Self-as-an-End
SAE Cosmological Physics Series · Paper VI

An Aether-Scalar-Tensor Structure for the Dark Sector from Dual-4DD Breathing
从 Dual-4DD 呼吸导出暗扇区的 Aether-Scalar-Tensor 结构

Han Qin (秦汉) · Independent Researcher · 2026
DOI: 10.5281/zenodo.21267555 · Full PDF on Zenodo · CC BY 4.0
Abstract

We derive, from the dual-4DD breathing structure of the Self-as-an-End (SAE) framework, the structural constraints on an aether-scalar-tensor action for the dark sector. Two four-dimensional timelike sectors (4DD) with nearly antiparallel time orientation each carry a breathing clock, τ₁ and τ₂; their symmetric combination τ_breath = (τ₁+τ₂)/2 acts as a khronometric aether and their antisymmetric combination C = τ₁−τ₂ as a DBI scalar. Three dark-sector effects are thereby placed in a single structure, with no particles: the khronon yields geometric dust (dark matter) through Mukohyama's "dark matter as an integration constant" mechanism; DBI-C yields intrinsically non-phantom dynamical dark energy together with MOND; and a 4-form field strength yields the cosmological constant Λ, with Λ₁+Λ₂ = 0 as one instance of a remainder-conservation axiom. The tensor-mode speed c_T = 1 follows from SAE's universality of c and is consistent with GW170817.

We then revise the MOND acceleration a₀ from an earlier vacuum scale to a horizon scale: with gravity read as information read-out, a galactic core feels the noise floor of the cosmic horizon flushing causal information, giving a₀ ∝ c²/R_A (apparent horizon), and a₀ ∝ cH in the flat limit. Two falsifiable hard predictions follow. (HP1) A redshift scaling of a₀, a₀(z)/a₀(0) ≃ H(z)/H₀, which at z ≳ 3 differs from constant-a₀ by more than a factor of four. (HP2) An intrinsic dark-energy equation of state w_int(z) ≥ −1: SAE dark energy does not cross the phantom divide. Both predictions can be adjudicated by current and near-term data. We state the remainders openly: the dust abundance Ω_d, the coupling g, the khronometric parameters, and the absolute value of the a₀ coefficient (limited by a systematic floor, unmeasurable to the precision that would distinguish 1/2π from nearby values) are posterior or motivated preferences rather than completed derivations; whether the projectable version (dust) and the non-projectable version (c_T = 1) of Hořava gravity can coexist is a foundational open problem.

Our methodological stance runs throughout: the current dark-sector programme absorbs anomalies at the parameter level with free parameters and is therefore hard to falsify; SAE instead trades structural constraint for falsifiability, issuing hard predictions that can be adjudicated, and — if falsified — pointing to where the prior must be revised.

1. Introduction

Dark matter, dark energy, and MOND phenomenology — the three pieces of the dark sector — are treated independently in the standard programme: cold dark matter is a particle, dark energy is a constant or an extra scalar field, and MOND is an empirical acceleration relation. Each carries its own free parameters and fits its own observations.

This paper places all three in a single structure, and introduces no dark-matter particle. The structure comes from SAE's dual-4DD picture: two four-dimensional timelike sectors with nearly antiparallel time orientation, each carrying a breathing clock τ₁, τ₂. Their symmetric combination τ_breath = (τ₁+τ₂)/2 acts as a khronometric aether; their antisymmetric combination C = τ₁−τ₂ acts as a DBI scalar. From these, the khronon supplies geometric dust that serves as dark matter, DBI-C supplies dynamical dark energy and MOND, and a 4-form field strength supplies the cosmological constant; the conservation laws of all three reduce to a single remainder-conservation axiom.

This paper follows the SAE cosmology series: Cosmo I gives the cosmological constant Λ = 2(ω₂²−ω₁²)/c², Cosmo II/III give the MOND acceleration a₀ and the geometric origin of its 3/2 power, Cosmo IV treats the effective gravitational constant, and Cosmo V proposes the C field as dynamical dark energy. Here we assemble these into a single modified-gravity action of the aether-scalar-tensor type — narrowing one free function of that class into two terms with structural origins — completing three sub-goals (the khronon's Mukohyama dust, the tensor speed c_T = 1, and the cosmological constant Λ₁), and revising a₀ from an earlier vacuum scale to a horizon scale.

The value of this structure lies not in its ability to fit existing data — there is no shortage of models that fit dark-sector data — but in its constraints on functional form, and in the falsifiable predictions those constraints entail. SAE's prior restricts the form of the action, not merely its parameters: the DBI kinetic term follows from the Nambu-Goto action of a brane rather than being chosen freely; the 3/2 power of the spatial term follows from the p = d = 3 theorem in three dimensions rather than being fit; the conservation laws follow from an axiom rather than being inserted as initial conditions; and c_T = 1 follows from the universality of c, confirmed by GW170817. It is these constraints that let the framework issue hard predictions the standard cold-dark-matter-plus-cosmological-constant model (ΛCDM) cannot — predictions that pin the framework down: an intrinsic dark-energy equation of state w_int ≥ −1 (dark energy structurally does not cross the phantom divide), and a redshift scaling of a₀ (a₀ grows with the horizon, differing from constant-a₀ by more than a factor of four at z ≳ 3). Both can be adjudicated by current and near-term observation.

This is a deliberate trade-off. A model with enough freedom fits almost any data, and fitting everything is equivalent to excluding nothing: it is precise but unfalsifiable, and therefore cannot be adjudicated or renewed. A framework whose structure is constrained by a prior, by contrast, has no room for post-hoc parameter adjustment and can only make hard predictions — much as general relativity, with almost no free parameters, made predictions like light bending and gravitational waves that were computed before they were measured. The two hard predictions of this paper are of this kind: they can be falsified, and that is the point; if falsified, the falsification itself indicates where the prior must be revised.

The remaining quantities — the dust abundance Ω_d, several couplings and khronometric parameters, the absolute value of the a₀ coefficient — are set by observation or boundary conditions, just as the gravitational constant in general relativity or the mass spectrum in the standard model. Throughout, we label prior-derived structural constraints, posterior-set values, and unresolved open problems separately.


2. The dual-4DD breathing structure

We summarize what is needed; full derivations are in the SAE foundations and in Cosmo I–V.

Two four-dimensional timelike sectors (4DD) coexist with nearly antiparallel time orientation and a slight symmetry breaking, parametrized as $$\varepsilon = \frac{\omega_2-\omega_1}{\omega_2+\omega_1} \approx 0.0127,$$ where ω₁, ω₂ are the frequencies of the sectors' breathing clocks τ₁, τ₂. The hard parameters are taken as T₁ = 20 Gyr, T₂ = 19.5 Gyr (SAE inputs, not re-estimated here).

The key decomposition combines the two clocks into $$\tau_{\rm breath} = \frac{\tau_1+\tau_2}{2}\ (\text{symmetric}),\qquad C = \tau_1-\tau_2\ (\text{antisymmetric}).$$ The symmetric combination τ_breath defines the normal to the causal foliation and acts as a khronometric aether; the antisymmetric combination C is a dynamical scalar. The two are not independent fields but two combinations of the same pair (τ₁, τ₂) — a point that matters in §6 when we discuss coupling.

Two established structural results (see the T2 working record) are used here. First, C is non-compact: the speed of light bounds the misalignment rate Ċ itself, and this bound is unreachable within a 4DD (it is a relativistic ceiling, not a channel to a fifth dimension), so C accumulates along the timelike direction without winding, and shift symmetry C → C + const forces U(C) = const. Second, there is a single light cone: the two 4DD share one c, and opposite time orientation means they correspond to the two directions of one cone rather than to two metrics. This structurally forbids the dangerous bimetric/disformal couplings once envisaged in Cosmo V; the "two-metric reconstruction" is thereby fixed as an aether-scalar-tensor reconstruction, by structure rather than by choice, and this is also a prerequisite for passing GW170817.


3. The action and its commitment layering

3.1 Template and SAE's narrowing

We take the aether-scalar-tensor action of Skordis–Złośnik (2021) as a template: $$S_G = \int d^4x\, \frac{\sqrt{-g}}{2\kappa}\Big[R - 2\Lambda - \tfrac{K_B}{2}F_{\mu\nu}F^{\mu\nu} + 2(2{-}K_B)J^\mu\nabla_\mu\phi - (2{-}K_B)\mathcal{Y} - \mathcal{F}(\mathcal{Y},Q) - \lambda(A^\mu A_\mu{+}1)\Big] + S_m[g],$$ with $Q = A^\mu\nabla_\mu\phi$, $\mathcal{Y} = (g^{\mu\nu}{+}A^\mu A^\nu)\nabla_\mu\phi\nabla_\nu\phi$, $J_\mu = A^\nu\nabla_\nu A_\mu$, $F_{\mu\nu} = \nabla_\mu A_\nu {-} \nabla_\nu A_\mu$. Matter couples to a single metric g (satisfying the equivalence principle), and the aether kinetic term is of Maxwell form.

AeST leaves $\mathcal{F}(\mathcal{Y},Q)$ a free function. SAE's narrowing fixes it at both ends: $$\boxed{\ \mathcal{F}_{\rm SAE}(\mathcal{Y},Q) = 2T\big[\sqrt{1-Q^2/c^2}-1\big] + M_Y^4\, y^{3/2}\ }$$ The time part is of DBI (tachyon) form, derived from the Nambu-Goto action of a brane (§4.2); the 3/2 power of the spatial part follows from the p = d = 3 theorem (§4.2, §5). This is SAE's core structural gain over AeST: a free function reduced to two terms with structural origins.

We take the scalar φ = C (the antisymmetric combination) and the aether $A_\mu = -N\nabla_\mu\tau_{\rm breath}$ (hypersurface-orthogonal, i.e. khronometric), with $Q_c = c$ as a prior (from the c-ceiling of §4.2).

A sign convention should be fixed to avoid mismatch with the $w_C$ derivation below. Here $\mathcal{F}_{\rm SAE}$ follows the AeST template convention, in which the action contains $-\mathcal{F}$; the DBI subterm therefore contributes $-2T[\sqrt{1-Q^2/c^2}-1]$ to the action, its physical Lagrangian has the form $-\sqrt{1-Q^2/c^2}$ (the brane derivation of §4.2), and the constant $+2T$ is absorbable — into $\Lambda_{\rm 4form}$ or by a zero-point subtraction. The factor of 2 in $2T$ comes from the template's $(2-K_B)$ normalization of the $\mathcal{Y}$ term, matching the DBI term to the $\mathcal{Y}$ term in the weak-field expansion. The $w_C = q^2 - 1$ of §4.2 uses the physical DBI stress-energy tensor, not the sign of $\mathcal{F}$ itself.

3.2 Consistency of the spatial scale: α is not a free constant

The MOND acceleration a₀ is precisely the normalization scale of the quasi-static $\mathcal{Y}^{3/2}$ term. If the coefficient of that term were a constant α, then a₀ would be constant, contradicting the a₀ ∝ H(z) of §5. We therefore do not write the spatial term with a constant coefficient $\alpha\mathcal{Y}^{3/2}$, but write the horizon scale into the non-dimensionalization: $$y \equiv \frac{\mathcal{Y}}{a_0(\tau)^2},\qquad a_0(\tau) = \frac{c^2}{2\pi R_A(\tau)},$$ where R_A(τ) is the apparent horizon (§5). The power 3/2 is fixed by p = d = 3, and the scale a₀(τ) is supplied by the horizon sector. The MOND normalization of §3 and the horizon a₀ of §5 are then the same a₀(τ), and the two are consistent.

This writing requires one remark at the level of the variation, or it would introduce higher derivatives. Since $a_0(\tau) \propto R_A^{-1} \propto H$ and $H = \dot a/a$ contains a time derivative of the metric, varying $a_0(\tau)$ together with the metric in the local field equations ($\delta S/\delta g_{\mu\nu}$) would produce Ostrogradsky-type higher-derivative (ghost) terms. Our position on this is consistent with the physical origin of a₀ (§5): $a_0(\tau)$ is the information read-out noise floor set by the global causal horizon, and in the local (galactic-scale) variation it is treated as an external evolving background that does not participate in the local metric variation — the back-reaction of local matter is too small to shift the horizon noise floor, so no higher-derivative variation term arises. Correspondingly, the spatial term containing $a_0(\tau)$ is not a complete covariant local Lagrangian but an effective term normalized by the horizon read-out on an FLRW background; its full covariantization (expressing $R_A^{-1}$ as a foliation-invariant local geometric scalar — the aether expansion $\theta = \nabla_\mu A^\mu = 3H$, spatial curvature, or another, e.g. $a_0(\tau) \simeq c\theta/6\pi$ in the flat approximation) is left as an open problem.

3.3 Separating the baseline action from the coupling branch

The baseline action and an optional interaction branch are listed separately. The baseline action contains no khronon–C mixing term: $$S_{\rm base} = S_{\rm grav}[g,A] + S_{\rm DBI\text{-}C}[C,A] + S_{Y}[C,A] + S_{\rm 4form} + S_m[g].$$ There is a further term $$S_{\rm mix} = g\int d^4x\,\sqrt{-g}\,\theta Q,\qquad \theta = \nabla_\mu A^\mu,$$ which is not part of the baseline, but an open interaction branch (see §6, HP2, layer 2); its coupling g is a free Wilson coefficient, not a number fixed by the dual-4DD structure. This separation is necessary to keep "intrinsic w ≥ −1" (a baseline result) distinct from "effective crossing" (a g-dependent optional branch).

3.4 Commitment layering

Labeling each term's status is required by SAE's honesty. The table below both guards against overstating the derivation of structural constraints as a full numerical derivation, and acknowledges the prior constraints that are genuinely present — constraints that ΛCDM/AeST do not have.

Term SAE status Free coefficient Observational role
$R - 2\Lambda_{\rm 4form}$AeST template + prior 4-form formΛ₁ value posteriorconstant part of dark energy
DBI time term $\sqrt{1-Q^2/c^2}$prior (brane-derived)tension T posteriordark energy, w_int ≥ −1
spatial term $y^{3/2}$power prior (p = d = 3)scale = horizon a₀(τ)MOND / a₀
khronon aether (HSO)prior (breathing foliation normal)α, λ posteriordark matter (Mukohyama dust)
$-\tfrac{K_B}{2}F^2$AeST templateK_B posterioraether kinetic (c_T = 1)
$S_{\rm mix} = g\theta Q$open interaction branch (non-baseline)g free WilsonHP2 effective crossing (undetermined)

The prior-derived items (single metric, c_T = 1, DBI form, y^{3/2} power, the conservation laws) are structural constraints, not values; the posterior items (Λ₁ value, T, K_B, α, λ) are on the same footing as G measured in general relativity or the nineteen parameters measured in the standard model, and do not detract from this being a framework with structural constraints.

Three interfaces should be made explicit. C is a dynamical scalar (with its own equation of motion, contributing ρ_C(z)), not a pure background quantity. HSO = khronometric is a choice SAE fixes, and it is precisely the interface of the version tension between §4.1 (dust) and §4.4 (c_T = 1). Relative to AeST, SAE fixes the two terms of $\mathcal{F}$ and $Q_c = c$, and leaves K_B, T, α, λ undetermined.


4. The three objects

4.1 Khronon → dark matter (Mukohyama integration-constant dust)

The HSO aether reduces the gravitational sector, in the infrared, to projectable Hořava–Lifshitz gravity. Consider its vacuum FRW dynamics (flat, unit lapse). Varying the scale factor gives the acceleration equation $$3(1-3\lambda)(2a\ddot a+\dot a^2) + 6\Lambda a^2 = 0,$$ which has a first integral (sign check: $\tfrac{d}{dt}[3(1-3\lambda)a\dot a^2+2\Lambda a^3] = \dot a \times$ the acceleration equation, conserved exactly): $$3(1-3\lambda)a\dot a^2 + 2\Lambda a^3 = \mathcal{C}\quad\Longrightarrow\quad H^2 = \frac{\mathcal{C}/a^3}{3(1-3\lambda)} - \Lambda_{\rm eff}.$$ Even in vacuum (no matter of any kind), a term $\rho_d = \mathcal{C}/a^3$ appears — a pressureless dust. This is precisely Mukohyama's (2009) "dark matter as an integration constant": the Hamiltonian constraint of the projectable version is global (a spatial integral) rather than local, and this looser constraint lets dust emerge as an integration constant, whose classical solution mimics general relativity plus cold dark matter. The dust need not be promoted to an independent dynamical field; it emerges only when the equations are solved — and is therefore geometric and particle-free.

Epistemology. The scaling $\rho_d \propto a^{-3}$ is a structural consequence of the first integral, one instance of the remainder-conservation axiom (prior); the abundance Ω_d is the integration constant, set by conditions in the very early universe (posterior). This agrees, independently, with the earlier result from the brane shift charge (conservation prior, value posterior). The posterior status of the abundance is on the same footing as Ω_c determined by observation in ΛCDM, or the dust fraction as a free initial value in AeST; what is distinctive to SAE is the geometric (rather than particle) ontology of the dust and the axiomatic origin of its conservation. This dust term is precisely the $A_m/a^3$ already used in Cosmo III. The effective gravitational coupling is $G_{\rm eff} \propto 1/(1-3\lambda)$. Positivity of the dust (ρ_d > 0 and G_eff > 0) requires $(1-3\lambda) > 0$, i.e. λ < 1/3, which is off the general-relativity limit λ = 1; the observational viability of this regime belongs to the khronometric α, λ parameter-space open problem listed below.

Version tension. Mukohyama dust arises in the projectable Hořava theory (lapse depending on time only, global constraint), and the projectable version has a known problem — an extra scalar graviton mode that is a ghost or strongly coupled at low energy (Blas–Pujolàs–Sibiryakov). The c_T = 1 / healthy structure of §4.4 belongs to the non-projectable (khronometric) version. These are different Hořava versions; the literature (e.g. MNRAS 2023) notes that realizing cold-dark-matter-like behaviour in the non-projectable version is not automatic ("if one can"). Whether one can simultaneously have Mukohyama dust (projectable) and the healthy khronometric structure (non-projectable) is therefore an unresolved structural problem, not a settled fact; the stability of the dark-matter sub-goal's foundation depends on it. §7 and the open-item list mark this as a foundational open problem.

4.2 DBI-C → dark energy and MOND

Substituting the decomposition into $Q = A^\mu\nabla_\mu C$, the cross terms cancel and $$Q \propto |\nabla\tau_1|^2 - |\nabla\tau_2|^2 \propto \omega_2^2-\omega_1^2 \propto \Lambda,$$ so the time kinetic energy of C is of order Λ (small). In the DBI form, the equation of state $w_C = q^2 - 1$ ($q = Q/c$) is slightly above −1 — C is dark energy, consistent with Cosmo V.

The brane derivation of the DBI form (prior, not analogy). The worldvolume action of C is of Nambu-Goto type, $\mathcal{L} = -T\sqrt{-\det(g+\partial C\partial C)/\det g} = -T\sqrt{1+g^{\mu\nu}\partial_\mu C\partial_\nu C}$; the determinant of the induced metric gives $\det h/\det g = 1-\dot C^2/c^2$, so the time part is $-T\sqrt{1-Q^2/c^2}$. This is not a chosen function but a consequence of brane geometry; the dual-4DD has an embedded brane structure (time arrows reversed but not exactly 180°, with a symmetry breaking). $Q_c = c$ is a prior.

The structural bound (hard). Since $w_C = q^2 - 1 \ge -1$ ($q^2 \ge 0$), together with a positive 4-form Λ₁ (w = −1), the total dark energy satisfies $w_{\rm int} \ge -1$. This is the standard non-phantom property of tachyon/DBI, a hard structural theorem rather than a fit — see §6, HP2.

MOND (the spatial part). The spatial term $y^{3/2}$ gives the AQUAL structure in the quasi-static, deep-MOND limit; the 3/2 power follows from the p = d = 3 theorem in three dimensions (3/2 = 3DD ÷ 2), and the normalization scale a₀ is supplied by the horizon sector (§5). The baryonic Tully–Fisher relation $v^4 = GM_b a_0$ is a first integral of the nonlinear Poisson equation and is exact.

4.3 4-form → the cosmological constant

The explicit Λ in the action comes from a 4-form gauge field. In four dimensions the field strength is $F_{\mu\nu\rho\sigma} = f\cdot\varepsilon_{\mu\nu\rho\sigma}$, its equation of motion makes f constant, and its stress-energy $T_{\mu\nu} = -\tfrac12 f^2 g_{\mu\nu}$ is proportional to the metric — a cosmological constant $\Lambda_{\rm 4form} = (\kappa/2)f^2$.

The dual-4DD gives two 4-form sectors, with field strengths f₁, f₂, so $\Lambda_1 \propto f_1^2$ and $\Lambda_2 \propto f_2^2$ (opposite sign). Hence $$\boxed{\ \Lambda_1+\Lambda_2 = 0\ }$$ is the remainder-conservation axiom acting on the vacuum (4-form) sector — the same axiom as the khronon dust conservation, and as antimatter B₁+B₂ = 0 and zero energy E₁+E₂ = 0. The observed Λ is the single-sector Λ₁, whose prior form (Cosmo I, dual-face reciprocity) is $\Lambda_1 = 2(\omega_2^2-\omega_1^2)/c^2$ (the "2" being the dual-face factor); its value is posterior (from the measured T₁, T₂), and differs from one breath to the next. In the dual-frame picture (Cosmo V): Λ_total = 0 in the geometric frame, while Λ₁ > 0 in the Jordan frame we inhabit, the two related by the conformal factor A²(C).

Consilience. Both the Λ₁ of the 4-form and the dynamical dark energy of DBI-C are ∝ (ω₂²−ω₁²) — the same breathing-asymmetry scale; together they compose the observed dynamical dark energy.

4.4 The tensor speed c_T = 1

In khronometric gravity the linearized spin-2 tensor perturbation mode has speed $c_t^2 = 1/(1-\beta)$, β being one of the khronometric couplings, so $c_T = 1 \iff \beta = 0$. (SAE's ontology holds that gravity is not a force and that there is no independent graviton particle; here $c_T$ is the propagation speed of the linearized tensor mode, not the speed of a graviton particle.)

In SAE, β = 0 follows from structure rather than tuning. The DD Breakthrough theorem holds that c is defined at the birth of the one-dimensional-time sector, that all DD share one spacetime, and that c is universal; taken seriously, this implies that all propagating modes — including the tensor mode — propagate at the same c on this one shared spacetime, so $c_t = 1$, i.e. β = 0. This is the same universality-of-c axiom as STEP 0 (Ċ bounded by c) and STEP 1 (single light cone) of §2. GW170817/GRB170817A is consistent with this and constrains deviations strongly (|β| < 10⁻¹⁵) — noting that the observation confirms the closeness of the gravitational-wave and light speeds, not the SAE universality-of-c derivation itself. This meets c_T = 1 by a different route than AeST's Maxwell-form $F^2$, but in SAE it is structurally forced rather than a choice of form.

Parameter constraints. c_T = 1 only fixes β. The other two khronometric parameters α, λ are independently constrained (post-Newtonian parameters, pulsars, big-bang nucleosynthesis, absence of Cherenkov radiation); the scalar-mode speed c_s is barely constrained by gravitational waves and is a known soft spot of khronometric gravity. Full parameter viability (α, λ within the intersection of these constraints) is an independent check inherited from khronometric gravity and does not hold automatically.


5. The horizon origin of a₀

5.1 From vacuum scale to horizon scale

Earlier (Cosmo II/III), a₀ = (π/2)c(ω₂−ω₁) was a vacuum scale and constant. But intermediate-redshift data disfavour this: MUSE-DARK III (Ciocan et al. 2026) and MIGHTEE-HI (Vărăşteanu et al. 2025) show a₀ increasing with redshift at z ≲ 1.5 (tentatively, ~2.4σ). This directly contradicts the a₀ decline given by Cosmo III's η(t) factor — a closed-FRW artifact, of the same kind as the C-dust misassignment. The a₀ decline given earlier by Cosmo III's η(t) had the opposite sign to these data; here we revise it to a horizon scaling, and η(t)'s high-redshift decline is not retained. The old form a₀ = (π/2)c(ω₂−ω₁) is reduced to a z = 0 normalization, whose present-matching gives ω₂−ω₁ ≈ H₀/π²; the corresponding update to Cosmo III's text awaits z > 3 data.

5.2 The mechanism: a₀ as the information read-out noise floor of the horizon

The revised picture is SAE-native, and promotes the numerical coincidence a₀ ∼ cH₀ from a coincidence to a structure. SAE's ontology of gravity (the four-force prequel) reads gravity as information read-out: a system's gravitational response corresponds to the information it can read within the causal horizon. What a galactic core feels is the noise floor projected inward as the cosmic horizon continually flushes causal information with expansion. Inverting through an Unruh-type relation, this noise floor corresponds to an acceleration $$a_0 \sim \frac{c^2}{R_A} \sim cH(z),$$ with $R_A$ the apparent horizon. When the Newtonian acceleration from baryons $g_N > cH$, the baryons' "command" overrides the noise floor (the Newtonian regime); when $g_N \le cH$, it is drowned by the noise floor of the expanding horizon (the MOND regime). MOND is then neither dark matter nor a vacuum aether, but the geometric noise floor projected inward as the horizon consumes causal information. This mechanism accounts for the coincidence a₀ ∼ cH₀ (a₀ ∼ cH/2π, with the status of the coefficient discussed in §5.3; today H = H₀) and for the direction of the a₀(z) increase.

5.3 The geometric coefficient and its three-layer status

The numerical coefficient is understood in three layers, whose observational and derivational statuses differ.

Write $a_0 = c^2/(2\pi R_A)$, with $2\pi R_A$ the circumference of the horizon's great circle. Both the radius $R_A$ and the circumference $2\pi R_A$ are lengths, and $c^2/R_A = cH$ (coefficient 1) and $c^2/(2\pi R_A) = cH/(2\pi)$ (coefficient 1/2π) are both dimensionally valid; so 2π is not forced by dimensions, but is the result of the geometric choice to take the circumference rather than the radius. Its justification rests on a "read-out must close" closure-loop principle, which is not yet axiomatically proven (§7 open problem).

The three layers of a₀ are then:

Layer one — the scaling direction (hard prediction). a₀ grows with the horizon ($\propto R_A^{-1}$). This is a falsifiable hard prediction (§6, HP1). The slope cancels systematic error in the ratio and is therefore measurable.

Layer two — the absolute value of the coefficient (not observationally distinguishable). The absolute value of $\chi \equiv a_0/(cH_0)$ is limited by a systematic floor. The initial-mass-function uncertainty in the mass-to-light ratio is about 20% and is systematic (it does not reduce as $\sqrt N$ with sample size), and the Hubble tension contributes about 8%. To distinguish 1/(2π) = 0.159 from 1/6 = 0.167 requires χ to about 5%, which a pure a₀(z) survey route cannot reach persistently (barring independent breakthroughs in both the initial mass function and the Hubble tension). The absolute value of the coefficient therefore cannot serve as an observationally falsifiable hard prediction; the predictive power of a₀ is in the scaling (slope), not the coefficient (absolute value).

Layer three — the value 1/(2π) of the coefficient (motivated preference, not a completed derivation). Although observation cannot distinguish them, 1/(2π) and 1/6 are not symmetric a priori. 1/(2π) has structural support (great-circle normalization of the horizon), while 1/6 and other alternatives have no corresponding structural motivation. We therefore prefer 1/(2π) among the candidates — a legitimate prior preference, much as in physics θ_QCD ≈ 0 is preferred by strong-CP symmetry, or O(1) group-theory factors are preferred by geometry, even when observation cannot yet distinguish them. This differs in kind from "a numerical coincidence that happens to fall within the error band but has no derivational origin": 1/(2π) is the simplest candidate and carries a geometric derivation chain. But it remains a motivated preference rather than a completed derivation — the closure-loop question "why the circumference rather than the radius" has not been axiomatically proven, just as θ = 0, before the Peccei–Quinn mechanism gave it a dynamical explanation, was a strongly motivated preference rather than a proven prediction.

5.4 Distinguishing SAE from Verlinde emergent gravity

On the absolute value of the coefficient, SAE and Verlinde emergent gravity cannot be distinguished (if both give 1/2π the values coincide, and the coefficient is unmeasurable). SAE is distinguished by its mechanism (information read-out, more ontological than an entropic-force phenomenology), by its horizon choice (SAE takes the apparent horizon $R_A = c/\sqrt{H^2+kc^2/a^2}$, which differs from other horizon definitions under curvature or at high redshift — structurally distinct and, in principle, measurable), and by the scaling direction. Moreover, the great-circle normalization that gives 2π is a geometric choice on a purely causal manifold with no thermodynamic-temperature residue, so its 2π does not arise from an "erase-ℏ" kind of fitting; but, as noted in §5.3, the step "take the circumference rather than the radius" itself awaits proof by the closure-loop principle, so what distinguishes SAE from Verlinde here is the character of the source of 2π (causal geometry rather than thermodynamics), not a completed derivation of the coefficient.

Thus the horizon-sector form of a₀ is $$\boxed{\ a_0(z) = \frac{c^2}{2\pi R_A(z)} \xrightarrow{\ \text{flat}\ } \frac{cH(z)}{2\pi}\ }.$$


6. Predictions

6.0 The parameter-locking protocol

All predictions in this section use only independent inputs, to preclude the circularity of "tuning parameters against the data to be tested": T₁, T₂ are SAE inputs (not re-estimated here); Ω_d, Ω_Λ are constrained by the cosmic microwave background; a₀(0) is anchored by the local radial-acceleration relation / SPARC; the coupling g is not used in the baseline. In particular, the DESI (w₀, wₐ) is not used to fix parameters; the a₀(z) of MUSE/MIGHTEE is used only for an a posteriori test of the scaling. Lock first, then compute.

We restrict the hard predictions to no more than three, to avoid dilution. Below we give two hard predictions and one via-negativa expectation.

HP1 · The horizon scaling of a₀

$$\frac{a_0(z)}{a_0(0)} = \frac{R_A(0)}{R_A(z)} \simeq \frac{H(z)}{H_0}\ (k\simeq0).$$ Numerically: z = 1 → 1.79, z = 3 → 4.57, z = 4 → 6.33. Compared with the constant-a₀ branch, this differs by more than a factor of four at z ≳ 3. Because a₀(0) is anchored by the local radial-acceleration relation, the falsifiable content of HP1 is the shape of the redshift ratio and slope, not the absolute normalization. Absolute-calibration errors (overall mass-to-light ratio, Hubble tension) partly cancel in the ratio; but redshift-dependent systematics do not cancel automatically — stellar-population evolution, gas content, disk thickness, non-circular motion, selection function, feedback, and resolution can all vary with redshift. The strength of HP1 is therefore that it gives a definite scaling shape (whose difference from constant-a₀ is far larger than these systematics), not a claim that systematics have vanished. This slope test forms a key asymmetry with the unmeasurable absolute coefficient (§5.3): the predictive power is in the shape of the slope.

The primary adjudicator is the high-redshift radial-acceleration relation / baryonic Tully–Fisher relation, especially at z > 3.

Relation to current data. Current tentative data (the linear-in-z fit of MUSE-DARK III, which itself reports "faster than H(z)") are not necessarily on the side of HP1 — their growth may already be somewhat steeper than ∝H. So what HP1 predicts is the specific form "exactly ∝H": if high-redshift data confirm "faster than H," then the exact ∝H is falsified (while the mechanism "a₀ grows with the horizon" survives — only its coefficient-fixed ∝H does not). In practice we first test γ = 1 in $a_0 \propto H^\gamma$. This makes HP1 cleanly falsifiable while not presuming that current data are already on its side. z > 3 is the decisive test.

HP2 · Intrinsic dark energy is non-phantom

There are three layers. The first is a parameter-free structural bound; the second and third depend on a free coupling and have a different status from the first.

Layer one — a genuinely hard bet (parameter-free structural theorem). A positive DBI-C plus a positive Λ₁ gives $$w_{\rm int}(z) \ge -1.$$ SAE's intrinsic dark energy structurally does not cross the phantom divide. This is a hard prediction that a non-parametric reconstruction would falsify, not a soft statement, and it is not to be downgraded together with the softer layers below. The falsifier: if a reconstruction independent of the CPL parametrization and independent of a dark–dark interaction assumption robustly gives intrinsic w < −1, the positive-sign DBI-C structure of SAE is falsified.

On DESI: its CPL best fit (w₀, wₐ) ≈ (−0.75, −0.86) extrapolates to w < −1 at high redshift (apparent phantom crossing). We treat this apparent crossing as an effective reconstruction, not an intrinsic target. The reason: low-order extrapolation fails repeatedly in cosmology (the deceleration parameter, constant-w, CPL alike), because cosmological quantities are dynamical solutions rather than low-order polynomials, and w(z) must be doubly differentiated from integral distance quantities and is sensitive to the parametrized shape; the CPL high-redshift crossing may come partly from the parametrization tail extrapolated into a data-sparse region, and cannot be equated directly with a crossing in the intrinsic field's p/ρ. Moreover, DESI measures a reconstructed effective expansion history, not the microscopic p/ρ of any field; if the dark sector has an interaction, intrinsic w ≥ −1 and effective w_eff < −1 can coexist. This judgment is itself contested: some non-parametric reconstructions also suggest crossing; we take the side "the apparent crossing is partly a parametrization artifact," and place the burden of adjudication on a reconstruction independent of CPL. To be clear, we do not claim to have falsified DESI — DESI's departure from ΛCDM is real, and SAE is consistent with it; what we distinguish is only two different objects, "the w of the effective reconstruction" and "the w of the intrinsic field," the former of which may cross while the latter (in this framework) does not.

Layer two — soft (the effective-crossing branch, one parameter, non-baseline). The kinetic mixing θQ of khronon and C (which preserves shift symmetry, since Q is invariant under C → C + const, so U(C) = const is preserved) gives a source $$S_\theta = -3gQ(\dot H + 3H^2).$$ When an observer reconstructs assuming "matter conserved independently," the effective equation of state $w_{\rm eff} = w_C - S_\theta/(3H\rho_C)$ can cross −1 while the intrinsic $w_C$ does not — consistent with the post-DESI literature on "effective crossing via a dark interaction." But the coupling g is free: the field redefinition (τ₁, τ₂) → (τ, C) does not fix it (the redefinition generates ∇τ·∇C, not θQ; θQ is an allowed rather than a forced operator), and the dual-exchange symmetry (θQ is odd under τ₁ ↔ τ₂) only constrains g ∝ ε, not its magnitude or sign. Effective crossing further requires $gQ < 0$, and the sign is likewise undetermined. This mixing is of kinetic-braiding type, and its true w_eff must be obtained by a full variation (the fluid-decomposition formula is only diagnostic). It should be emphasized that g is not a backdoor parameter free to fit arbitrary data: any nonzero θQ coupling must leave a distinctive imprint at the cosmological perturbation level — on the growth rate $f\sigma_8$ and on the integrated Sachs–Wolfe effect of the microwave background (the source must reach 10–30% of $H\rho_C$, not a small correction). Therefore, if future observation sees an effective crossing only in the background $H(z)$ but finds no perturbation feature corresponding to this operator in the perturbation data, this branch is likewise falsified. So this is an SAE-permissible one-parameter dark-sector extension whose one parameter is itself independently constrained at the perturbation level, not a free escape route for post-hoc fitting.

Layer three — the commitment boundary (open). If a foundational two-clock (τ₁, τ₂) action is written down and fixes g and its sign, the effective crossing of layer two can be promoted to a prediction. This is a larger structural task, left for the future, and does not block the layer-one bet of the mainline.

Remainder-conservation confirmation. The exchange source among khronon dust, C, and geometry is the field-theoretic version of remainder conservation ($\nabla_\mu T^{\mu\nu}_{\rm total} = 0$, a reallocation of accounts rather than creation of energy from nothing); what is conserved is the total dark/geometric sector.

HP3 · A particle-free dark sector (via negativa)

Direct detection of conventional dark-matter particles (WIMPs, axions, etc.) continues to yield null results, consistent with this framework. We list this as a "via-negativa expectation" rather than a strong positive prediction (a null result cannot prove "there is none"); true discrimination still lies in a₀(z), the external-field effect, structure growth / lensing, and the full microwave-background spectrum.

A demoted note on deceleration turnaround. Late-time weakening of dark energy means the acceleration slows earlier than in ΛCDM (DESI's cross-statistics already hint at "slowing acceleration at low redshift," in the same direction); but its specific turnaround redshift depends on the free g of HP2, layer two, and is therefore only directional, with the specific value awaiting the fixing of g. A Roman + Euclid reconstruction of q(z) tests its direction.

Structural statements (not falsifiable hard predictions, listed for reference). Λ_total = 0; c_T = 1 (confirmed by GW170817); the geometric turnaround is unobservable; ξ > 0 would falsify the causal-reinforcement prior. These are structural statements, not among the three hard predictions above.


7. Remainders

SAE's honesty requires stating the remainders openly, without passing them off as predictions, while preserving remainder conservation.

  • Dust abundance Ω_d: posterior (set by the microwave background); $\rho_d \propto a^{-3}$ is remainder conservation, and the value is an integration constant (Mukohyama). Same footing as Ω_c in ΛCDM, or the dust fraction in AeST.
  • a₀ coefficient 1/(2π): its absolute value is unmeasurable (persistent systematic floor, not a hard prediction); its value 1/(2π) is a motivated preference (supported by great-circle geometry, better-reasoned than 1/6, the θ = 0 analogy), not a completed derivation (the closure-loop principle is open), and not a numerical coincidence fitted post-hoc. Three layers in §5.3.
  • khronon–C coupling g: a free Wilson coefficient; not fixed by the field redefinition, with dual-exchange constraining only g ∝ ε and the magnitude and sign undetermined.
  • Λ₁ value: form prior, value posterior. K_B, α, λ: posterior (inherited khronometric parameter space).
  • Closure-loop principle: the great-circle normalization rests on the "read-out must close" motivation and is not yet axiomatically proven (open).
  • Hořava version tension: khronon dust (§4.1, Mukohyama) is cleanest in the projectable version (with its ghost/strong-coupling problem of the extra scalar mode), while c_T = 1 / healthy (§4.4) is in the non-projectable (khronometric) version; realizing integration-constant dust in the khronometric version is an open structural task, not an automatic inheritance — the stability of the dark-matter sub-goal's foundation depends on it.
  • Full Boltzmann (CLASS/CAMB full spectrum): marked as a prerequisite for quantitative work, not an optional engineering task. Without a full-spectrum computation one can only say "structurally corresponds to the AeST microwave-background lesson," not "passes the microwave-background test."

The relations above — B₁+B₂ = 0, E₁+E₂ = 0, Λ₁+Λ₂ = 0, ρ_d ∝ a⁻³, khronon ↔ C ↔ geometry exchange — are instances of one remainder-conservation axiom.


8. Comparison with, and discrimination from, existing frameworks

Relative to AeST. AeST obtains its phenomenological flexibility from a free function plus background initial values; SAE reduces part of that freedom to structural consequences of the brane-DBI, p = d = 3, and the khronon integration constant, and is narrower in function space, hence more easily falsified. This does not classify SAE as a subset of AeST (SAE makes hard predictions AeST does not), but a structural narrowing. c_T = 1 follows from the universality of c.

Discriminating SAE from Verlinde. Not in the a₀ coefficient (unmeasurable), but in the mechanism (information read-out), the horizon choice ($R_A$), and the a₀ scaling.

Discriminating SAE from ΛCDM plus particle dark matter. The a₀ scaling (z > 3), intrinsic w ≥ −1, and no dark-matter particles (WIMP null, via negativa). The external-field effect (e.g. the dynamics of dark-matter-deficient galaxies) is in principle a further discriminant, whose operational quantitative criterion is left for future work.


9. Conclusion

We have derived, from dual-4DD breathing, an aether-scalar-tensor structure that places the three dark-sector effects in a single structure, with no particles: the khronon gives geometric dust, DBI-C gives intrinsically non-phantom dynamical dark energy and MOND, and a 4-form gives the cosmological constant; all conservation laws reduce to one remainder-conservation axiom; and the tensor speed c_T = 1 follows from the universality of c and is confirmed by GW170817. We have revised a₀ from a vacuum scale to a horizon scale, and give two hard predictions that later data can adjudicate: the horizon scaling of a₀ (adjudicated by the high-redshift radial-acceleration relation) and the non-phantom bound on intrinsic dark energy (adjudicated by non-parametric reconstruction).

We have stated all remainders openly: the dust abundance, the coupling g, and the khronometric parameters are posterior; the absolute value of the a₀ coefficient is unmeasurable, and its value 1/2π is a motivated preference rather than a completed derivation; whether the projectable and non-projectable versions can coexist is a foundational open problem. Where the framework has revised earlier intermediate conclusions — the C-dust misassignment, the a₀ decline given by η(t), the undetermined dark-energy coupling g — the revisions are noted in the corresponding sections.

The path taken here trades structural constraint for falsifiability. The two hard predictions place the framework where it can be adjudicated — which is the value of the approach: a theory whose structure is constrained by a prior has no room for post-hoc parameter adjustment and can only be tested by hard predictions. If one of them is falsified, the falsification itself indicates where the prior should be revised — something a model with enough freedom to fit everything cannot provide.


Acknowledgments

The derivations, computations, and internal critique of this paper used a four-AI collaborative method: Claude, ChatGPT, Gemini, and Grok took the roles of conceptual coordination, derivation and review, geometry and topology verification, and adversarial critique, with an additional independent review line for cross-checking. The method was used for drafting, cross-validation, and the surfacing and correction of errors (a methodological record accompanies the prequel); its operation, including several intermediate conclusions that were progressively revised or abandoned, is noted in the corresponding sections.

These AI systems are tools and methods used in this research and do not constitute authors. The entire content of this paper — including its prior assumptions, structural choices, predictions, and everything marked as remainder or open — is the sole responsibility of the author.


Appendix A · Open-item list

Open item Nature If resolved
coexistence of the projectable (dust) and non-projectable (c_T = 1) versionsfoundationalsecures the foundation of the dark-matter sub-goal
a foundational two-clock (τ₁, τ₂) actionstructuralfixes g → promotes HP2's effective crossing to a prediction; or fixes the a₀ coefficient
a₀(τ) full covariantizationstructuralexpresses $R_A^{-1}$ as a foliation-invariant local geometric scalar (θ, curvature), making the MOND term a complete local Lagrangian rather than an FLRW effective term
axiomatic proof of the closure-loop (great-circle) principletheorypromotes the a₀ coefficient from "motivated preference" to "structurally motivated choice" (still unmeasurable)
the perturbation level of khronon–C mixing (S₈ / growth / lensing)computation (viability-critical)the viability of the θQ branch
khronometric α, λ parameter space (post-Newtonian / pulsar / nucleosynthesis)inherited checkfull viability
full Boltzmann (CLASS/CAMB full spectrum)engineeringquantitative comparison with the microwave background
the C-field tracking corridor (carried over from Cosmo V)numericalU(C) entering the corridor naturally

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