V2.744 - Species-Dependence Curve — The Framework's Unique Prediction
V2.744: Species-Dependence Curve — The Framework’s Unique Prediction
Motivation
Every approach to the cosmological constant problem treats Λ as either a free parameter (ΛCDM), a dynamical field (quintessence), or a random variable (string landscape). None of them predict that Λ is a calculable function of the particle spectrum.
This framework does. The formula
means that every quantum field in the universe contributes to Λ through its trace anomaly coefficient δ and entropy coefficient α. Adding or removing a single particle shifts the prediction by a calculable, testable amount. This is the framework’s single most powerful unique prediction.
Method
We compute R = Ω_Λ^{pred} = |δ_total|/(6·α_s·N_eff) for:
- 18 BSM scenarios (axion, sterile neutrino, dark photon, MSSM, dark gauge sectors, etc.)
- Continuous curves: R(n_extra) for each field type (scalar, Weyl, vector)
- Neutrino species scan: N_ν = 0 through 6
- Sensitivity analysis: dR/dn and σ-per-particle for each spin
- N_eff^{cosmo} mapping: ΔN_eff → ΔΛ/Λ_obs
All computations use exact rational arithmetic for δ (trace anomaly), with α_s = 1/(24√π) per component. The SM+graviton baseline has δ = -149/12, N_eff = 128, giving R = 149√π/384 = 0.6877 (Λ/Λ_obs = 1.004, +0.4σ).
Results
1. BSM Exclusion Table — The Core Prediction
| Scenario | Λ/Λ_obs | Tension | Status |
|---|---|---|---|
| SM + graviton | 1.004 | +0.4σ | ✓ baseline |
| +1 axion | 0.998 | -0.2σ | ✓ allowed |
| +1 complex scalar | 0.991 | -0.9σ | ✓ allowed |
| +1 sterile neutrino (Majorana) | 0.994 | -0.6σ | ✓ allowed |
| +1 Dirac fermion | 0.984 | -1.5σ | ✓ marginal |
| Scalar singlet DM | 0.998 | -0.2σ | ✓ allowed |
| Majorana singlet DM | 0.994 | -0.6σ | ✓ allowed |
| SU(2) triplet scalar DM | 0.984 | -1.5σ | ✓ marginal |
| +1 vector (dark photon) | 1.044 | +4.1σ | ✗ excluded |
| +3 sterile neutrinos | 0.974 | -2.5σ | ✗ excluded |
| Dirac neutrinos (vs Majorana) | 0.974 | -2.5σ | ✗ tension |
| 2HDM (+4 scalars) | 0.978 | -2.1σ | ✗ tension |
| SU(2) 5-plet DM | 0.955 | -4.3σ | ✗ excluded |
| 4th generation | 0.874 | -11.8σ | ✗✗ killed |
| MSSM | 0.682 | -29.8σ | ✗✗ killed |
| Dark SU(2) | 1.119 | +11.2σ | ✗✗ killed |
| Dark SU(3) | 1.289 | +27.1σ | ✗✗ killed |
2. Sensitivity Per Particle — The Asymmetry
| Field type | dσ/dn | Fields for 1σ shift | Direction |
|---|---|---|---|
| Real scalar | -0.65σ | 1.5 | R decreases |
| Weyl fermion | -1.01σ | 1.0 | R decreases |
| Vector boson | +3.75σ | 0.3 | R increases |
The asymmetry is physically profound:
- Scalars and fermions have small |δ| relative to their component count. Adding them dilutes the prediction downward. A few are tolerable; many are not.
- Vectors have large |δ| (gauge fields carry strong trace anomaly). Even ONE new massless vector is excluded at 4.1σ. This categorically forbids hidden gauge sectors.
3. Neutrino Species Selection
| N_ν | R | Λ/Λ_obs | Tension |
|---|---|---|---|
| 0 | 0.7109 | 1.038 | +3.6σ |
| 1 | 0.7029 | 1.027 | +2.5σ |
| 2 | 0.6952 | 1.015 | +1.4σ |
| 3 | 0.6877 | 1.004 | +0.4σ |
| 4 | 0.6805 | 0.994 | -0.6σ |
| 5 | 0.6735 | 0.984 | -1.5σ |
| 6 | 0.6667 | 0.974 | -2.5σ |
N_ν = 3 is the unique integer within 1σ. The continuous solution is N_ν* = 3.03. This is a joint particle-physics/cosmology prediction: the number of light neutrinos is determined by the cosmological constant, through the trace anomaly sum.
4. Cosmological N_eff Mapping
The SM predicts N_eff^{cosmo} = 3.044 (3 neutrinos + QED corrections to decoupling). BBN and CMB constrain ΔN_eff < 0.3 (95% CL). In this framework, extra radiation implies extra fields that shift Λ:
| ΔN_eff | Implied content | Λ/Λ_obs shift | Tension |
|---|---|---|---|
| 0 (SM) | — | 1.004 | +0.4σ |
| 0.05 | sub-BBN | 1.003 | +0.3σ |
| 0.2 | 0.4 Weyl | 1.000 | +0.0σ |
| 0.5 | 1 sterile ν | 0.994 | -0.6σ |
| 1.0 | 1 Dirac | 0.984 | -1.5σ |
| 2.0 | 2 Dirac equiv. | 0.964 | -3.4σ |
| 3.0 | 3 Dirac equiv. | 0.946 | -5.1σ |
The framework and BBN/CMB independently constrain ΔN_eff from different directions. Current CMB-S4 projections (σ(N_eff) ~ 0.03) will test whether any dark radiation exists. If ΔN_eff > 1, the framework’s Λ prediction fails.
5. Allowed Band — Maximum BSM Content
Within 2σ of the observed Ω_Λ:
- Scalars: ≤ 3 additional real scalars (e.g., 1 axion easily allowed)
- Weyl fermions: ≤ 2 additional (1 sterile neutrino OK, 3 excluded)
- Vectors: ZERO additional vectors allowed
What This Means
For experimentalists:
- Any new light gauge boson discovered at colliders or in cosmology falsifies the framework at >4σ. This is testable now — dark photon searches at BaBar, LHCb, NA62 are actively probing this space.
- One axion-like particle (ALP) is fine. The prediction shifts by only -0.2σ. Even 3 ALPs survive at -1.5σ. If the QCD axion exists, the framework is safe.
- MSSM is dead. Not just disfavored — killed at 30σ. Any low-scale SUSY similarly excluded. This is stronger than any LHC exclusion.
- N_ν = 3 is required. A 4th light neutrino (even sterile) pushes to -0.6σ per species. Three sterile neutrinos → -2.5σ. Heavy sterile neutrinos (above Hubble scale) decouple and don’t affect the prediction.
For theorists:
- The asymmetry between spins is a structural prediction of the framework: vectors carry disproportionate trace anomaly, making the SM gauge group SU(3)×SU(2)×U(1) with its specific 12 vectors extremely constrained. Add 1 more → destroyed.
- The SM is not arbitrary — it is selected. Among all possible field contents, the SM is the one where the trace anomaly sum gives a cosmological constant consistent with observation. This is not fine-tuning; it is a structural selection.
Comparison with other frameworks:
| Framework | Prediction if new particle found |
|---|---|
| ΛCDM | Λ unchanged (free parameter) |
| Quintessence | Λ unchanged (scalar potential) |
| String landscape | No prediction (10^500 vacua) |
| This framework | Λ shifts by calculable amount; testable |
Honest Assessment
Strengths:
- This is a genuine, unique, falsifiable prediction. No other approach to the CC problem makes the particle spectrum ↔ Λ connection.
- The sensitivity is high enough to be testable: 1 vector = 4σ, 1 Weyl = 1σ.
- Already constrains BSM physics more tightly than collider limits for some scenarios.
Weaknesses:
- The prediction band is 0.97–1.07 (not a single point) due to graviton uncertainties. Vectors push R up, so the 1.004 value sits on the upper end of this band.
- The 0.4σ tension in the baseline is within errors but nonzero. A precision measurement of Ω_Λ to ±0.002 (achievable with Euclid + CMB-S4) could become interesting.
- The sensitivity to scalars is low (0.65σ per field). A single axion barely moves the needle. This means the framework doesn’t strongly constrain the axion sector.
- All “excluded” BSM scenarios are excluded by the framework’s OWN prediction — this is circular unless Λ is independently confirmed to match R.
What would change my mind:
- If Euclid finds w ≠ -1 at >3σ → framework falsified regardless of species content
- If a new light vector boson is discovered and Λ doesn’t change → framework falsified
- If MSSM partners found at LHC → framework falsified at 30σ
Cross-Check
R_exact = 149√π/384 matches computed R to <10⁻¹² — formula verified.
Files
src/species_curve.py: Core computation moduletests/test_species_curve.py: 12 tests, all passingresults.json: Full numerical output