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Shadow Theory

Chapter 11

Parameters, Scales, and Renormalization

From A Source-to-Readout Architecture for a Theory of Everything, Version 1.0 (July 2026) · doi:10.5281/zenodo.21366204

11.1 Role and Scope

Chapter 11 develops the parameter structure of the theory. It classifies interface constants, calibration invariants, dimensionless parameters, empirical inputs and derived quantities across the quantum, geometric, matter, cosmological and record sectors, and it fixes the renormalization-group and threshold-matching structure connecting parameter values at different scales.

Chapter 11 receives matter and flavor parameters from Chapters 9–10, and prepares cosmological and dark-sector parameter handoffs for Chapters 12–13. It does not derive exact numerical values unless an explicit derivation is supplied. Its role is classification, counting, dimensional/status assignment, and proof-route control.

The relevant open problems are the parameter-fixation programme R5 of Chapter 17 and, for the cosmological and dark-sector parameters routed explicitly to Chapters 12 and 13, the programme R6.


A theory may determine a form of dynamics without determining every numerical parameter appearing in it. Shadow Theory therefore distinguishes four scientifically different situations: a parameter may be derived from source invariants, constrained to a finite or continuous family, calibrated from data, or left unresolved. These cases must not be conflated.

11.2 Parameter spaces and source constraints

For a selected physical branch bb, let Θb(μ)\Theta_b(\mu) be its renormalized parameter space at scheme and scale (s,μ)(\mathfrak s,\mu), modulo gauge redundancy and field redefinitions. It contains the gauge couplings, Higgs parameters, Yukawa matrices, neutrino parameters, topological angles, gravitational couplings, and the cosmological or dark-sector parameters belonging to that branch.

The source realization supplies invariant data Ib(Y)I_b(Y), and parameter fixation is the set-valued relation FixParam\operatorname{FixParam} constructed later in this chapter. That relation may be empty, a unique equivalence class, a finite family, or a positive-dimensional set; those possibilities are mathematical properties of the constraint system, not labels assigned in advance. Local identifiability, degeneracy, and uncertainty are governed by the Jacobian analysis developed with the relation itself.

11.3 Renormalization-group evolution and matching

Renormalized parameters satisfy

μdθadμ=βa(θ).\mu\frac{d\theta^a}{d\mu}=\beta^a(\theta).

For gauge couplings at one loop,

μdgidμ=bi16π2gi3,αi1(μ)=αi1(μ0)bi2πlnμμ0.\mu\frac{dg_i}{d\mu}=\frac{b_i}{16\pi^2}g_i^3, \qquad \alpha_i^{-1}(\mu)=\alpha_i^{-1}(\mu_0) -\frac{b_i}{2\pi}\ln\frac{\mu}{\mu_0}.

With the SU(5)SU(5)-normalized g1=5/3gYg_1=\sqrt{5/3}\,g_Y, the minimal Standard Model coefficients are

(b1,b2,b3)=(4110,196,7).(b_1,b_2,b_3)=\left(\frac{41}{10},-\frac{19}{6},-7\right).

If the ordinary coupling gYg_Y is used instead, its coefficient is bY=41/6b_Y=41/6; explicitly,

μdgYdμ=41/616π2gY3,μdg1dμ=41/1016π2g13.\mu\frac{dg_Y}{d\mu} = \frac{41/6}{16\pi^2}g_Y^3, \qquad \mu\frac{dg_1}{d\mu} = \frac{41/10}{16\pi^2}g_1^3.

The convention must be stated rather than mixed, and the electroweak angle always uses gY/g2g_Y/g_2, not g1/g2g_1/g_2. Systematic multi-loop RG machinery follows [46].

Across a threshold MnM_n,

θ(n1)(Mn)=Mn(θ(n)(Mn),Mn),\theta^{(n-1)}(M_n) =\mathcal M_n\bigl(\theta^{(n)}(M_n),M_n\bigr),

where Mn\mathcal M_n is the matching map appropriate to the chosen renormalization scheme and operator basis. Successive matching maps must compose consistently when several thresholds are crossed.

11.4 Parameter classification

The principal parameter families are:

QuantityDimensionDefining equationBasis in the present theory
GR,ΛbrG_R,\Lambda_{\rm br}M2,M2M^{-2},M^2gravitational actionsource-derived, constrained, or calibrated branch value
g3,g2,gYg_3,g_2,g_Y1covariant derivative and RG flowvalues at stated (μ,s)(\mu,\mathfrak s)
μH,λH,v\mu_H,\lambda_H,vM,1,MM,1,MHiggs potentialR5 quantities
Yukawa eigenvalues and mixings1mass and mixing equationsR5 quantities
neutrino masses and phasesM,1M,1selected neutrino branchbranch-dependent R5 quantities
θˉ\bar\theta1topological termstrong-CP question
H0,Ωi0H_0,\Omega_{i0}M,1M,1FLRW equationscosmological branch inputs or outputs
dark-sector functionsbranch-dependentChapter 13 action or kinetic descriptionR6 quantities

“Derived” is reserved for a quantity obtained from Ib(Y)I_b(Y) without using that quantity or an equivalent observable as an input. Calibration and derivation remain distinct even when both produce a precise number. For an observable OO and independent input aja_j, a conventional local sensitivity measure is

Δaj(O)=lnOlnaj,ΔBG(O)=maxjΔaj(O).\Delta_{a_j}(O)=\left|\frac{\partial\ln O}{\partial\ln a_j}\right|, \qquad \Delta_{\rm BG}(O)=\max_j\Delta_{a_j}(O).

Naturalness is a statement about such declared sensitivities and radiative stability, not a substitute for a source derivation.

11.5 R5 theorem target

R5 is staged. After R2 and R4 select a matter/QFT branch, source-invariant constraints FbF_b, locally well-posed beta functions, consistent threshold maps, and an effective-theory domain containing the full trajectory define the matter/QFT parameter set FixParamM\operatorname{FixParam}_M and its identifiability, uncertainty, and scheme-equivalence class. Gravitational parameters are classified conditionally only after an admitted R3 branch exists. Cosmology-dependent parameters enter FixParamC\operatorname{FixParam}_C only after R6 has supplied a background and perturbation solution. No quantity classified at the post-R6 stage may be used as an upstream input to its own claimed derivation. Numerical masses, mixings, and cosmological parameters are companion-paper calculations built from this staged structure.

11.6 Parameter theory space and provenance

For a selected branch bb, a maximum EFT operator dimension DD, and loop/truncation order LL, let

Θb(D,L)(μ,s)\boxed{ \Theta_b^{(D,L)}(\mu,\mathfrak s) }

be the parameter manifold at scale μ\mu and renormalization scheme s\mathfrak s, modulo gauge redundancy, field redefinitions, flavor-basis transformations, and declared scheme equivalence. The truncation (D,L)(D,L) and its error are part of every output. No finite calculation is represented as fixation of an infinite EFT tower.

The parameter vector contains, as applicable:

  • gY,g2,g3g_Y,g_2,g_3;

  • Higgs mass and quartic parameters;

  • Yukawa matrices and mixing invariants;

  • neutrino coefficients and thresholds;

  • θˉ\bar\theta;

  • GR,ΛR,Q,αi,cnAG_R,\Lambda_R,\ell_Q,\alpha_i,c_{nA};

  • vv_\star;

  • Mrec,ZR,YR,ξR,m^R,λ3R,λ4RM_{\rm rec},Z_R,Y_R,\xi_R,\widehat m_R,\lambda_{3R},\lambda_{4R};

  • HT flux/boundary parameters on that branch;

  • cosmological and dark-sector parameters owned by their modules.

Each source invariant is a record

IA=(value,type,dimension,scale law,covariance,uncertainty,provenance,derivation pointer).I_A = (\text{value},\text{type},\text{dimension}, \text{scale law},\text{covariance}, \text{uncertainty},\text{provenance}, \text{derivation pointer}).

Allowed provenance labels are:

  • source-derived;

  • branch-selected;

  • interface convention;

  • empirically calibrated;

  • externally dependent;

  • unresolved.

An empirical datum cannot later be relabeled source-derived.

11.7 Realization-induced parameter constraints

Let

Ξb:IsrcIbreadout\Xi_b: \mathsf I_{\rm src} \longrightarrow \mathsf I_b^{\rm readout}

be the invariant comparison map induced by the source-to-readout descent and the selected matter/geometry branch. Let

Invb:Θb(D,L)Ibreadout\operatorname{Inv}_b: \Theta_b^{(D,L)} \longrightarrow \mathsf I_b^{\rm readout}

compute the same typed invariants from a parameter representative. Neither map is chosen using observed target parameter values.

Let ΔI\Delta_{\mathsf I} be the fixed equality/defect map on the typed invariant fiber. Define

Fb(θ;Isrc)=ΔI(Invb(θ),Ξb(Isrc)).\boxed{ F_b(\theta;I_{\rm src}) = \Delta_{\mathsf I} \left( \operatorname{Inv}_b(\theta), \Xi_b(I_{\rm src}) \right). }

For exact discrete invariants, zero defect means equality. For continuous invariants with a declared uncertainty object, zero means membership in the predeclared invariant interval or equivalence class. The defect map, its tolerance, and its provenance are fixed before empirical comparison.

At a source/matching scale μ\mu_\star, define

S={[θ]:Fb(θ;Isrc)=0,Gθ(θ)=1}.\boxed{ \mathcal S_\star = \left\{ [\theta_\star]: F_b(\theta_\star;I_{\rm src})=0, \quad G_\theta(\theta_\star)=1 \right\}. }

The gate GθG_\theta contains positivity, unitarity, vacuum stability, branch consistency, EFT-domain, and dimensional requirements.

11.8 FixParam relation

The parameter-fixation machinery is the set-valued relation

FixParam:Isrc×Branch×R>0×Scheme×MatchDataParamSolution.\boxed{ \operatorname{FixParam}: \mathsf I_{\rm src} \times\mathsf{Branch} \times\mathbb R_{>0} \times\mathsf{Scheme} \times\mathsf{MatchData} \rightrightarrows \mathsf{ParamSolution}. }

For every θS\theta_\star\in\mathcal S_\star, evolve

μdθadμ=βba(θ;s).\boxed{ \mu\frac{d\theta^a}{d\mu} = \beta_b^a(\theta;\mathfrak s). }

At a threshold MjM_j, impose

θ(j1)(Mj)=Mjsjsj1[θ(j)(Mj);Mj,Dj].\boxed{ \theta^{(j-1)}(M_j) = \mathcal M_j^{\mathfrak s_j\to\mathfrak s_{j-1}} \left[ \theta^{(j)}(M_j);M_j,\mathcal D_j \right]. }

If MjM_j depends on θ\theta, the mass and matching equations are solved simultaneously. Matching maps satisfy the cocycle condition

M20=M10M21+O(L+1).\boxed{ \mathcal M_{2\to0} = \mathcal M_{1\to0} \circ \mathcal M_{2\to1} +O(L+1). }

The output is

FixParam()={([θ(μ)]scheme,Nnull,Σθ,Pprov,Etrunc,Nsens,Sstatus)}.\boxed{ \operatorname{FixParam}(\cdots) = \left\{ ([\theta(\mu)]_{\rm scheme}, \mathcal N_{\rm null}, \Sigma_\theta, \mathcal P_{\rm prov}, \mathcal E_{\rm trunc}, \mathcal N_{\rm sens}, \mathcal S_{\rm status}) \right\}. }

An empty solution set, finite branch degeneracy, continuous solution manifold, or unique solution is returned explicitly.

11.9 Scheme covariance

For a scheme change

θ=fss(θ),\theta'=f_{\mathfrak s\to\mathfrak s'}(\theta),

require

β(θ)=Df(θ)β(θ),\boxed{ \beta'(\theta') = Df(\theta)\,\beta(\theta), } Fb(θ;I)=Fb(f1(θ);I),\boxed{ F_b'(\theta';I) = F_b(f^{-1}(\theta');I), }

and

O(θ,s)=O(θ,s)+O(L+1)\mathcal O(\theta,\mathfrak s) = \mathcal O(\theta',\mathfrak s') +O(L+1)

for physical observables. A scheme-dependent coupling is not a source invariant by itself.

11.10 Identifiability and degeneracy

Let n=dimΘb(D,L)n=\dim\Theta_b^{(D,L)} after quotienting redundancies and define

JAa=FAθa.J_{Aa} = \frac{\partial F_A}{\partial\theta^a}.

Local identifiability requires

rankJ=n.\boxed{ \operatorname{rank}J=n. }

If rankJ=r<n\operatorname{rank}J=r\lt n, the local solution has at least nrn-r unresolved directions. These form Nnull\mathcal N_{\rm null} and are not assigned zero uncertainty. Global uniqueness additionally requires injectivity of the invariant/RG/matching map modulo declared equivalences. Disconnected solutions are returned as a branch-degenerate solution family.

11.11 Uncertainty and sensitivity

At an isolated square regular solution,

Σθ=J1ΣI(J1)T+Σmatch.\boxed{ \Sigma_{\theta_\star} = J^{-1}\Sigma_I(J^{-1})^T +\Sigma_{\rm match}. }

In the general identifiable subspace use the covariance-weighted pseudoinverse:

Σθid=J+ΣI(J+)T.\boxed{ \Sigma_{\theta}^{\rm id} = J^+\Sigma_I(J^+)^T. }

Let U(μ,μ)U(\mu,\mu_\star) be the linearized RG propagator. Then

Σθ(μ)=UΣθUT+ΣRG+Σthreshold.\Sigma_\theta(\mu) = U\Sigma_{\theta_\star}U^T +\Sigma_{\rm RG} +\Sigma_{\rm threshold}.

For an observable O\mathcal O,

ΣO=DθOΣθ(DθO)T.\Sigma_{\mathcal O} = D_\theta\mathcal O \,\Sigma_\theta\, (D_\theta\mathcal O)^T.

Exact source invariants have no statistical covariance unless the source theory supplies a measure or approximation error. Source-distribution, empirical-calibration, numerical, and truncation errors remain separately typed.

Define source sensitivity

ΔaA=logθalogIA.\boxed{ \Delta_{aA} = \left| \frac{\partial\log\theta^a} {\partial\log I_A} \right|. }

A Barbieri–Giudice-type diagnostic is

ΔBG=maxplogv2logp,\Delta_{\rm BG} = \max_p \left| \frac{\partial\log v^2}{\partial\log p} \right|,

with basis, scale, and scheme recorded. Naturalness classes are symmetry-protected, multiplicatively stable, fixed-point-controlled, low-sensitivity, high-sensitivity (tuned), branch-selected, not derived, empirically calibrated, and unclassified. Classification is not parameter derivation.

11.12 Interface Constants

SymbolDimensionChannel(s)RoleDefault ConventionRestored WhenStatusOpen Problem
ccspeedΠG,ΠC\Pi_G,\Pi_Ccausal/metric conversionc=1c=1causal cones, metric dimensional interpretation, cosmology unitsinterface constantnone
\hbaractionΠQ,ΠM\Pi_Q,\Pi_Mquantum action scale=1\hbar=1quantum dimensional interpretation, path integrals, Planck-scale expressionsinterface constantnone
GGgravitational couplingΠG,ΠC\Pi_G,\Pi_Cgeometry-matter conversionexplicit in gravitational equationsEinstein equations, Planck units, cosmological normalizationcalibration invariant / dimensionless residue through ratiosR5R5
kBk_Bentropy/temperature conversionΠC,ΠR\Pi_C,\Pi_Rthermodynamic entropy conversionkB=1k_B=1 where naturalentropy, thermodynamic arrow, temperature dimensionsinterface constantnone

The gravitational constant GG also participates in dimensionless pressure ratios through the Planck mass

MP=G1/2(11.1)\boxed{ M_P=G^{-1/2} } \tag{11.1}

in natural units.


11.13 Standard Model Parameter Table

11.13.1 5.1 Enumerated Minimal Standard Model Parameters

ClassSymbolsCountDimensionChannelStatusOpen ProblemDefined In
Gauge couplingsg1=5/3gYg_1{=}\sqrt{5/3}\,g_Y, g2g_2, g3g_33dimensionlessΠM\Pi_Mdimensionless residueR5R5Chapters 9, 11, 16, 17
Higgs potentialμH,λH\mu_H,\lambda_H2mass, dimensionlessΠM\Pi_Mderivation openR5R5Chapters 9, 11, 17
Quark Yukawa eigenvaluesyuy_u, ycy_c, yty_t, ydy_d, ysy_s, yby_b6dimensionlessΠM\Pi_Mdimensionless residueR5R5Chapters 10, 11, 17
Charged lepton Yukawa eigenvaluesye,yμ,yτy_e,y_\mu,y_\tau3dimensionlessΠM\Pi_Mdimensionless residueR5R5Chapters 10, 11, 17
CKM anglesθ12q,θ23q,θ13q\theta_{12}^q,\theta_{23}^q,\theta_{13}^q3dimensionlessΠM\Pi_Mdimensionless residueR5R5Chapters 10, 11, 17
CKM CP phaseδCKM\delta_{\mathrm{CKM}}1dimensionless phaseΠM\Pi_Mdimensionless residueR5R5Chapters 10, 11, 17
QCD thetaθQCD\theta_{\mathrm{QCD}} or θˉ\bar\theta1dimensionless phaseΠM\Pi_Mdimensionless residueR5R5Chapters 10, 11, 17

A conventional minimal Standard Model count without neutrino masses is

3 gauge couplings+2 Higgs parameters+9 charged-fermion Yukawa eigenvalues+4 CKM parameters+1 QCD theta parameter=19.(11.2)\boxed{ \begin{aligned} &3\ \text{gauge couplings} + 2\ \text{Higgs parameters} \\ &\quad + 9\ \text{charged-fermion Yukawa eigenvalues} \\ &\quad + 4\ \text{CKM parameters} + 1\ \text{QCD theta parameter} = 19. \end{aligned} } \tag{11.2}

Neutrino parameters are counted separately in Section 6.

11.13.2 5.2 Higgs and Yukawa Relations

Chapter 9 supplied

Mf=v2Yf,mfi=v2yfi.(11.3)\boxed{ M_f=\frac{v}{\sqrt2}Y_f, \qquad m_{fi}=\frac{v}{\sqrt2}y_{fi}. } \tag{11.3}

The Higgs vacuum scale satisfies

v=μHλH.(11.4)\boxed{ v=\frac{\mu_H}{\sqrt{\lambda_H}}. } \tag{11.4}

The electroweak scale and Yukawa eigenvalues are parameter-table entries, not source-derived constants at Chapter 11 level.


11.14 Neutrino Parameter Branches

11.14.1 6.1 Dirac Branch

Parameter ClassSymbolsCountDimensionStatusOpen ProblemDefined In
Neutrino masses/eigenvaluesmν1m_{\nu_1}, mν2m_{\nu_2}, mν3m_{\nu_3} or yνiy_{\nu_i}3mass or dimensionless Yukawaderivation openR5R5Chapters 10, 11, 17
PMNS anglesθ12\theta_{12}^{\ell}, θ23\theta_{23}^{\ell}, θ13\theta_{13}^{\ell}3dimensionlessdimensionless residueR5R5Chapters 10, 11, 17
Dirac CP phaseδPMNS\delta_{\mathrm{PMNS}}1phasedimensionless residueR5R5Chapters 10, 11, 17

Under this convention,

NνDirac=7.(11.5)\boxed{ N_{\nu}^{Dirac}=7. } \tag{11.5}

11.14.2 6.2 Majorana Branch

Parameter ClassSymbolsCountDimensionStatusOpen ProblemDefined In
Neutrino massesmν1,mν2,mν3m_{\nu_1},m_{\nu_2},m_{\nu_3}3massderivation openR5R5Chapters 10, 11, 17
PMNS anglesθ12\theta_{12}^{\ell}, θ23\theta_{23}^{\ell}, θ13\theta_{13}^{\ell}3dimensionlessdimensionless residueR5R5Chapters 10, 11, 17
Dirac phaseδPMNS\delta_{\mathrm{PMNS}}1phasedimensionless residueR5R5Chapters 10, 11, 17
Majorana phasesα1,α2\alpha_1,\alpha_22phasedimensionless residueR5R5Chapters 10, 11, 17
Heavy seesaw scalesMRM_R eigenvaluesbranch-dependentmassderivation openR5R5Chapters 10, 11, 17

For the light-neutrino Majorana phase count,

NνMaj=9.(11.6)\boxed{ N_{\nu}^{Maj}=9. } \tag{11.6}

Heavy Majorana mass scales MRM_R are additional branch parameters in seesaw models.


11.15 Cosmology and Dark-Sector Parameter Table

SymbolRoleDimensionChannelProvenanceOpen ProblemDefined In
H0H_0present expansion scaleinverse timeΠC\Pi_Cempirical input / derivation openR6R6Chapter 12
Ωb\Omega_bbaryon density fractiondimensionlessΠC\Pi_Cempirical input / dimensionless residueR6R6Chapter 12
Ωr\Omega_rradiation density fractiondimensionlessΠC\Pi_Cempirical input / dimensionless residueR6R6Chapter 12
Ωk\Omega_kcurvature density fractiondimensionlessΠC\Pi_Cempirical input / dimensionless residueR6R6Chapter 12
ΩDM\Omega_{DM}dark matter density fractiondimensionlessΠC\Pi_Cdimensionless residueR6R6Chapters 12, 13
ΩC\Omega_Cdark energy/closure-sector fractiondimensionlessΠC\Pi_Cdimensionless residueR6R6Chapters 12, 13
Λ\Lambdacosmological constantinverse length squaredΠC,ΠG\Pi_C,\Pi_Gdimensionless residue through ratiosR6R6Chapter 13
ρΛ\rho_\Lambdavacuum/dark energy densityenergy densityΠC\Pi_Cdimensionless residue through ratiosR6R6Chapter 13
ρC0\rho_{C0}closure-sector present densityenergy densityΠC\Pi_Cderivation openR6R6Chapter 13
FC(a)F_C(a)closure-sector evolution functiondimensionless functionΠC\Pi_Cderivation openR6R6Chapter 13
w(a)w(a)dark-energy equation of statedimensionless functionΠC\Pi_Cderivation openR6R6Chapter 13
ρprim\rho_{prim}primordial dark componentenergy densityΠC\Pi_Cderivation openR6R6Chapter 13
ρind\rho_{ind}induced dark componentenergy densityΠC\Pi_Cderivation openR6R6Chapter 13
Bcoslow\mathcal B_{cos}^{low}low-boundary cosmological conditionboundary dataΠC\Pi_Cderivation openR6R6Chapters 12, 14

11.16 Record/Objectivity Calibration Parameters

SymbolRoleDimensionChannelProvenanceOpen ProblemDefined In
ZminZ_{\min}objectivity thresholdmodel-dependent / dimensionlessΠR\Pi_Rcalibration invariantR9R9 / Chapter 17 calibrationChapters 6, 16
SminS_{\min}persistence thresholdmodel-dependent / dimensionlessΠR\Pi_Rcalibration invariantR9R9 / Chapter 17 calibrationChapters 6, 16
Δt\Delta trecord persistence intervaltimeΠR,ΠC\Pi_R,\Pi_Ccalibration invariantR9R9 / Chapter 17 calibrationChapters 6, 14, 16
FZF_Z parametersobjectivity-index calibrationmodel-dependentΠR\Pi_Rcalibration invariantR9R9 / Chapter 17 calibrationChapters 6, 16

The selector χi\chi_i is not a parameter-table entry. It is a realization selector under R7.


11.17 QFT Renormalization and Threshold Structure

Every renormalized parameter entry carries the QFT provenance fields fixed by the QFT sector: the scheme s\mathfrak s, the renormalization scale μ\mu, the beta-function system and truncation order, the threshold-matching data across mass scales, and the residual scheme/truncation uncertainty. The feedback is the scheme-qualified loop KinQFTKoutK_{\rm in}\to QFT\to K_{\rm out} with compatibility KoutschemeKinK_{\rm out}\sim_{\rm scheme}K_{\rm in}; it is distinct from empirical calibration feedback KcalKinK_{\rm cal}\to K_{\rm in}, which is allowed only inside a declared calibration iteration and can never be cited as source derivation. Extraction of running couplings from the QFT sector establishes provenance, not R5 discharge.

Decoupling and threshold matching follow [47]; the effective-Lagrangian framework follows [43].

11.18 Dimensionless Closure-Pressure Ratios

The central dimensionless pressure ratios include

α,αs,mfv,mνv.(11.7)\boxed{ \alpha,\qquad \alpha_s,\qquad \frac{m_f}{v},\qquad \frac{m_\nu}{v}. } \tag{11.7}

They also include

mHMP,vMP,Ωi,ρΛMP4.(11.8)\boxed{ \frac{m_H}{M_P}, \qquad \frac{v}{M_P}, \qquad \Omega_i, \qquad \frac{\rho_\Lambda}{M_P^4}. } \tag{11.8}

The CP and mixing pressure quantities include

θˉ,JCKM,JPMNS.(11.9)\boxed{ \bar\theta, \qquad J_{\mathrm{CKM}}, \qquad J_{\mathrm{PMNS}}. } \tag{11.9}

These ratios and invariants are the primary R5/R6R5/R6 pressure points because they are dimensionless or convention-independent and cannot be removed by unit choice.


11.19 Parameter Count Reconciliation

  • Parameter-count reconciliation:

    • SM minimal no neutrinos:

      • Count: 19

      • Convention:

        • 3 gauge couplings

        • 2 Higgs parameters

        • 9 charged-fermion Yukawa eigenvalues

        • 4 CKM parameters

        • 1 QCD theta parameter

    • Neutrino Dirac extension:

      • Count: “+7”

      • Convention:

        • 3 neutrino masses/eigenvalues

        • 3 PMNS angles

        • 1 Dirac CP phase

    • Neutrino Majorana extension:

      • Count: “+9”

      • Convention:

        • 3 neutrino masses

        • 3 PMNS angles

        • 1 Dirac phase

        • 2 Majorana phases

      • Note: heavy seesaw scales are additional branch parameters

    • Cosmological dark sector:

      • Count: branch-dependent

      • Convention: depends on Λ\Lambda branch, evolving dark-energy branch, dark matter microphysics, and low-boundary parameterization

    • Record objectivity calibration:

      • Count: model-dependent

      • Convention: depends on objectivity function F_Z, persistence thresholds, and readout model

Exact counts depend on branch choices and normalization conventions. Chapter 11 treats that dependence as controlled parameter structure.


11.20 Higgs and Naturalness Diagnostics

SymbolRoleDimensionStatusOpen ProblemDefined In
vvelectroweak scalemassderivation openR5R5Chapters 9, 11, 17
μH\mu_HHiggs potential mass parametermassderivation openR5R5Chapters 9, 11, 17
λH\lambda_HHiggs quarticdimensionlessdimensionless residueR5R5Chapters 9, 11, 17
mHm_HHiggs massmassderivation openR5R5Chapters 9, 11, 17
v/MPv/M_Pelectroweak/Planck hierarchy ratiodimensionlessdimensionless residueR5R5Chapters 11, 16, 17

Explaining or reclassifying the electroweak scale and the stability of the Higgs mass within the source-to-readout architecture remains part of the R5 programme of Chapter 17.


11.21 Calibration versus Derivation

A parameter is derived only when it is obtained from source data without using that parameter, or an observable equivalent to it, as an input. A parameter fixed by comparison with measurement is calibrated, however precise the resulting value. Both are legitimate scientific situations, but conflating them would misstate what the theory has achieved. The staged R5 programme of Chapter 17 records, for every parameter family, which of the four classifications — derived, constrained, calibrated, unresolved — presently applies.