Scope first: By construction, SPSP–SSC matches GR + SM in screened/validated regimes (the paper’s stated domain). Differences can only show up when either (i) screening is imperfect, or (ii) the boundary-value setup for the elliptic sorting field Φ is not satisfied (e.g., during strongly time-dependent horizons). That makes the theory easy to falsify:
Prediction: Because Φ is a non-propagating elliptic constraint (no kinetic term), there is no fifth-force mediator and no −1PN dipole radiation in binaries. Leading radiation remains quadrupolar (GR value), and GWs are luminal in screened domains.
Falsify by:
Prediction: If sources are compactly supported and Φ has homogeneous data on the enclosing surface (A6′), then Φ=0 in the exterior and the outside metric is just GR. Any deviation must come from a failure of those exterior conditions.
Falsify by:
Prediction (screened linear scales): No gravitational slip: ΦNewton−ΨNewton=0. Growth, ISW, lensing match ΛCDM up to O(εscr).
Where differences could appear: On horizon-scale / unscreened domains, deviations scale with a small screening parameter εscr. The pattern is constrained (no new wave mode; any deviation looks like a static constraint leakage, not a propagating scalar).
Falsify by:
Prediction: During rapid horizon growth, if A6′ momentarily fails, there could be tiny, transient near-zone imprints (elliptic, non-radiative) that only modify initial data of ringdown—not the QNM spectrum. No extra polarizations.
Falsify by:
Prediction: Low-energy gauge group SU(3)×SU(2)×U(1) with SM hypercharges (derived via anomaly constraints), one Higgs doublet, and standard one-loop β functions. No light Z′, no extra chiral matter.
Falsify by:
Action S = ∫√-g [R⁄16πG + Lm − Φ(ρ−ε)] with GHY boundary term.
Vary gμν: Gμν = 8πG Tμν in screened domains (A3 fixes the same G).
Vary Φ: ∇2Φ = 4πG(ρ−ε) (no (∇Φ)2 ⇒ non-propagating).
Key: Φ is a constraint, not a field with its own wave equation.
ADM analysis: primary/secondary constraints close; Dirac algebra intact; 2 tensor DOF, no scalar mode.
→ No dipole radiation channel and no fifth force.
With A6′ (compact support + homogeneous boundary data on an enclosing surface), maximum principle for Laplace ⇒ Φ=0 outside.
→ Exterior = GR unless A6′ fails.
Harmonic-gauge linearization: GR propagator; PPN parameters γ=β=1; GW flux pure quadrupole; GW speed = c in screened domains.
SVT: no slip in the screened limit (ΦN−ΨN=0); any deviation is O(εscr) and elliptic-patterned (no extra propagating scalar).
→ Distinguishes this from many modified-gravity models that predict slip or GW damping.
Imperfect screening: define εscr ≡ sup|δP|/Λ4. Any deviation on a given domain is at most O(εscr), with no new wave pole.
Boundary failures (time-dependent horizons): only initial-data tweaks to ringdown; spectrum unchanged.
Assumptions (compact YM factors + one U(1), minimal Higgs doublet, anomaly cancellation) ⇒ unique SM hypercharges and standard one-loop β’s.
→ Any confirmed low-energy extension (light Z′, extra chiral gen) breaks the minimality/anomaly setup used here.
Any anomaly confined to an unscreened, horizon-scale regime that can be quantitatively fit by a small εscr and preserves the “no new propagator” character would be a signal, not a refutation.
TL;DR: In its stated domain, SPSP–SSC deliberately reproduces GR + SM. It differs from many alternatives by predicting no extra mode, no slip, no GW damping—and gives a tight falsifier list: any fifth force, dipole radiation, non-luminal GWs, PPN γ,β≠1, linear-scale slip, or new low-energy gauge content would rule it out under its assumptions. The “research notes” above show how each claim follows from the constraint nature of Φ, the boundary-value result, the ADM DOF count, and the anomaly-based SM construction.