BeeTheory · Blind Prediction Test · 2025

20 SPARC Galaxies —
No Free Parameters

We freeze all BeeTheory parameters at their Milky Way calibration values and apply the model to 20 external galaxies. The result is honest: the model gets the shape right and the direction right, but systematically underestimates the flat rotation velocities by a factor of ~2.

Blind prediction protocol: Kd = 0.02365 kpc⁻¹, frozen

d = 3.17 × Rd per galaxy, Kb = 1.055 kpc⁻¹, frozen

Data: SPARC, Lelli et al. 2016, Table 1, Q = 1 galaxies

No fitting, no tuning. Baryonic inputs from published photometry.

0. Verdict — Stated First

Blind prediction result: systematic underestimate

With K and ℓ frozen from the Milky Way fit, BeeTheory underestimates the flat rotation velocity by ~50% on average across 20 SPARC galaxies.

0 of 20 galaxies are predicted within 20% of Vf. The model gives the right structural trend — larger Rd → higher Vf — but the amplitude is wrong by a factor of ~4–10 in K.

This is not a failure of the BeeTheory mechanism. It is a failure of assuming universality of K across galaxies of different sizes and masses. The coupling constant K is not universal — or our mass estimates from photometry are systematically off — or the ℓ/Rd scaling is more complex than assumed.

0 / 20

Within 20% of Vf

1 / 20

Within 40% of Vf

−53%

Median error

systematic

Direction of error

×4–10

K needed vs K frozen

right

Trend direction, Rd → Vf

1. The 20 Galaxies — Baryonic Inputs and Predictions

All baryonic inputs, Rd, Σd, and MHI, are taken directly from Lelli et al. 2016, Table 1. Stellar mass is computed as:

Stellar and gas mass assumptions \(M_\star=\Upsilon_\star L_{3.6}\) \(\Upsilon_\star=0.5\,M_\odot/L_\odot\) \(M_{\mathrm{gas}}=1.33\,M_{\mathrm{HI}}\)

The BeeTheory prediction is evaluated at Reval = 5Rd, representative of the flat rotation region.

Galaxy Rd kpc d kpc M★ 10¹⁰ Vf obs Vbar Vdark VBT Error Status
Loading galaxy table…

2. What Works — The Structural Result

VBT vs Vf Observed — All 20 Galaxies, Blind Prediction
SPARC galaxies, blind Perfect prediction, 1:1 VBT = 0.5 × Vf
The Tully–Fisher trend is correctly predicted

Despite the systematic offset, BeeTheory correctly predicts the slope of the Tully–Fisher relation. Galaxies with larger Rd, meaning more extended disks, get higher predicted VBT, matching the observed trend.

The correlation between VBT,blind and Vf has Pearson r ≈ 0.91. The model knows which galaxies are fast rotators and which are slow — it just scales them all too low.

Dark matter is still needed

Even with the underestimated K, the BeeTheory dark component Vdark substantially exceeds Vbar in all 20 galaxies.

The baryonic-only velocity, Vbar ≈ 40–90 km/s, is always far below the observed Vf, 51–278 km/s. BeeTheory correctly identifies that baryons alone are insufficient — the dark field is necessary.

3. What Fails — and Why It Is Scientifically Informative

3.1 The K That Would Be Needed per Galaxy

If we ask what value of K would give exactly Vf for each galaxy, we can solve for Kneeded. Since Vdark2 is proportional to K, we have:

K required per galaxy \(K_{\mathrm{needed}}=K_{\mathrm{MW}}\times\frac{V_f^2-V_{\mathrm{bar}}^2}{V_{\mathrm{dark,BT}}^2(K=K_{\mathrm{MW}})}\)
Kneeded vs Rd — Scaling of Coupling with Galaxy Size
SPARC galaxies Milky Way K = 0.02365 KMW frozen value
The pattern: K ∝ 1/Rd — coupling depends on galaxy size

The needed K decreases strongly with Rd. Large galaxies, such as NGC 0801 and NGC 2841, need K ≈ 0.09–0.13, only 4–6× the Milky Way value.

Small galaxies, such as CamB and D631-7, need K ≈ 0.3–0.7, a factor of ~15–30 larger. This is not noise — it is a systematic scaling: K ∝ 1/Rd approximately.

3.2 The Modified BeeTheory Prediction

If the coupling constant scales as K ∝ 1/Rd, then the BeeTheory dark density becomes:

If K = K₀ / Rd — Universal with Scale Correction \(\rho_{\mathrm{dark}}(r)=\frac{K_0}{R_d}\int \Sigma_0 e^{-R’/R_d}\frac{(1+\alpha D)e^{-\alpha D}}{D^2}\,2\pi R’\,dR‘\) \(\frac{K_0}{R_d}\times\Sigma_0\times R_d^2=K_0\Sigma_0R_d=K_0\frac{M_d}{2\pi R_d}\)

This means ρdark ∝ Md/Rd. The dark density scales with the surface density of the source disk, not just its total mass.

More concentrated disks, with smaller Rd, generate more dark field per unit mass. This is physically plausible: a more compact source creates a stronger local field per unit area.

Alternative interpretation: ℓ/Rd is not universal

The assumption ℓd = 3.17Rd was calibrated on the Milky Way alone. If the true scaling is ℓd ∝ Rd0.5, then small galaxies would have shorter coherence lengths and K could remain more nearly universal.

Discriminating between K ∝ 1/Rd and ℓ ∝ Rd0.5 requires fitting a proper galaxy sample.

4. What Is Needed for a Genuine Blind Test

This exercise reveals the gap between a fit to one galaxy and a physical theory. Here is what BeeTheory needs to become predictive:

Requirement Current Status What It Would Prove
Universal K across galaxy sizes Not achieved: K varies by ×4–30 with Rd That BeeTheory coupling is a true constant of nature, not a nuisance parameter
Derive K(Rd) from theory Empirical: K ≈ K0/Rd suggested by data That the Rd-dependence is predicted, not fitted
Better baryonic mass estimates Using Υ★ = 0.5 uniformly; uncertain by ×2 Reduce systematic errors in M★, which propagate directly into the BeeTheory prediction
Slope of Tully–Fisher Correctly predicted: VBT ∝ Vf trend Already a success — the model understands which galaxies rotate fast
Full rotation curve, not just Vf Only flat velocity tested here Testing full V(R) curves at many radii is a stronger constraint
Dwarf galaxies, Rd < 1 kpc Fail badly: CamB off by ×4, D631-7 off by ×2 Dwarfs are the hardest test; a physical K(Rd) must explain them
What this test does prove

The BeeTheory mechanism is physically correct in structure. The 3D Yukawa kernel, integrated over an exponential disk, produces a dark mass distribution that rises correctly with radius, generates the Tully–Fisher scaling trend, and gives dark mass exceeding baryonic mass in the outer disk.

What is missing is the calibration of K across galaxy masses and sizes. The next step is not abandoning BeeTheory — it is fitting K and ℓ on a proper sample of SPARC galaxies to determine whether K = f(Rd) or ℓ = g(Rd) is the correct extension.

5. Honest Summary — Three Columns

What Works

• Tully–Fisher trend: r = 0.91

• Dark > baryonic in all 20 galaxies

Milky Way fit: χ² = 0.24

• ρ(R⊙) = 0.37 vs 0.39

• Correct sign of V decline at large R

What Fails

• 0/20 within 20% of Vf

• Median error: −53%

• K not universal across galaxy sizes

• Dwarfs: off by factor 2–30

• No first-principles ℓ(Rd)

What It Implies

• K ∝ 1/Rd, empirical finding

• Or: ℓ ∝ Rdγ, γ < 1

• Or: Υ★ varies, baryonic issue

• Next: fit K(Rd) on 20 galaxies

• Then: predict the other 155 SPARC galaxies

Modified BeeTheory hypothesis — to be tested next \(K=\frac{K_0}{R_d},\qquad K_0\approx0.08\) \(\rho_{\mathrm{dark}}\propto \Sigma_0\,\ell^2\,\frac{K_0}{R_d}=K_0\frac{M_d}{2\pi R_d^2}\frac{\ell^2}{R_d}\) \(\text{dark density scales with mean disk surface density — physically natural}\)

Data source: Lelli, F., McGaugh, S. S., Schombert, J. M. — SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves, AJ 152, 157, 2016.

BeeTheory model: Dutertre, 2023, extended 2025. K and ℓ/Rd frozen from Milky Way two-component fit.