Yang–Mills Dynamics from Projective Spectral Entropy

Overview

On a supplied Riemannian metric, the Gravity paper states the conditions under which the horizontal variation of the projective spectral entropy functional \[ S_\Pi[g] = \tfrac{1}{2}\log\det' A_g \] with respect to the base metric is locally dominated by the Einstein tensor: a non-zero Einstein coefficient, which is a matching datum whose cutoff contribution comes from the Seeley–DeWitt coefficient $a_2$, and small curvature relative to the renormalized higher-derivative scale.

Q12 carries out the complementary vertical variation. The operator $A_g$ is extended to \[ A_{g,\mathcal{A}} = -(\nabla^{\mathcal{A}})^2 + E \] on the vector bundle associated with a supplied compact gauge group, and the Seeley–DeWitt coefficient $a_4$ is computed. Q12 does not select that group.

The extended functional $S_\Pi[g,\mathcal{A}]$ contains the renormalized Yang–Mills term with logarithmic coupling, and its vertical variation yields the Yang–Mills equations $D_\mu F^{a\mu\nu} = 0$ in the current-free sector.

Status distinction. The $a_4$ calculation and vertical theorem hold at a supplied fixed metric. Identifying that metric with the Cosmochrony emergent base is separately conditional on [H-L], [H-lift] and a supplied rank-four extension, and needs a Riemannian-to-Lorentzian continuation that is not performed; the emergent co-metric has no established coefficient value, and $g^{\mu\nu}=2\eta^{\mu\nu}$ is not established: Q5b gives a rank-three co-metric, and Q11 a rank-four form only for a supplied extension with independent scales (emergent-geometry presentation note; Q6b 2.0).

Core contributions

Extension to vector bundle: the spectral operator $A_g$ is lifted to $A_{g,\mathcal{A}}$ on the associated bundle, incorporating the admissible gauge connection $\mathcal{A}$ supplied as an explicit input.
$a_4$ coefficient and Yang–Mills term: isolating the gauge component $\Omega^{\mathrm{gauge}}_{\mu\nu} = F_{\mu\nu}$ of the total bundle curvature, \[ a_4(A_{g,\mathcal{A}})\big|_{\mathrm{gauge}} = \int \frac{1}{12}\,\mathrm{tr}_\rho(F_{\mu\nu}F^{\mu\nu})\sqrt{g}\,\mathrm{d}^4x, \] with the overall $(4\pi)^{-2}$ carried once by the heat-kernel prefactor. The induced logarithmic running of $g_{\mathrm{YM}}^{-2}$ has coefficient $I_\rho/(3\cdot 16\pi^2)$ — the entropy term carries $I_\rho/(12\cdot 16\pi^2)$ for $\int F^2$, which matches $(4g_{\mathrm{YM}}^2)^{-1}$ rather than $g_{\mathrm{YM}}^{-2}$ — depending on the representation through the Dynkin index $I_\rho$, hence not universal.
Vertical variation yields Yang–Mills equations: $\delta_{\mathcal{A}} S_\Pi[g,\mathcal{A}] = 0$ gives $D_\mu F^{a\mu\nu} = 0$ (proved for the $a_4$ derivation given $G_\Pi$).
Difference in UV divergence degree: within a proper-time cutoff, the Einstein term diverges quadratically (order $a_2$) and the Yang–Mills term logarithmically (order $a_4$). This difference is structural in that scheme and is not scheme-independent — the zeta-regularized determinant carries no power divergences. The physical couplings $g_{\mathrm{YM}}$ and $G_N$ are renormalized matching data, and only the logarithmic running is computed. No predictive formula for $G_N$ and no tuning-free hierarchy is claimed (consistent with the Gravity paper, where $G_N$ is a matching datum).
Vertical variation at fixed metric: at fixed base metric, the vertical variation isolates the Yang–Mills sector. Full horizontal–vertical decoupling does not hold: the metric variation of $F^2$ is the Yang–Mills energy–momentum tensor $T^{\mathrm{YM}}_{\mu\nu}$, an $a_4$-order back-reaction treated in Q13.

Spectral stratification as an organisational principle

Beyond the technical derivation, Q12 identifies a conceptual principle that distinguishes the Cosmochrony approach from conventional unification schemes.

In standard group-theoretic unification, gravity and gauge interactions are sought at the same algebraic level — different representations of a common group $G_{\mathrm{unif}}$. Their combination requires finding a symmetry large enough to accommodate both.

The present framework suggests a different picture: gravity and gauge dynamics are separated by geometric direction (horizontal vs. vertical variation on the admissible bundle) and by spectral order ($a_2$ vs. $a_4$ in the Seeley–DeWitt hierarchy). Their distinct UV behaviours — quadratic divergence for gravity, logarithmic for gauge — are structural consequences of this separation, not independent empirical inputs.

Implication for unification. The difficulty of incorporating gravity into the Standard Model framework may reflect a difference of Seeley–DeWitt order rather than the absence of a common symmetry group. The natural organisational space for unification in this framework is spectral and variational, not primarily group-theoretic.

Relation to the Cosmochrony programme

Q12 is the vertical counterpart to the Gravity paper. Each sector follows from the same functional by varying in a different direction; joining the two variations, and the conditional system that results, belongs to Q13:

Gravity paper: $\delta_g S_\Pi \supset c_{\mathrm{EH}}^{\mathrm{ren}}\,G_{\mu\nu}$, dominant for $c_{\mathrm{EH}}^{\mathrm{ren}} \neq 0$ and $R\,L_4^2 \ll 1$ (the coupling to matter, $G_{\mu\nu} + \Lambda g_{\mu\nu} = 8\pi G_N T_{\mu\nu}$, is the conditional result of the Thermodynamics paper)
Q12: $\delta_{\mathcal{A}} S_\Pi = 0 \implies D_\mu F^{a\mu\nu} = 0$

The compact gauge group and connection are hypotheses of the vertical construction, and every result of Q12 holds for any supplied compact group. No source identifies that group: O31 withdraws every derivation of colour co-admissibility, of $\mathrm{SU}(3)$ and of the composite, so Q12 establishes no colour factor or complete Standard Model gauge group.

The joint variation — the conditional Einstein–Yang–Mills system and the $a_4$-order back-reaction $T^{\mathrm{YM}}_{\mu\nu}$ — is carried out in Q13, where the couplings likewise remain independent renormalized matching data, so no numerical value for $G_N g_{\mathrm{YM}}^2$ follows.

Open directions

Gauge-group identification: derive, independently of the withdrawn O31 chain, which compact group and representation act on the admissible bundle. Until then the Yang–Mills result is conditional on those inputs.
Matter sector: extend the vertical variation to include projected matter currents $J^{a\nu}$.
Spectral stratification beyond order 4: investigate whether higher Seeley–DeWitt coefficients $a_6$, $a_8$ produce further interaction sectors or remain suppressed.

References

Jérôme Beau. Yang–Mills Dynamics from Projective Spectral Entropy: Vertical Heat-Kernel Variation on the Admissible Fibre, 2026. doi:10.5281/zenodo.20189137