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We examine the operator content of three scalar certificate families and supply explicit spectral comparisons where the stated hypotheses permit them. For radial stellar pulsations, we derive a Newtonian work identity and a self-adjoint general-relativistic form, distinguish homologous trial values from fundamental eigenvalues, and recover a post-Newtonian structural benchmark. For a discrete Dirichlet Hardy-type form with constant confinement, we obtain the complete finite spectrum and the sharp box-uniform spectral floor; direct action variations identify an obstruction to a proposed physical coupling identification. For the SU(N) Hamiltonian lattice gauge model at fixed lattice spacing, a full-space single-plaquette comparison gives an explicit gap for all N at the stated coupling, and an application of Yarotsky's weak-interaction theorem gives a sufficiently strong-coupling window uniform in N and open-lattice volume, including the canonical infinite-volume physical GNS representation. The paper separates analytic proofs, applications of established external theorems, Lean-certified scalar results, and finite numerical checks. It does not assert a stellar mass cutoff, physical selection of the coupling kappa=1/2, a numerical many-plaquette threshold, or a continuum Yang-Mills mass-gap solution. The supplementary archive includes proof notes, Lean sources, reproducible computation scripts, results, and provenance records. The manuscript is CC BY 4.0; repository software in the supplement retains its AGPL-3.0-or-later license.
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Carl P. Zimmerman (2026) studied this question.
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