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P10

The canonical problem of time as a category error

an empirically forced cosmic time, deparametrization, the dissolution of frozen dynamics, and a graviton quantization the de~Sitter horizon closes without a free parameter—the seam where enters gravity—in Cosmological Relativity

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Abstract

In the canonical formulation of general relativity the Hamiltonian is a sum of constraints that vanish on the physical phase space: no preferred time survives, and the generator of evolution annihilates physical states rather than evolving them. This is the canonical “problem of time.” We argue that it is not a technical defect awaiting a technical repair, but the canonical symptom of a category error—treating the four-dimensional manifold of occurrences as the thing that exists, the block universe.

The companion framework paper [JanzenCRframework] introduced, as an ontological commitment of Cosmological Relativity (CR), a global cosmic time that general relativity's formalism admits but does not supply. Here we show what that commitment does to the canonical formalism. The decisive premise is not a new calculation but a selection: the bare Arnowitt–Deser–Misner (ADM) machinery propagates data along an arbitrary hypersurface and settles nothing, whereas CR selects a preferred cosmic foliation—forced empirically by the isotropy of the cosmic microwave background (CMB) and structurally by the horizon geometry of collapse [JanzenBHcausality]. On that foliation the lapse recovers its meaning as the metrical rate of the existing layer's advance, dτ= N dt; the constraint, deparametrized along cosmic time, is solved for a true Hamiltonian that generates the advance; and quantum evolution in cosmic time is unitary. The frozen constraint and the true Hamiltonian are the same canonical content under two readings, differing only in whether the manifold is granted existence.

The deparametrization is, as a technique, entirely standard; what CR adds is not a mechanism but a warrant. The multiple-choice problem—that many candidate internal times exist, that inequivalent quantizations follow from different choices, and that the formalism prefers none—has force exactly when the clock is chosen for formal convenience internal to the theory, and loses it when the clock is fixed from outside the formalism by ontology and observation. It is dissolved, not solved within the space of formal clocks.

We exhibit the structure first in flat Friedmann–Lemaître minisuperspace, where the deparametrized Hamiltonian reproduces the flat-ΛCDM expansion—the sinh2/3 law established in [JanzenCRframework]—and then lift it to the closed-S3 layer's propagating sector: the transverse-tracelessL20 graviton modes form a discrete tower that deparametrizes to a unitary evolution in cosmic time, and project into a fundamental observer's frame as the flat-ΛCDM graviton, with matter density appearing only as the bend of the slicing rather than as ontological content. The external clock is no convenience: an internal area clock separates the dynamics at Λ=0 and would serve, but at Λgt;0 it no longer does, and the absolute cosmic time is forced.

In that sector the quantization moreover closes without a free parameter. The scale-factor Hamiltonian carries deficiency indices (1,1) independently of operator ordering—the inverse-square coefficient at the origin attaining γ= 14 across the natural ordering family, strictly below the essential-self-adjointness threshold 34—so a single boundary condition at a=0 remains; and that point is not a generic half-line endpoint but the de Sitter cosmological horizon, whose Hartle–Hawking thermal state, at the surface gravity κ=1/α the substrate itself fixes, selects the Friedrichs extension. The deficiency freedom is thereby not merely parametrized but closed, and closed without a free parameter: enters the gravitational sector at the seam, scaled by Λ alone.

With the tower coupled, the boundary coefficient is promoted to an operator straddling the threshold and the same thermal regularity supplies the condition fibre by fibre, so that what remains open is not the boundary condition but the definition of the interacting tower. That is a different thing from a residual freedom in the quantization, and its shared character with every interacting field theory does not settle it: the divergence is measured here rather than characterised—quartic at a leading constant fixed by the propagating-component count rather than assumed; logarithmic at a coefficient the tower's own spectrum settles exactly; and, where the shear breaks the degeneracy among the quadratic invariants, one further counterterm whose Weyl-squared coefficient is twice a real scalar's—and it is carried as this programme's own open frontier.

The problem of time is thereby dissolved as a category error, not solved by an addition to the formalism, in exactly the way the same ontological correction dissolves the inference that gravitational collapse completes in finite cosmic time [JanzenBHcausality].

Introduction: the problem of time, as standardly posed

The canonical quantization of general relativity confronts a difficulty that has resisted resolution for half a century. In the ADM decomposition [ADM1962], spacetime is foliated by spatial hypersurfaces and the Einstein–Hilbert action is recast in Hamiltonian form. The result is a fully constrained system in the sense of Dirac [Dirac1964]: the total Hamiltonian is a sum of the scalar (Hamiltonian) constraint H and the momentum constraint Hi, each weighted by the lapse and shift Ni, and each vanishing on the physical phase space. The lapse and shift are not dynamical; they are Lagrange multipliers enforcing the constraints. Promoting the scalar constraint to an operator yields the Wheeler–DeWitt equation HΨ= 0 [DeWitt1967]: the physical state is annihilated by the generator that should evolve it. The wavefunction of the universe does not appear to depend on any time parameter at all.

This is the problem of time [Kuchar1992, Isham1993]. Its sharpest statement is that the formalism contains no preferred time variable, that every spatial foliation of a given spacetime is related to every other by a gauge transformation generated by the constraints, and that “evolution” in the coordinate label is therefore pure gauge—a re-slicing of one fixed four-dimensional object, carrying no physical content. The many proposed responses—identifying an internal time among the canonical variables before quantization, coupling a material clock, treating observables as relational “evolving constants,” or abandoning a fundamental time altogether—each carry well-known costs [Kuchar1992, Isham1993, Rovelli2004, BarbourEnd], to which we return in Section 8.

Our claim is that the difficulty is conceptual before it is technical, and that the conceptual diagnosis is precise rather than vague. The frozen formalism is the canonical expression of a single metaphysical commitment: that the four-dimensional manifold is the object that exists. We will argue, following the ontological foundation of CR [Janzen2025, JanzenCRframework] and the necessity assembled in Section 2, that this commitment is a category error—the confusion of what happens with what exists—and that it is empirically false, the universe having furnished, in the CMB, direct evidence of the very cosmic time the formalism declines to recognize. When that error is declined, the same canonical equations describe a real cosmic time all along.

We stress at the outset the register of this paper. We do not propose a modification of general relativity, a new term in the action, or an additional structure bolted onto the canonical formalism. The equations are those of Einstein and of ADM, unchanged. What changes is the reading. The frozen constraint and a true Hamiltonian generating cosmic-time evolution are, as we will show, the same content under two readings, differing only in whether the manifold of occurrences is granted the kind of existence that belongs to the evolving three-dimensional world. The problem of time is not solved here. It is dissolved.

The paper proceeds as follows. Section 2 earns the premise the argument needs—that a preferred cosmic time is real—on two independent grounds, one conceptual and one empirical. Section 3 reads the unchanged ADM formalism under the two ontologies, and Section 4 isolates why the move is a selection rather than a construction: the bare machinery settles nothing, and everything turns on whether a foliation is distinguished to be selected. Section 5 carries out the deparametrization, structurally and then in flat minisuperspace, marking the boundary between the two. Section 6 lifts it to the closed-S3 layer's propagating sector—the transverse-traceless graviton tower, advanced unitarily in cosmic time—and there the quantization closes: the scale-factor Hamiltonian's deficiency-(1,1) freedom, ordering-independent, is fixed by the de Sitter horizon's own thermal state, without a free parameter, leaving open not the boundary condition but the definition of the interacting tower. Section 7 states the verdict negatively, and Section 8 places the argument against the internal-time, relational, and timeless programmes, where the multiple-choice objection is met not with a mechanism but with a warrant.

The necessity: a cosmic time that is real, not posited

The canonical move of this paper rests on one premise: that there is a preferred cosmic time, and that it is a real feature of the world rather than a convention chosen for convenience. This premise is not assumed. It is forced, on two independent grounds—one conceptual, one empirical—which we summarize here; the full argument is developed in [Janzen2025, JanzenWildGoose, JanzenFortress] and stated as the necessary-and-sufficient augmentation of general relativity in [JanzenModernParallax].

The conceptual ground: occurrence is not existence. To exist is to endure—to persist through an interval. The three-dimensional world exists in this sense, and so do the things in it. An event, by contrast, is something that happens: it occurs at a place and an instant and is gone. A worldline is the continuous succession of events associated with an enduring thing, and four-dimensional spacetime is the manifold of all such events—the totality of what happens. The persistent confusion about time, traceable from Heraclitus and Parmenides through to modern eternalism, is the treatment of occurrences as though they were existents: the reification of the event-manifold into a thing that exists [Janzen2025]. Once spacetime is imagined to exist, every moment along a worldline is imagined to exist on equal footing, the distinction between past, present, and future is declared an illusion, and time is said not to pass. But that conclusion was smuggled into the premise. Granting existence to the manifold of occurrences is not a discovery about time; it is a misuse of the word “exist.” The coherent picture is the one in which an evolving three-dimensional world exists and advances, and events happen in the course of that advance, mapping to a four-dimensional spacetime that represents them without being a further existent of the same kind.

In CR this distinction is structural. What exists is the layer —a real three-sphere evolving in a real de Sitter substrate [JanzenCRframework, JanzenSlicing]. The four-manifold is the representational record of the events that happen as the layer advances. The layer's existence and advance are not optional gloss on a fundamentally four-dimensional object; they are the ontology, and is its shadow.

The empirical ground: the CMB measures the cosmic rest frame. That a preferred cosmic time might be real but undetectable is the situation relativity leaves open: local experiments cannot distinguish a true state of rest, because the relativity of synchrony—a general kinematic consequence of one's chosen rest convention, independent of the light postulate—and the round-trip symmetry of local signalling together hide one's motion. Einstein's identification of simultaneity with frame-relative synchrony was, on this much, a philosophical choice among two empirically equivalent options, not a deduction; treating the local inaccessibility of a cosmic rest frame as evidence of its nonexistence is a modal fallacy [JanzenWildGoose].

The universe, however, did furnish the missing evidence. The cosmological redshift of the CMB is isotropic to high precision, and the primordial temperature anisotropies at the level of one part in 105 have been preserved across the entire history of expansion [Aghanim2020]. Had the expansion rate varied locally with the inhomogeneous matter distribution, the accumulated redshift along different lines of sight would differ by far more than is observed—by some three orders of magnitude, as we establish quantitatively in the companion paper [JanzenModernParallax]—and the isotropy therefore certifies that cosmological space has expanded uniformly throughout cosmic history. But to speak of a three-dimensional space expanding uniformly through time already presupposes a cosmic time, a cosmic rest frame, and an associated simultaneity. The same data fix our own velocity relative to that frame through the CMB dipole. The cosmic rest frame is thus not a large-scale average or a coordinate convenience but one of the better-measured structures in cosmology. Synchrony is relative; simultaneity is absolute [JanzenWildGoose, JanzenFortress].

The two grounds are one correction. These are not two arguments but two faces of one. The relativity-of-simultaneity premise is precisely what licenses the reification of the block: if there is no objective “now,” the four-dimensional manifold is all there coherently is, and the layer's privileged advance has no referent. Conversely, an empirically real cosmic “now” restores the layer as the existent and demotes the manifold to its record. Declining the block (the conceptual correction) and admitting the cosmic rest frame (the empirical correction) are the same move. The equations of relativity are untouched by it; only the interpretation shifts—from “if two events appear simultaneous they must be simultaneous” to “apparent simultaneity is a local matter with no bearing on the global cosmic simultaneity that cosmology establishes empirically” [JanzenFortress].

This is the premise the canonical argument needs, and it has been earned rather than assumed: there is a preferred cosmic foliation, and it is real.

The canonical formalism, read two ways

We now read the standard canonical formalism under the two ontologies. Nothing in this section alters the equations.

In the ADM form, a spacetime (M,g) is foliated by spacelike hypersurfaces Σt with induced metric hij and conjugate momentum πij, and the line element is

ds2 = -N2 dt2 + hij (dxi + Ni dt)(dxj + Nj dt),
(1)

with lapse and shift Ni. The action becomes S = ∫dt d3x (πij hij - N H - Ni Hi), and variation of and Ni enforces the constraints H=0, Hi=0. The total Hamiltonian H = ∫d3x (N H + Ni Hi) is a sum of constraints; on the constraint surface it vanishes.

The frozen reading. Suppose the existing object is the four-dimensional manifold itself. Then a choice of foliation is a choice of how to slice one already-existing thing into a stack of three-dimensional pictures, and a different foliation is a different slicing of the same thing. No slicing is distinguished; the relation between any two is a gauge transformation generated by the constraints; and since the generator of -evolution is a constraint, it moves a physical state nowhere. Quantum-mechanically, HΨ=0: the state is timeless. This reading is internally consistent. Its content is exactly the content of the premise: if the block is what exists, time does not pass, and the formalism correctly reports that there is nothing for a Hamiltonian to do. The frozen formalism is not a mistake of calculation. It is the faithful canonical image of the block.

The reading CR adopts. Suppose instead, with CR, that what exists is the evolving layer , and that is the record of the events that happen as it advances (Section 2). Then a foliation is not a slicing of a pre-existing block; it is a choice of how to coordinate the advance of the existing world, and one such foliation—the cosmic one—tracks that advance rather than cutting across it. On this reading the lapse is not a bookkeeping multiplier but the metrical amount by which the existing layer advances per unit of the time label,

dτ= N dt,
(2)

with the shift Ni carrying the foliation's non-orthogonality to the layer. The constraint H=0 is still an equation; but now it is read as the relation that, once solved for the momentum conjugate to the cosmic time, yields the generator of the layer's advance—a true Hamiltonian. The same symbols, the same constraint surface, the same dynamics; a different answer to the single question of what exists. This lapse and shift are the very levels the cosmological development computes on: the lapse is the foliation stacking rate the observable expansion rides—set by the geometry, the density the content that set rate carries, read off the clock rather than sourcing it—and the shift is the synchronization through which that expansion is observed as distance and redshift, with the leaf's bend the matter it carries [JanzenOperator, JanzenCosmogenesis]. That a plasma process rides the one rate or the other is then fixed by which side of the reassignment seam it falls on, not chosen: the same selection of the existent's foliation that turns the frozen constraint into a true Hamiltonian here fixes, one level down, which rate a recombination-era or a nucleosynthesis-era computation must read—and reifying the shift's synchronous slicing as the existent is the block error, met at the level of a rate.

The selection is the whole of the move

It is worth isolating why the foregoing is a recognition rather than a new construction, because this is the crux of the paper.

The ADM machinery propagates canonical data along whatever foliation one supplies. It is indifferent to which foliation that is; it has no preferred time of its own, and in this exact sense the bare formalism contains no resolution of the problem of time and no obstruction to one. Everything turns on what is fed to it. If nothing distinguishes a foliation, the constraint is all there is and the state is frozen. If a foliation is distinguished, the constraint deparametrizes along it and a true Hamiltonian appears. The canonical formalism is the same in both cases; what differs is whether a preferred foliation exists to be selected.

CR supplies exactly that, and supplies it from outside the bare formalism, on the grounds of Section 2: the cosmic foliation is real, forced empirically by the CMB and conceptually by the occurrence/existence distinction. It is moreover the foliation that the rest of the programme independently singles out. The metric-singularity structure of the event horizon determines a unique limiting causal orientation in collapse, generically non-orthogonal to any spacelike slice, and this is the orientation CR reassigns as cosmic time [JanzenBHcausality, JanzenCRframework]; the representational freedom in choosing among Lorentzian metrics on the fixed manifold is a genuine gauge symmetry, organized by the description groupoid [JanzenGroupoid], but the cosmic foliation is not one of its orbits to be quotiented away—it is fixed by the ontology the gauge freedom is defined over.

The consequence is methodological as well as physical. There is no separate “canonical machinery” result to be proved here; the deparametrization that follows is standard once a clock is in hand. The content of this paper is that CR's cosmic time is the physically correct clock, on grounds that are ontological and empirical rather than formal, and that the canonical face of the existing physics is therefore a true Hamiltonian rather than a frozen constraint. The move is the selection. Everything else is reading the textbook on it.

The same selection settles what a mass charge could be. The ADM mass is defined relative to an asymptotic time translation, and exists only where the geometry supplies one—which asymptotically-de Sitter spacetimes do not, there being no global timelike Killing vector, so that no conserved charge is well defined there at all [JanzenSlicing]. On the reading taken here that absence is not a deficiency of the geometry but a misplacement of the question: the time this construction runs on is not recovered from an asymptotic symmetry but selected and measured, so a quantity whose definition waits on an asymptotic Killing vector is waiting on the wrong thing. It is the same move as the paper's own—what the formalism cannot supply from inside, the selection supplies from outside, and the question that presupposed the missing structure lapses with it.

Deparametrization and the true Hamiltonian

We now carry out the reading. The structural statement is independent of any model; the explicit minisuperspace realization that follows is an illustration of it, and we are careful to mark the boundary between the two.

The structural statement. Let the cosmic time of Section 2 be the distinguished foliation parameter, and let pτ denote the momentum conjugate to it. The scalar constraint, linear in pτ after the cosmic clock is isolated, takes the deparametrized form

pτ+ (qA,pA) = 0,
(3)

where (qA,pA) are the remaining (true, gauge-invariant) degrees of freedom of the layer and depends on the cosmic time only through them. Equation (3) is the same constraint that, read with no preferred foliation, gives HΨ=0. Read with the cosmic clock selected, it is solved for the generator of advance: classically dqA/dτ= ∂ /∂pA, and on quantization

i ∂τΨ(qA,τ) = Ψ(qA,τ).
(4)

This is a genuine time-dependent Schrödinger equation generating unitary evolution in cosmic time, not the frozen Wheeler–DeWitt constraint. The foliation is fixed—by the ontology, not by a gauge choice—so there is a true time and a true Hamiltonian. The frozen constraint and the true Hamiltonian are (3) read two ways; they are the same content, differing only in whether the manifold is granted existence. Deparametrization here is not a trick that restores a time that was really absent; it is the formal face of a time that was never lost, because the cosmic foliation was real all along.

A zero-duration boundary, and what it does to the evolution. The cosmic time of Section 2 is the real part of the companion framework's complex cosmic time, and that framework's closed contour contains one segment—the lift, joining the collapse's comoving turnaround to the branch point at which a collapse becomes a cosmology—along which the real part does not advance [JanzenCRframework]. The consequence for (4) is immediate and worth stating plainly, because it is unusual: cosmogenesis occupies no cosmic time at all, so the evolution operator across it is U(Δτ=0)= 1. The true Hamiltonian has no interval in which to act there. The geometry nonetheless changes across the segment—the areal radius climbs from the turnaround to zero and the expansion rate is carried from zero to divergent—so the change is not generated by but is the segment's own analytic content, the contour read at another point of itself. The beginning is therefore not a first instant of the evolution this section constructs; it is a boundary of zero duration within it, and that is why nothing can be lost across it: no evolution acts, so none can be non-unitary.

We mark the limit of the claim. What is established is the classical statement—the foliation parameter does not advance on that segment, so no interval of τ separates the two legs—together with its immediate consequence for the evolution operator. What is not established here is a quantization of the Euclidean segment itself. The state on either side is related by the identity in cosmic time; whether the imaginary-time stretch admits a quantum treatment in its own right, and what that treatment would say about the {qA,pA} across it, is not addressed by this deparametrization and is not claimed by it. The gap is named rather than managed: it is carried as an open problem of the companion framework [JanzenCRframework], and its shape is definite. The silence is structural, not a matter of refinement—an evolution parametrized by cosmic time cannot describe a segment of zero cosmic duration, so no sharpening of reaches it. What is owed is an account of an imaginary-time stretch across which the classical configuration changes while the foliation parameter does not, and it is the natural point of contact between this construction and Euclidean approaches to the quantum beginning—contact the programme does not presently make. The classical account of the beginning is complete; the quantum account of it is absent, and the second half of that sentence travels with the first. One step of it can nonetheless be taken here, and taking it sharpens what remains.

The propagator across the lift is Euclidean. The evolution (4) is generated in the framework's complex cosmic time, and on the lift that time runs along the imaginary direction: τ= const+is, so s=i ∂τ and (4) becomes sΨ=- Ψ. The kernel carrying the state across is therefore not the unitary U=e-i Δτ but

K=e- |Δη|,
(5)

a Euclidean kernel—real, contracting, and not unitary—with |Δη| the lift's imaginary conformal-time interval. This is consistent with U(Δτ=0)= 1 rather than in tension with it: no cosmic time elapses, and the kernel is not an evolution in cosmic time.

Two things follow, and the first is a check the construction did not have to pass. A mode of frequency ω is damped by e-ω|Δη| under (5); the framework's independent classical reading of the same segment damps a mode carrying eikcsη by e-kcs|Δη| [JanzenCRframework]. With ω=kcs these are the same expression, term for term. The classical selection rule—frozen content crosses, oscillating content does not—is the Euclidean kernel, read classically. Second, and this is the content the classical reading could not supply: a Euclidean kernel run for a long imaginary interval projects onto the ground state, suppressing each excitation by e-(En-E0)|Δη|. The scope of that statement should be fixed carefully, because the two sectors it separates are not symmetric. The kernel acts on oscillatory content; a frozen, zero-frequency mode is a fixed point of it and passes unchanged. And at the crossing no mode is oscillating: on the contracting leg grows without bound as r→0, so the comoving horizon shrinks to zero and every mode exits it and freezes before the branch point [JanzenCRcosmology]. So the projection does not select the frozen content that crosses—it has nothing to act on there. What it acts on is the oscillatory content of modes while they were sub-horizon, which it annihilates; the ground-state projection is the statement that this content, and not the frozen amplitude, is what the segment removes.

The projection is not exact, and where it fails is a scale rather than a caveat. At |Δη|≃1.7×104 Mpc the damping reaches e-2 only at k∼2×10-4 Mpc-1, so modes below that wavenumber are not strongly suppressed and cross with residual excitation. That wavenumber subtends ℓ≈3 on the last-scattering sphere, which is where the framework's independent transmission calculation places the boundary of the filter's reach [JanzenCRframework]. The two routes agree on the scale as well as on the factor.

The obvious objection is that a Euclidean kernel needs a Hamiltonian bounded below, and that Euclidean gravity notoriously lacks one—the conformal factor entering the Einstein–Hilbert action with the opposite sign, so that the Euclidean action can be driven arbitrarily negative. That objection does not reach this construction, and the reason is structural rather than fortunate. The conformal-factor problem arises when the path integral ranges over the conformal factor of the metric. Here it does not. The substrate's scale is α and is fixed—not chosen, but required, as the unique maximally symmetric structure carrying no unforced modulus [JanzenShadowExistence, JanzenSlicing]—so there is no conformal mode to integrate over; and the propagating gravitational degree of freedom of the layer is the transverse-traceless shear of Section 6, which is precisely the sector the conformal mode is absent from. Mode by mode that sector is (13), a harmonic oscillator, whose Hamiltonian is bounded below. The areal radius along the lift is likewise confined, running between the comoving turnaround and the branch point on an interval fixed by the progenitor mass, with the substrate curvature finite throughout [JanzenCRframework, JanzenCircle]: there is no runaway direction for the kernel to diverge along.

And the state the kernel projects onto is not a new posit but one this paper has already selected on independent grounds. Section 6 finds the scale-factor Hamiltonian to have deficiency indices (1,1)—a one-parameter family of candidate quantizations—and closes it, without stipulation, by observing that the boundary at a=0 is the de Sitter horizon, that its surface gravity is κ=1/α, and that the regular Euclidean state at that κ leaves nothing to choose. That is the same condition the kernel (5) enforces}: regularity in the Euclidean continuation. And that regularity is available only because of what the causality companion establishes about the boundary. A regular Euclidean state exists at a horizon only if the Euclidean continuation is smooth there—free of a conical defect, curvature finite. The horizon at a=0 is a metric singularity, at which the spatial measure collapses while the curvature stays finite, and not a curvature singularity [JanzenBHcausality]; had it been the latter there would be no smooth Euclidean section, no regular state to select, and the extension would remain unfixed. The distinction that dissolves the information paradox is the same distinction that makes this quantization unique. The extension-fixing condition and the lift's kernel are one requirement met twice, once at the horizon and once across the beginning.

One approximation is carried and its size is bounded below rather than left open. The kernel's frequency is not constant along the segment—the layer's scale varies with the path parameter—so the projection is adiabatic rather than exact, and the residual at the largest scales quantified above is one face of that. The ceiling on what it can transmit is computed in §7}, and it is small enough that nothing above turns on it. The segment's variational treatment, by contrast, is not owed: it is given below. The relation between the configuration variables {qA,pA} on the two sides is described through the kernel's action on the modes, and the segment is exhibited there as a solution of a variational principle in its own right.

the marginal congruence (dr/d τ)2+f=1—the γ=1, J=0 case of the effective-potential form (dr/dτ)22-Veff with Veff=f derived in [JanzenThesis, Eq. (4.24)]—which is 12 r2+V= 12 with V(r)= 12 f(r). Continuing τ=is sends r↦-i r' and the Lorentzian action S=∫d τ[12 r2-V] to S=-iSE with

SE=∫ds [12 r'2+V(r)],
(6)

whose stationary points obey r”=+V'(r)—motion in the inverted potential, the standard signature of a Euclidean solution—with first integral 12 r'2-V=- 12. The lift's closed form r(s)=-(2Mα2)1/3| sin (3s/2α)|2/3 satisfies both: the first integral is - 12 identically along the segment, and r” agrees with V'(r) to the precision of the checkP10R9. So the imaginary-time segment is not a formal device but a solution of a variational principle—an instanton connecting the Lorentzian turning point to the branch point.

Its action converges. Near the branch point V≃-M/r while r∝s2/3, so the integrand of (6) grows as s-2/3 and is integrable; numerically SE→1.489 in units α=1 on the forced member. The segment therefore carries a finite weight rather than a divergent one, which is what a saddle-point treatment of the beginning would require of it. Two normalisations are in play, and the relation between them can be settled rather than flagged. The functional (6) carries a unit kinetic term; the gravitational action carries the metric factor and the prefactor implied by (9). They share a solution—the contour's law (dr/d τ)2=2M/r+r22 is the Friedmann equation with a=r, the identification 2M↔(8π/3)ρd being just M=(4π/3)ρd—so the instanton is one trajectory read in two measures, and only its action value differs.

That value follows without further input. On shell the reduced action is S=∫pa da, and inverting (9) gives pa=(3/4π)a a; continuing τ=is yields S=-iSE with

SEgrav=3/4π∫ds r r'2 =3/4π∫ds r [f(r)-1],
(7)

using r'2=f-1 on the segment. The integral converges rapidly and gives SEgrav=-0.0481 α2/G on the forced memberP10R8.

Its sign is the informative part, and it is not a pathology. A negative Euclidean gravitational action is the Hartle–Hawking sign: the no-boundary de Sitter action is likewise negative, 2/8G in this convention, yielding an enhanced rather than suppressed weight [HartleHawking1976]. The present value is the same sign and the same order, smaller by a factor of order two, which is what a segment of the contour rather than a full hemisphere should give.

The sign traces to the segment lying on the r lt;0 branch, where pa lt;0 while increases. So the beginning's weight is of the no-boundary type, obtained here from a contour the construction already possessed rather than from a boundary condition imposed on the path integral. One register point must be made here, because the vocabulary invites a reading the construction refuses. The segment's parametrisation runs imaginary, and the kernel and action computed above are the kernel and action of that parametrisation; they are not the Euclidean objects of a Wick-rotated spacetime. The geometric-core paper states the guard generally: the construction reaches a real manifold through imaginary instruments, and the continuations it uses—the embedding coordinate, the equatorial seam, the cosmogenesis reassignment—are real analytic continuations on a spacetime that is Lorentzian throughout, not Wick rotations [JanzenGeometricCore]. The de Sitter horizon's Gibbons–Hawking state, by contrast, is a Euclidean continuation, and that paper marks it as distinct in kind from these. So the two must not be conflated: the thermal register in which is fixed by the period β=2πα is not the register the segment's action belongs to, and dividing that action by that would be joining two continuations the construction keeps apart. What the action is, is a real integral along a real curve of a real Lorentzian geometry, whose parameter happens to run imaginary over one stretch; what it is not is an exponent awaiting a quantum of action. Its comparison with the no-boundary sign above is a comparison of signs and magnitudes, not an identification of frameworks. The adiabatic correction, and where it fails. The kernel projects exactly only if is constant along the segment, and it is not: the tensor tower of Section 6 carries frequencies ωnn/a, and varies along the lift, diverging in ω as the branch point is approached. The exact suppression exponent is therefore ∫ωn ds rather than ωn|Δη|, and the first question is whether it converges at all. Two different questions are in play here and it is worth keeping them apart, because only one of them is what the word “adiabatic” names.} An adiabatic expansion is controlled by |dω/ds|/ω2, and along this segment that quantity is ∝s-1/3 and diverges at the branch point—so the adiabatic invariant E/ω, which is what an adiabatic approximation conserves, is not conserved through it. The suppression is nonetheless finite, and for a different reason: the exponent ∫ωn ds converges because ω∝s-2/3 is integrable, which is a statement about the action integral and not about slow variation. So the correction here is semiclassical rather than adiabatic—the companion cosmology paper names the same object correctly, as a WKB form whose adiabaticity parameter is of order unity [JanzenCRcosmology]L14. It does: near the branch point |r|∝s2/3, so the integrand grows only as s-2/3 and

0πα/3ds/|r(s)|=3.3387 α-1
(8)

on the forced memberP10R7. The correction is not small and it runs the conservative way: the constant-frequency estimate using the turnaround value gives 1.4396 α-1, so the exact exponent is larger by a factor 2.32 and the suppression is stronger than the naive reading of (5) suggests.

Whether the projection is adiabatic is a separate question with a definite answer. The adiabaticity parameter |dω/ds|/ω2 is C/μn with running from 1.72 near the branch point to 0.16 near the turnaround, so the approximation is controlled by the harmonic index alone. With μn2=n(n+2)-2, n≥2, this gives 0.70 at n=2, 0.48 at n=3, and 0.16 by n=10. The projection is therefore adiabatic for all but the lowest few harmonics, and degrades to order unity only at n=2 and n=3. That the approximation should fail exactly where the tower is coarsest is expected rather than surprising—there are no modes below n=2 on S3—and it locates the correction rather than leaving it as a caveat. We record, without claiming it, that the harmonic indices at which the treatment loses control are the lowest ones.

What that loss of control costs is bounded, and the bound is one-sided because of the tower's own floor. The suppression falls monotonically with the harmonic index—2.8×10-4 in amplitude at n=2, 5.9×10-6 at n=3, and by roughly two orders of magnitude per step thereafter—so the mixing the adiabatic projection neglects can only carry amplitude into more-suppressed modes. And there is no mode below n=2 to carry amplitude the other way: the least-suppressed mode has no source beneath it, so the bound is structural rather than estimated. Taking the whole O(ε) fraction out of n=2 at the worst case leaves that mode more suppressed, not less, and the mode it enriches does not reach the unmixed ceiling. The ceiling on transmitted power is therefore the unmixed n=2 value, 7.9×10-8—and below 10-3 even on the naive exponent, which is the weaker estimate. So the residual is located, bounded, and reaches nothing observableP10R12. The relation between S3 tensor harmonics and observed multipoles is developed in the companion framework [JanzenCRframework], whose perturbation-spectrum treatment carries the source spectrum of a closed S3, discrete by degree, projected to the sky through the flat distance slicing rather than a closed one—the flat/closed decoupling carried by the non-synchrony. That projection is that paper's; this section's own contribution to it is the harmonic-side adiabaticity above, controlled by the harmonic index alone—so the two meet at the lowest harmonics, where that paper's lowest physical mode and this section's loss of control coincide.

An explicit illustration, and its limits. To show the structure is not empty we exhibit it in the simplest cosmological model, flat Friedmann–Lemaître minisuperspace. With scale factor , conjugate momentum pa, cosmological constant Λ, and a pressureless (dust) reference fluid serving as the cosmic clock in the manner of Brown and Kucha\v{r} [BrownKuchar1995], the deparametrized gravitational Hamiltonian reduced from the Einstein–Hilbert action (in units G=1, fiducial comoving volume unity) is

(a,pa) = 2π/3 pa2/a - Λ/8πa3,% r2376+c54.9: a second stood here; amsmath keeps only one % per equation and silently dropped it,leaving two eq:Hphys dangling. Both names pointed at % this same equation,so the references were redirected to eq:Hphys rather than the label duplicated.
(9)

equal on shell to the conserved comoving dust energyP10R1. Hamilton's equation a = ∂ /∂pa = 4πpa/3a, together with = ρd on shell, gives

(a/a)2 = 8π/3 ρd/a3 + Λ/3,
(10)

the flat-ΛCDM Friedmann equation. Its solution is the sinh2/3 law

a(τ) = A sinh2/3 (3τ/2α),α= √3/Λ,
(11)

with the single scale α of the de Sitter substrate; one verifies directly that this a(τ) satisfies (11) identically. This is precisely the expansion history that the companion framework paper derives, by a wholly independent route, as the SdS expansion law of the layered construction [JanzenCRframework]: the deparametrized generator reproduces, in cosmic time, the same flat-ΛCDM evolution that the null-boundary correspondence delivers geometrically. Promoting (9) to an operator on L2 of the half-line and applying (4) gives unitary evolution of the cosmological wavefunction in cosmic time.

Two honest qualifications attach to this illustration. First, it is a minisuperspace toy: a homogeneous truncation with a dust clock, not the full Schwarzschild–de Sitter object of CR, and the operator ordering of pa2/a and the self-adjoint extension on the half-line are genuine technical questions not settled by the reduction. The illustration establishes that the deparametrized structure is consistent and reproduces the right cosmology; it does not by itself constitute the canonical quantization of the full theory. That next object—the lift to the closed-S3 layer and its propagating degrees of freedom—is carried out in Section 6. Second—and this is a feature rather than a gap—the CR cosmology is non-singular: the sinh2/3 law has no finite-cosmic-time curvature singularity, and indeed no finite layer reaches one [JanzenBHcausality, JanzenCRframework]. The usual motivation for quantizing minisuperspace, to resolve an initial singularity, therefore does not arise. The point of (4) is not singularity avoidance but the demonstration that, on the selected foliation, the canonical generator evolves rather than annihilates.

The closed-S3 lift: the graviton sector on the layer

The minisuperspace illustration of Section 5 truncates the layer to its scale factor alone; it carries no propagating degree of freedom and so cannot exhibit what the true Hamiltonian generates beyond the background expansion. The full layer does carry such a degree of freedom—the transverse-traceless shear of its spatial geometry, the graviton—and the lift of the deparametrization to it is the substantive canonical content. We carry out that lift here. Throughout, the foliation parameter is the same absolute cosmic time of Section 2: the comoving congruence of the layer, which the companion framework paper identifies with the cosmic rest frame the CMB measures and with the S3 family of the null-boundary correspondence [JanzenCRframework]. It is one congruence, carrying the flat-ΛCDM and the closed-S3 slicings as two synchronizations of itself, not two frames.

The layer is best represented by the background geometry on which the cosmology is built—the reassigned de Sitter geometry, distinct (as a Lorentzian metric) from the Schwarzschild–de Sitter cosmology it underlies but sharing its manifold and foliation [JanzenCRframework]. Its closed synchronous slicing is the evolving round three-sphere of radius a(T)=α cosh (T/α) in cosmic time . A transverse-traceless perturbation of the spatial metric decomposes into the tensor harmonics of S3, hij(T,x)=n φn(T) Y(n)ij(x), with the Y(n)ij the standard transverse-traceless rank-two harmonics of the unit three-sphere and Laplace eigenvalues μn2=n(n+2)-2, n≥2. The second-order Einstein–Hilbert action in the transverse-traceless sector reduces, mode by mode, to that of a harmonic oscillator with time-dependent mass a3 and frequency μn/a,

Sn= 12 ∫dT a3n2n2/a2 φn2],πn=a3 φn.
(12)

Read on the absolute foliation exactly as in Section 5, the constraint deparametrizes and (4) becomes

i ∂TΨ= Ψ,=nn2/2 a(T)3+ 12 a(T) μn2 φn2],
(13)

a unitary evolution in cosmic time of a tower of time-dependent oscillatorsP10R2, one per tensor harmonic. This is the lift the toy lacked: the abstract gauge-invariant degrees of freedom (qA,pA) of Section 5 are here concrete—the graviton modes φn—and the deparametrized generator advances them rather than annihilating them. Each mode is a Schrödinger oscillator on L2(R) and is manifestly self-adjoint; the closed topology of the layer enters as the discreteness of the tower, in contrast to the continuous spectra of the flat minisuperspace and planar reductions.

The same tower has a second reading, in the frame of a fundamental observer. Under the null-boundary reassignment the observer's worldline is one of the reassigned null rulings, and the layer's expansion read along it is the areal radius a(τ)=(2Mα2)1/3 sinh2/3(3τ/2α) in the observer's proper time τ—the flat-ΛCDM scale factor of the framework paper, the expansion leg of the cosmogenetic bead the framework proves one closed curve [JanzenCRframework]. The cosmic time deparametrized here is the very parameter along that bead: real on the expansion leg the observer inhabits, it is what continues off the real axis, through a bounded contour, along the bead's lap into the antecedent collapse. The tower projected into this frame is (14) with a(T) replaced by a(τ), the discrete index passing to the continuous wavenumber of the observer's locally flat slices. What distinguishes the two readings is the bend: the observer's Friedmann readout is

(a/a)2=2M/a3+1/α2,
(14)

carrying a pressureless matter term 2M/a3 that is absent from the background geometry's pure-Λ expansion, (a/a)2 →α-2. The matter the observer attributes to the graviton's background is thus the bend of the slicing—a feature of the projection, not of the layer—exactly the reclassification the framework makes for matter content generally [JanzenCRframework, JanzenOperator]. The graviton sector therefore exhibits, in one object, both faces of the layered reading: the discrete unitary tower on the ontological background, and the continuous flat-ΛCDM spectrum a real observer measures, with the matter density appearing only in the latter.

This realizes concretely the loop drawn in Section 7 with the dynamical content. The propagating degree of freedom is the transverse-traceless shear of the evolving layer, advanced by a true Hamiltonian on the absolute foliation—the same structure the companion dynamics paper exhibits for the confined polarized wave [JanzenDynamics], here for the cosmological sector and the full tensor tower. The necessity of the external clock is sharpest here: an internal (area) clock is available at Λ=0 and would serve, but at Λgt;0 it no longer separates the dynamics, and the absolute cosmic time is forced. Of the two background-sector questions, the first is settled in structure. The operator ordering and the half-line self-adjoint extension of the scale factor (Section 5) are one coupled question: in the geodesic coordinate x∝a3/2 the kinetic operator carries an inverse-square term γ/x2 at the origin whose coefficient, across the natural ordering family, attains a maximum γ= 14—strictly below the essential-self-adjointness threshold γ= 34—so the operator is limit-circle at a=0 for every ordering, while the -Λ/83 term maps to the marginal -x2 and is limit-point at a→∞, forcing no condition there. The scale-factor Hamiltonian therefore has deficiency indices (1,1) independently of the ordering [Weyl1910, ReedSimon1975]: a one-parameter family of self-adjoint extensions fixed by a single boundary condition at a=0. The ordering ambiguity cannot render the quantization unique; the residual reduces to the physical choice of that boundary condition. That choice is fixed, for the free scale-factor sector, by the geometry of the boundary itself. It is worth naming what kind of closure that is, because the corpus has a criterion for exactly this and this is its sharpest instance. A one-parameter family of self-adjoint extensionsL10 is a one-parameter family of candidate quantizations—distinct physical predictions indexed by a λ that the formalism does not pin. That is the structure the epistemic reading excludes: a structure carrying an unforced parameter is not a single world but a family, and answers “what is the world?” with a family rather than a world [JanzenShadowExistence]. What follows below is not a stipulation that removes the family but the substrate requiring its own configuration: the boundary at a=0 is the de Sitter horizon, its surface gravity is κ=1/α, and the regular Euclidean state at that κ leaves nothing to choose. The distinction that makes this the criterion's instance and not merely an analogy is worth keeping: λ indexes distinct worlds, so it is an ontological family and inadmissible as it stands, whereas a parameter that merely records an unknown datum of one world—the progenitor's mass, say—is an epistemic gap and not a family at all. The point a=0 is not a generic half-line endpoint but the de Sitter cosmological horizon—the smooth, finite-curvature metric singularity at which the comoving congruence's past null ruling closes, the substrate curvature staying finite while the comoving ruler collapses [JanzenBHcausality, JanzenOperator, JanzenCRframework]. A Killing horizon of surface gravity κ carries a thermal (Hartle–Hawking) state [HartleHawking1976], the unique state regular in the Euclidean continuation and free of a conical defect at the horizon; for the de Sitter cosmological horizon f=1-r22 gives κ= 12|f'(α)|=1/α, regularity period β=2π/κ=2πα, and the Gibbons–Hawking temperature T=ℏκ/2πkB=ℏ/2παkB [GibbonsHawking1977]. Imposed on the scale-factor wavefunction, Euclidean regularity is exactly the condition that retains the regular indicial branch x1/2+ν, ν=√γ+ 14 lt;1, and excludes the irregular admixture x1/2-ν, whose presence is a conical defect—an off-temperature state. This is the Friedrichs extension, and it is a single boundary condition: the deficiency-(1,1) freedom is thereby not merely parametrized but closed, and closed without a free parameter, since the de Sitter horizon fixes one temperature. The physical choice the ordering ambiguity left open is the horizon's own thermal state, and enters the gravitational sector here, at the seam, scaled by Λ alone—the quantum instance of the substrate's constant ledger, in which the fundamental constants enter as unit gauges over the single scale and the one place a free quantum parameter could sit is closed by the horizon's own thermal state [JanzenGeometricCore]. And that continuation is not a device brought in to close the freedom; it is the substrate's other real form. The global Wick rotation x0↦ix0 carries dS5=SO(5,1)/SO(4,1) to the compact S5=SO(6)/SO(5), and the two are the real forms of the one complex group SO(6,C) [JanzenBoundary, JanzenGeometricCore]. So the register in which enters is the same substrate read on its compact face, and the horizon—where the period is β=2πα—is where the two faces meet: the extension is fixed not by an extra assumption but by the geometry the Lorentzian reading already carries, seen from its other side. This determines the free scale-factor sector; the coupled sector below is where the open structure remains. The second background-sector question—the couplings of the tower to the scale-factor sector beyond quadratic order—sharpens this structure rather than threatening it. Deparametrizability is not at risk: the cosmic clock is a Brown–Kucha\v{r} dust fluid (Section 5), whose momentum enters the scalar constraint linearly whatever the graviton content, so the constraint solves for a true Hamiltonian at every order of the coupling—which enters as interaction terms between and the modes, not as an obstruction. The free tower above evolves on a(T) as a fixed classical background, which is why each mode is manifestly self-adjoint on L2(R); the coupling question is what happens once the scale factor is itself quantized and back-reacts, and there it acts at the a=0 boundary of the scale-factor half-line. Each mode's kinetic term πn2/2a3 is, in the geodesic coordinate, the inverse-square operator πn2/2x2 at the origin, so the boundary coefficient is promoted from the c-number γ≤ 14 of the free scale factor to an operator Γ on the tower whose spectrum straddles the 34 threshold. At leading order that spectrum is bounded below by γ and unbounded above—the operator is a sum of squares, displayed below—but the decomposition that follows uses only that both sides of the threshold are occupied, and not that the spectrum has a floor; whether the complete Γ is bounded below is not assumed here P10R10, though it does in fact follow: the full inverse-square coefficient is positive on non-degenerate metrics, so Γ=γ+cn πn2 retains its floor at γ beyond leading order, and the question of a spectrum below - 14—where ν=√Γ+ 14 would leave the reals and no regular branch would exist—has no object. The straddle itself is now a computed factP10R11: the spectrum does occupy both sides of 34, since Γ=γ+cn πn2 with c gt;0 has spec Γ=[γ,∞), and γ≤ 14 lt; 34 places spectrum strictly below the threshold while the unboundedness above places spectrum strictly above it—the negation requiring γ≥ 34, three times its own bound. That threshold is a different one from - 14, deciding a different property: 34 separates limit-point from limit-circle and so decides whether a boundary condition must be chosen at all, while - 14 decides whether a regular branch exists to choose. How the straddle falls does not bear on the closure below, which is supplied fibre by fibre and so cannot be broken by the size of the sub-threshold set R. As Γ commutes with the radial part, -∂x2+ Γ/x2 decomposes as a direct integral over its spectrum: essentially self-adjoint where Γ≥ 34—the graviton momentum makes the origin limit-point and removes the boundary freedom—and limit-circle where Γlt; 34. The single boundary condition of the free scale factor is thereby replaced, in the coupled theory, by a self-adjoint condition supported on the sub-threshold graviton subspace, its deficiency that subspace rather than a line. At leading order Γ=γ+cn πn2; but the cubic and higher self-interactions enter at the same inverse-square order at the origin (πn2φm/a3 in kind), so the complete boundary coefficient is the singular part of the interacting graviton Hamiltonian, and the ultraviolet definition of the tower sums is the open frontier—the interacting tower as a defined theory, met here at its boundary face. The spectrum is not open with it: it is computed branch by branch below, and which branch is a question the construction has been shown not to answer internally. Two things can be said about that spectrum without settling the frontier, and both bear on the decomposition. First, it is computable branch by branch: on the natural ordering family the minimum of Γ is 14 under normal ordering and 34 under symmetric ordering with one mode occupied, and the difference between the two is exactly the zero-point quantum of that mode—which is why the threshold sits at 34= 14+ 12, the free boundary coefficient plus one such quantum, rather than at a value the construction chose. Second, the two orderings answer the paper's own question oppositely: under normal ordering the origin remains limit-circle and the boundary freedom survives, while under symmetric ordering it becomes limit-point from the first occupied mode upward. The decomposition below is untouched by the choice, since it uses only that both sides of the threshold are occupied and both orderings occupy both sides; but the physical content is not, and the choice is not one this construction can make internally. Asking which ordering is asking whether the graviton tower's zero-point energy gravitates at the horizon—the cosmological-constant problem in local dress, reached from inside the boundary coefficient rather than imported. That the construction makes no such choice is an exhaustion rather than an omission. The ordering is inert in the bulk—normal and symmetric ordering differ by the c-number zero-point 12ℏωn, a global phase under the deparametrized evolution—and becomes physical only in the boundary coefficient, so any selector would have to act there; and each candidate the construction offers fails to, for a structural reason: the horizon's thermal state and the seam's characteristic structure act downstream, closing the extension given Γ (the regular branch x1/2+ν exists for either ordering); the substrate isometry, positivity, the single-scale ledger and covariance under configuration redefinition each respect both orderings; and the deparametrization, which supplies a preferred vacuum and so makes normal ordering available, does not make it mandatory—and, by solving the constraint rather than imposing it, removes the anomaly-freedom lever a Wheeler–DeWitt quantization would have used. What is left is not a residual freedom the quantization failed to close but a single physical datum—whether vacuum energy gravitates—localized precisely as one computable quantity: an epistemic gap of the kind the construction admits, not an ontological family of the kind it excludesP10R18. The boundary condition on that sub-threshold subspace, however, is supplied by the same principle that fixed the free sector. Thermal (Hartle–Hawking) regularity is Euclidean smoothness at the horizon mode by mode: across the direct integral it imposes the regular branch x1/2+ν, ν=√ Γ+ 14, on each sub-threshold fibre at the one horizon period β=2πα (the surface gravity κ=1/α belongs to the background horizon, not to the graviton content, and so is common to every fibre), and asks nothing of the limit-point fibres Γ≥ 34. The self-adjoint condition on the sub-threshold subspace is therefore the de Sitter horizon's thermal state at every order of the coupling, exactly as in the free sector; what remains open is accordingly not the boundary condition but the definition of the interacting tower—the spectrum of Γ and the ultraviolet definition of the tower sums—the first of which admits a verdict here, and it is affirmativeP10R13. The DeWitt form carries exactly one negative direction and it is the conformal one, which is why the Wheeler–DeWitt equation is hyperbolic; on transverse-traceless momenta that term drops and the form is tr((gπ)2), equal to tr(S2) for the symmetric S=LTπL with the Cholesky factor of , hence positive definite for every non-degenerate spatial metric. So the cubic term's apparent unboundedness is an artefact of truncation: π2(1-λφ+) is the expansion of π2/(1+λφ), whose full coefficient is positive wherever the metric is non-degenerate.R That sentence is the one a reader arriving at the truncated form will not have reached yet, and the distance is short enough to be worth marking: the expansion is handed over four sentences earlier, and a truncation of a positive function reads as an operator that has lost its floor. The cited receipt exists because that reading was taken—the first-order term -λφπ2 sampled alone does go arbitrarily negative, and the resummed coefficient on the same points never falls below γ. The deparametrization that yields a true Hamiltonian is the same move that yields a bounded-below one, both being the removal of the conformal direction—though the positivity speaks only of the interior, the degenerate boundary being what the thermal condition above is for. What remains genuinely open is accordingly the ultraviolet definition of the tower sums—a different thing from a residual freedom in the quantization at the boundary, and not settled by being shared with every interacting field theory. And what remains open is narrower than it was, because the coefficient's response to the coupling is settled even though the coupled sector is not. The logarithmic coefficient is the 1/m term of d(m)μ(m), hence an exact functional of the spectrum, so the deformations that could discharge it can be enumerated without solving the coupling: an overall rescale μ2→(1+ε)(m2-3) returns L=(39/4)√1+ε, which vanishes only where every frequency in the tower does. So no multiplicative renormalisation of the frequencies discharges the log—and that is the class the leading back-reaction lives in, the coupling acting through and through Γ, whose instantaneous expectation is the same sum rescaled. A mass-like shift μ2→m2-3+δ returns L=-(δ-3)(δ+13)/4, so the one such discharge is δ=3: there μn=n+1 and d(m)μ(m)=2m3-8m is a polynomial, the 1/m term not cancelling but not existing—and +3 is exactly the curvature offset that makes these frequencies non-integer.P10R15 That is a characterisation, and it can be replaced by a measurement and a structural remark, neither of which was in print.R The measurement first. The tower is a discrete sum rather than a momentum integral—the harmonics run from n≥2 with no zero mode and no soft region—so the infrared is regulated by the compactness of the layer and needs nothing. The ultraviolet is untouched by that: with μn∼n, ⟨ πn2⟩∼n in the instantaneous ground state, and a degeneracy growing as n2, the shell contribution goes as n3 and the sum diverges quartically—the ordinary zero-point degree of a field in four dimensions. The third of those inputs was carried as a scaling and is now a formula: since S3=SU(2) is parallelizable, a frame-indexed field of frame-spin is L2(SU(2)) Vs, Peter–Weyl returns level- totals of 1, 3 and 5 times (2j+1)2 for s=0,1,2—the component counts—and the transverse-traceless part is the two extreme summands, exactly two fifths of the symmetric-tracefree total. Organised by eigenvalue, the degeneracy is 2(n-1)(n+3), ten at the floor n=2, so the shell contribution is 2n3 and the leading constant is settled rather than assumedR. And the constant is the propagating-component count rather than a universal: the scalar tower's counting function grows with leading coefficient 13 against the tensor tower's 23, so the growth is n2 per propagating component and not per tensor rank. So “standard” is the right word and it is now a number. And the leading term's counterterm is one this framework already carries. The quartic piece of the one-loop vacuum energy is independent of mass and of field—it survives at m=0 and is the same for every species—so it is a constant vacuum energy, and the counterterm a constant vacuum energy requires is a cosmological-constant term. That is the framework's single dimensionful constant, absorbed into the one observed curvature with no bare-Λ-versus-vacuum split [JanzenGeometricCore]; and since P is a gauge-combination rather than a second physical length, the cutoff is not smuggling a scale in either.

The subleading term is measured on the same spectrum rather than estimated. Written in the labels m=n+1 that carry μ2=m2-3 and d=2(m2-4), the spectral zeta at the origin is ζ(0)=10 exactly—the binomial expansion terminating there, so the value is an identity and not an asymptotic estimate—and the zero-point sum's logarithmic coefficient is 39/4, the 1/m term of d μ=2m3-11m+39/4m-1+…, which a hard cutoff carrying no zeta function reproduces. And the scale factor does not enter it: the free tower's frequencies are μn/a, so factors out of the sum identically and the coefficient's independence of the expansion is exact rather than adiabatic—which is also why the coupled sector, and not a time-dependent free one, is where what remains livesP10R3.

The structural remark is about the terms after it, and it is sharper than the leading case because their counterterms are not cosmological-constant terms. Only the quadratic and logarithmic successors carry the mass, which is to say only they renormalise masses and couplings; in the standard curved-space expansion the first goes with the Ricci scalar and the second with curvature-squared invariants, and a curvature-squared coupling is not an entry in this framework's ledger. The reason that is not fatal here is a property of the backgrounds this construction admits rather than of the divergences. On a maximally symmetric geometry of radius α every curvature invariant is a pure power of 1/α2 [JanzenGeometricCore], so ∫√g R2, ∫√g RμνRμν, ∫√g RμνρσRμνρσ and ∫√g are not four independent functionals but four multiples of one; and the substrates the construction admits are a one-parameter family, the α-foliation, every descent step above the last changing the scale and nothing else [JanzenGeometricCore, JanzenAlgebroid]. So the counterterm basis is one-dimensional because the admitted background family is, and a divergence of any degree requires exactly one counterterm where a generic theory requires three.

What that argument does not reach is stated here rather than left for a reader to find, because it is the whole of what remains. A degeneracy among counterterms is a property of the background class: the functionals are distinguished by their response to varying the background, and on a one-parameter family they cannot be told apart. The first thing to check is therefore which background the tower is defined on, and it is this section's own: the closed synchronous slicing a(T)=α cosh (T/α) of §5, whose Ricci scalar is the constant 12/α2. That geometry is exactly de Sitter, so the degeneracy holds on the very background the free tower uses, and the argument above is not an appeal to a nearby object.

Where it genuinely stops is elsewhere, and the section has already named the place. The free tower evolves on a(T) as a fixed classical background; the coupled sector is what happens once the scale factor is itself quantized and back-reacts, and that is precisely the regime the boundary operator Γ belongs to. The natural worry there is that a counterterm basis is a statement about a class of fixed backgrounds, so that once the scale factor is quantized there is no fixed background left to state it on. That worry does not survive being checked, and what replaces it is sharper.

The collapse of the three quadratic invariants is not a consequence of maximal symmetry: in four dimensions their deficit Riem2-2 Ric2+ 13R2 is exactly CμνρσCμνρσ, every Friedmann geometry is conformally flat for every scale factor, and on such a geometry the Gauss–BonnetL17 combination is an exact total derivative, √g (R2-4 Ric2+ Riem2)=24 d(a3/3+ a)/dT.

So ∫√g Ric2 and ∫√g Riem2 are both fixed by ∫√g R2 up to a boundary term whatever does: no scale factor breaks it, because no scale factor can make an FRW geometry anything but conformally flatR. And because that is an identity holding pointwise in a(·) rather than an evaluation on a chosen class, it survives superposition and descends to the quantized sector as an operator relation: the coupled sector never required a class of fixed backgrounds, because the statement was never made by evaluating on one. What maximal symmetry did buy is a weaker and different thing, and that half does not survive: on a constant-curvature background terms of different dimension—∫√g, ∫√g R, ∫√g R2—are proportional as well, and they part company as soon as is not the de Sitter cosh, as the geometric layer's running Ricci scalar shows directly. So the place the degeneracy genuinely ends is not the scale factor but the shear. The deficit is C2; for an anisotropic shear over an isotropic expansion the invariant is C2=2ii+Hσi)2 at second order in the amplitudeP10R4—so it carries two derivatives more than the shear itself, and for a mode of frequency ω it grows as ω2σ2, which is what makes it ultraviolet-sensitive at all; and the propagating content of this tower is the transverse-traceless shear. So what remains is the tower's own shear, which is a calculation and not a question about meaning—entering at second order in the mode amplitude, with the sub-leading heat-kernel coefficients as its instrument. That calculation is run, and its answer is smaller than the question sounds: for a transverse-traceless perturbation the first variation of the Ricci scalar vanishes identically and √g is unchanged, so R2 at second order in the amplitude is 2 R times at that order—pointwise, with no integration by parts—and ∫√g R2 is accordingly a multiple of the Einstein–Hilbert term rather than a new structure.

With the Gauss–Bonnet combination contributing no field equation, the three quadratic invariants leave ∫√g R2 and ∫√g C2, of which only the second is new: the shear therefore costs exactly one new counterterm, and it is the Weyl-squared oneR.

And its coefficient follows from what the tower is, without a second-order spectrum. Each mode is a harmonic oscillator of mass a3 and frequency μn/a, which is term for term the reduction of a minimally coupled massless scalar on this background, so the tower is two such degrees of freedom carrying the transverse-traceless spectrum. The C2 coefficient is a property of the field content rather than of the background, which is why it is fixed without one: for a single real scalar the entire C2 content of the second heat-kernel coefficient [Gilkey1975] sits in 2 Riem2-2 Ric2—independently of the curvature coupling, which is why the answer needs none—and that combination is 3C2-E4, giving 1/120 in units of (4π)-2 and therefore 1/60 for the towerP10R6: exactly twice a real scalar's. The count is of physical modes, and that is the reading on which the number stands: the constraints here are solved rather than gauge-fixed, so no ghost sector enters and no covariant spin-2 tabulation applies. The overall normalisation by which the coefficient enters a divergence is convention-dependent; the ratio is not.

Two things about that entry are settled and belong beside it. First, the two helicities are not identified by any symmetry the layer connectedly carries: on S3= SU(2) the connected isometry group is (SU(2)L×SU(2)R)/ Z2, transverse-traceless rank two carries |jL-jR|=2, and each level is (j,j+2)⊕(j+2,j) with 2j+1=n-1—whose dimensions sum to exactly the 2(n-1)(n+3) derived aboveP10R5. They are inequivalent irreducibles, and the map exchanging them is the exchange of the two factors, an orientation-reversing isometry—so a parity-odd term is not excluded by the geometry, and whatever excludes it does so through the state. Second, a topological term contributes no field equation, so a coefficient multiplying one is not read off any dynamics; its only remaining home is the horizon entropy, on which this construction is deliberately uncommitted [JanzenGeometricCore]. So whether such a term is an entry in this ledger is not a separate question from that one.

One caveat belongs in the statement rather than after it: the dimension-four scalars also include the parity-odd Pontryagin density, which is not a curvature-squared invariant of the kind counted above and is a total derivative, but which is non-zero at second order for a circularly polarised mode and reverses with the handedness—a linearly polarised mode returns zero for it, and the corpus carries a chirality [JanzenDynamics], so the zero is a property of the mode chosen and not of the geometry.

And what that scopes, first of all, is this computation. A counterterm answers to a parity-odd divergence of the effective action, which is a property of the theory and the state; it is not a property of a basis mode. The two helicities span the same space in either polarisation basis, and on a parity-symmetric state the two contributions cancel whatever an individual basis element returns. So a mode-level evaluation cannot fix what counterterm the theory needs, in either direction — the caveat bounds its own instrument rather than deferring the question to a choice of polarisation.

Two things would have to be settled before a parity-odd term could be scored at all, and they are independent. Whether the tower is chiral on the corpus's own criterion — which is not that a reflection exists but that no connected action completes it, a condition applied to the radiating sector and not to this one. And whether a total derivative is a ledger entry. The density above contributes no field equation, so it is not a coupling in the sense the constant-counting audit means, and the ledger has taken no position on topological terms because none has arisen before.

The propagating sector itself is a clean, unitary, deparametrized evolution—a true Hamiltonian generating the graviton on the layer, in cosmic time.

Dissolution, not solution

The result of Sections 45 is best stated negatively. We have added nothing to the formalism. We have not introduced a new time variable into general relativity, nor a matter field whose role is to be a clock, nor a modification of the constraint algebra. We have identified, on external grounds, which foliation is physically real, and read the existing constraint on it. The problem of time, on this account, was never a problem internal to the formalism; it was the formalism faithfully reporting the consequences of an ontological premise—the block—that is both a category error and empirically false.

This is why the appropriate verdict is dissolution rather than solution, and the distinction is not merely rhetorical. A solution would add structure to make a defective formalism work. A dissolution removes a mistaken premise and finds the formalism was working all along. The four epistemic rules that govern such corrections [JanzenFortress, JanzenShadowExistence]—resist the naïve identification of appearance with reality; prefer a reading on which the observed structure is a structural necessity rather than a tuned permission; consolidate phenomena under one principle; treat accumulating patches as a red flag—each favour the CR reading over the frozen one. The cosmic time is a structural necessity of the ontology and an empirical datum, not a tuned addition. The reading consolidates: the same correction that turns the frozen constraint into a true Hamiltonian also dissolves the inference that gravitational collapse completes in finite cosmic time, since both inferences—the timeless wavefunction and the completed horizon—rest on granting existence to a manifold of occurrences that no observer's present ever contains [JanzenBHcausality, JanzenFortress]. One ontological correction, two canonical payoffs.

The reading also closes a loop with the dynamical content of the programme. The true Hamiltonian generates the advance of the layer ; the geometry of that advance is what the operator and range papers read directly, where the matter content of a layer is the bend of its spatial cut off the vacuum profile and gravitational radiation is the transverse-traceless shear of the evolving layer, up to the wall at which a symmetric layer can no longer carry the wave and ordinary inhomogeneous evolution begins [JanzenOperator, JanzenRange]. The canonical face (a Hamiltonian that advances the layer) and the geometric face (matter and radiation as features of the advancing layer's intrinsic geometry) are two descriptions of the one evolving three-dimensional world. The cosmogenesis re-expansion is one such advance: the companion cosmogenesis paper [JanzenCosmogenesis] runs the collapse-and-re-expansion thermal history—the layer's advance along cosmic time, generated by this true Hamiltonian rather than frozen—through a nuclear network to the primordial light-element abundances. The companion foundation roots these faces in a single augmentation of general relativity [JanzenModernParallax]; the present paper supplies the canonical one, and with it the recognition that CR's distinctive contribution to quantum gravity is not a new dynamics but an absolute cosmic time—real, forced, and already implicit in the formalism—that turns the constraint into a generator. This dissolution is the canonical face of the substrate's maximal symmetry gathered in the geometric core [JanzenGeometricCore]: the problem of time is identified in the constraint-algebroid construction as the base-dependence of the substrate's coset metric [JanzenAlgebroid], and the selection of the forced foliation is what deparametrizes it away—the structural and the canonical sides of one dissolution.

Relation to existing approaches

The deparametrization carried out in Section 5 is, as a technique, entirely standard, and it is important to be clear about what is and is not new here. Kucha\v{r}'s survey [Kuchar1992] classifies responses to the problem of time into those that locate an internal time before quantization, those that quantize first and seek time afterwards, and those that abandon time outright; Isham's review [Isham1993] maps the same terrain. The construction of Section 5 sits squarely in the first class, and its minisuperspace realization uses a dust clock of exactly the Brown–Kucha\v{r} type [BrownKuchar1995]. We claim no novelty in the mechanism.

What CR adds is not a mechanism but a warrant. The standard and well-known objection to internal-time approaches is the multiple-choice problem: many candidate internal times exist, inequivalent quantizations follow from different choices, and the formalism provides no principle to prefer one [Kuchar1992, Isham1993]. This objection has force precisely when the choice of clock is a matter of formal convenience internal to the theory. It loses that force when the clock is fixed from outside the formalism by ontology and observation. CR's cosmic time is not selected because it makes the equations tractable; it is selected because the occurrence/existence distinction identifies the evolving layer as what exists, and because the CMB measures the corresponding cosmic rest frame (Section 2). The multiple-choice problem is thus not solved within the space of formal clocks but dissolved by the recognition that one clock is physically real and the others are not. This is the same pattern as the rest of the paper: a difficulty that is genuine so long as a mistaken premise is held, and that disappears with the premise.

The timeless and relational programmes—Page and Wootters' conditional probabilities [PageWootters1983], Rovelli's relational quantum mechanics and evolving constants of motion [Rovelli2004], Barbour's denial of fundamental time [BarbourEnd]—take the opposite path with full consistency: they accept that no preferred foliation exists and reconstruct the appearance of time from correlations within a fundamentally timeless structure. We do not claim these programmes are internally flawed. We claim that the premise they share—that there is no objective cosmic now—is the very premise the CMB refutes [JanzenModernParallax], and that once a real cosmic time is admitted, the elaborate reconstruction of temporal appearance from timeless correlations is solving a problem that no longer arises. The choice between the programmes is, in the end, the choice of Section 2: whether to grant the manifold of occurrences the existence that the evidence assigns to the evolving layer.

Conclusion

The canonical problem of time is the block universe in Hamiltonian dress. Read the four-dimensional manifold as the existent, and the constraint correctly reports that nothing evolves; read the evolving three-dimensional world as the existent and its record as the manifold, and the same constraint, deparametrized along the cosmic time that the universe has let us measure, is a true Hamiltonian generating a unitary advance that reproduces the observed flat-ΛCDM expansion. Lifted beyond the background to the layer's transverse-traceless sector, that same Hamiltonian advances the graviton tower of the closed-S3 layer unitarily—the propagating degree of freedom a fundamental observer reads as the flat-ΛCDM graviton, with matter the bend of its slicing rather than an ontological content. The equations never changed. What changed was the answer to a single question—what exists—and that answer is not a matter of taste but one the occurrence/existence distinction and the isotropy of the CMB settle together. The problem of time was the canonical symptom of a category error; read without it, the formalism was describing a real cosmic time all along. Read so, the dissolution is one of a family: the same distinction that turns the frozen constraint into a true Hamiltonian is shown, in the companion framework paper's first synthesis, to dissolve a wider set of general relativity's standing problems together—the problem of time among them, and the unitary evolution established here underwriting the resolution of the black-hole information paradox on the realised, globally hyperbolic spacetime [JanzenCRframework]. That places the canonical face within the framework's one synthesis: the maximally symmetric de Sitter substrate the framework reads at once as general relativity's solution space [JanzenRange], as the discrete and charge structure, and as the gauge sector on its conjugate real form, is read here on its canonical constraint—where the deparametrized generator is the layer's true Hamiltonian, and the quantum of action enters the gravitational sector at the seam, scaled by Λ alone [JanzenGeometricCore].