A521 | 5.9 | 31.0 | 96.8 | 45.0 | 3.12 | 1.45 | 115% | ✓ |
| Test | CDM (fitted) | CDM (predicted) | MOND | Verlinde EG | GERT VI |
|---|---|---|---|---|---|
| Cosmological background (CMB+BAO) | Passes | Passes | Not applicable | Fails [21] | Passes () |
| Galaxy rotation curves | Passes (2–3 params/galaxy) | Mixed/limited with fixed c– | Passes | Passes [18] | Passes (6/6, 0 params) |
| RAR scatter reduction | Weak/no clear reduction | Weak/no clear reduction | Qualitative | Qualitative | quantitative |
| BTFR slope = 4 | Tuned via halo fit | Not guaranteed | Built in (interp.) | Asserted | Derived (Eq. 12) |
| BTFR amplitude | Tuned by halo parameters | Dependent on cosmology+halo relation | Fits | Fits | 11% from (0 params) |
| Cluster mass ratios | Tuned with halo model | Typically short without extra freedom | Fails ( short) | Fails [19,20] | Passes (6/6) |
| Coma cluster vs lensing | Fit-dependent | Not robustly predicted | Fails | Fails | 4.5% agreement |
| Milgrom coincidence | Does not derive | Does not derive | Postulates | Asserts | Derives |
| Free parameters (local) | 2–3 (halo) | 0 at galaxy level (if fixed relation) | 1 () | 0 | 0 |
| Connected to cosmos | Yes (global fit) | Yes (global priors) | No | No | Yes (same MCMC fit) |
| Prediction | Observable | Test dataset | Distinguishes from |
|---|---|---|---|
| BTFR scatter correlates with halo | σ(BTFR) vs mean halo density | Full SPARC (175 galaxies) | MOND (no prediction) |
| Compact galaxy (g > a₀, ≈ −23.93) receives GERT correction | Rotation curve excess | High-σ compact galaxies | MOND |
| Ultra-diffuse galaxy (g < a₀, ≪ −23.93) receives no correction | Flat outer curve | UDG sample | MOND |
| Cluster success without extra DM | / ≈ 5 for relaxed clusters | Chandra/eROSITA | MOND, Verlinde |
| BCG stellar mass shifts cluster ratios 10–20% | / with BCG | Perseus, Virgo | Open |
| M-T slope recovers 1.5 for -matched sample | Slope vs selection | Chandra archive | Open |
| System | range | Character | Status | |
|---|---|---|---|---|
| Solar System, stars | > −17 | S ≈ 1.8×10⁻⁸; ν ∼ 10⁻⁸ | Correction < 10⁻¹² | ✓ by construction |
| Molecular clouds | −18 to −15 | S ≈ 0 | Newton approx. | ✓ tested |
| Galactic discs | −20 to −22 | Small | Small correction | ✓ tested |
| Galactic halos | −22 to −24 | Large | Dark matter regime | ✓ tested (SPARC) |
| Galaxy clusters | −24 to −25 | Large | Mass excess ×5 | ✓ tested (6 clusters) |
| Cluster outskirts | −25 to −26 | Moderate | Near transition | Predicted, not yet tested |
| Cosmic web filaments | < −26 | Gas term | Ultra-dilute regime | Paper I [1] regime |
| Test | Scale | Result | Free parameters |
|---|---|---|---|
| Solar System | 1 AU | Correction < 10⁻¹² (double suppression) | 0 |
| 6 SPARC rotation curves | 1–80 kpc | 6/6 improved; RAR scatter −37.5% | 0 |
| BTFR exponent | All galaxies | 4 (exact, analytic derivation) | 0 |
| BTFR amplitude | All galaxies | 11% of observed | 0 |
| 6 galaxy clusters | 0.1–1.5 Mpc | 6/6; / ∈ [3.1, 7.1] | 0 |
| Coma cluster (benchmark) | 1.3 Mpc | 4.5% agreement with weak lensing | 0 |
| Milgrom coincidence | All scales | = 0.935 a₀ (derived from H₀) | 0 |
| Script | Equation | Role in paper | Figures |
|---|---|---|---|
| gert_p5_numerics.py | Paper V [5] | Verification of Paper V [5] results | — |
| gert_local_v01.py | Multiplicative + α free | v0.1: reveals α trend with M★ | 1–3 |
| gert_local_v02_sparc.py | Multiplicative + SPARC | Diagnoses need for additive form | 4–6 |
| gert_local_v03.py | Additive + | Discovery of = cH₀/2π | 7–9 |
| gert_local_v04.py | Final Equation (6) | 6/6 galaxies, RAR −37.5%, 0 params | 10–11 |
| gert_btfr.py | BTFR analytic limit | Derives slope = 4; 18 galaxies | 12–13 |
| gert_clusters.py | Cluster mass integral | 6 clusters; R = 0.938 | 14–15 |
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