Positive maps and finite-dimensional approximation Prerequisite proofs · Sources and terms

Finite measured groupoids and AFD algebras

Written by GPT-6.1 Sol (OpenAI), Ultra, September 2026. Self-checked by the writing AI. New original text: public domain (CC0).

Finite equivalence classes give matrix algebras with a measurable center. They need not give finite-dimensional algebras. To obtain finite-dimensional approximation, one must also discretize that center. We carry out both steps and prove that an ergodic principal measured AF groupoid of type II1\mathrm{II}_1 has an AFD factor of type II1\mathrm{II}_1.

We use standard Borel spaces, countable separating families, measure completion, monotone convergence and Hilbert-space operator theory. The injective-image input is the exact Lusin–Souslin Theorem 3.6 and Polish topology refinement F4 from Polish spaces and standard Borel spaces, already used in the fullness lesson. We explain its needed Borel-map version below. The finite-trace local AFD criterion and separable uniqueness theorem are proved in Hyperfinite finite factors. General modular weights or expectations are not needed for the kernel construction.

The freely readable equivalence-relation construction is Anantharaman–Popa, §1.5. We use the type II1\mathrm{II}_1 hypothesis to choose an equivalent invariant probability measure; we do not infer invariance from quasi-invariance alone. The AF exhaustion and its fixed finite class sizes are given hypotheses.

1. The measured equivalence relation

Principality identifies the groupoid with a Borel equivalence relation R⊂X×X\mathcal R\subset X\times X, with countable classes, on a standard Borel space XX. The arrow (x,y)(x,y) runs from yy to xx; multiplication is

(x,y)(y,z)=(x,z).(1)(x,y)(y,z)=(x,z). \tag{1}

Its source counting measure relative to a probability measure μ\mu is

ν(E)=∫X#{x:(x,y)∈E} dμ(y).(2)\nu(E)=\int_X\#\{x:(x,y)\in E\}\,d\mu(y). \tag{2}

The measured-relation setup includes measurability of source counting functions for Borel arrow sets and of countable-relation saturations. These are countable-section inputs; the finite-class labels below do not by themselves prove them for an arbitrary countable relation. Complete proofs of these Borel inputs are not established in these lessons.

Invariance means that ν\nu is unchanged by the flip (x,y)↦(y,x)(x,y)\mapsto(y,x). Equivalently, every Borel partial bijection whose graph lies in R\mathcal R preserves the restricted measure. The forward implication follows by comparing its graph and inverse graph over any Borel subset of its domain. The converse follows by decomposing the relation into countably many such graphs; our finite-class labels below provide that decomposition in the AF case.

The source AF hypothesis supplies increasing Borel subrelations

R1⊂R2⊂⋯ ,ν(R∖⋃nRn)=0,(3)\mathcal R_1\subset\mathcal R_2\subset\cdots,\qquad \nu\left(\mathcal R\setminus\bigcup_n\mathcal R_n\right)=0, \tag{3}

where each Rn\mathcal R_n has a fixed finite class size knk_n almost everywhere. This is the source's type Ikn\mathrm I_{k_n} condition. Statements and functions are taken modulo null sets.

There is no difficulty in discarding common exceptional classes. If N⊂XN\subset X is null, invariance gives

ν{(x,y):x∈N}=ν{(x,y):y∈N}=0.\nu\{(x,y):x\in N\} =\nu\{(x,y):y\in N\}=0.

The first set has a nonempty source fiber exactly on the saturation of NN, so that saturation is null as well. Thus countably many null exceptions can be removed without retaining arrows into them.

We can also make the AF model exact on a conull invariant set. Put R∞=⋃nRn\mathcal R_\infty=\bigcup_n\mathcal R_n and let N0N_0 be the measurable set of sources with at least one arrow in R∖R∞\mathcal R\setminus\mathcal R_\infty. Equation (3) makes N0N_0 null. It is saturated: if y∈N0y\in N_0 and z∼yz\sim y had no missing arrows, every point of their common orbit would be R∞\mathcal R_\infty-equivalent to zz; transitivity would contradict the missing arrow at yy. Remove N0N_0 and the null saturations of the countably many finite-stage class-size exceptions. On the resulting conull invariant model, R=R∞\mathcal R=\mathcal R_\infty literally and every stage has its stated finite class size. Its labeled stage graphs then describe every arrow.

If the initially given measure is merely equivalent to an invariant probability μ\mu, the associated regular algebras are normally isomorphic. Indeed if dμ′/dμ=h>0d\mu'/d\mu=h>0, the source counting measures satisfy dν′/dν(x,y)=h(y)d\nu'/d\nu(x,y)=h(y), and

V:L2(R,ν)⟶L2(R,ν′),(Vξ)(x,y)=h(y)−1/2ξ(x,y)(4)V:L^2(\mathcal R,\nu)\longrightarrow L^2(\mathcal R,\nu'), \qquad (V\xi)(x,y)=h(y)^{-1/2}\xi(x,y) \tag{4}

is unitary. Left convolution does not change the source coordinate yy, so it intertwines under VV. We may therefore work with the invariant probability furnished by the type II1\mathrm{II}_1 assumption.

2. Borel labels for finite classes

We need actual measurable matrix coordinates, not just a choice of labels on each finite class.

First recall the Borel-map form of the injective-image theorem. If f:Y→Zf:Y\to Z is an injective Borel map between standard Borel spaces, refine compatible Polish topologies on YY so that the inverse images of a countable base on ZZ become open and closed. F4 permits each refinement and their countable join, without changing the Borel sets. Then ff is continuous. Lusin–Souslin makes its image, and the image of every Borel subset, Borel. Thus ff is a Borel isomorphism onto its image. This uses the declared topology-refinement input; injectivity alone does not make arbitrary projections preserve Borel sets.

Lemma 2.1. A Borel equivalence relation with all classes of size k<∞k<\infty has a Borel partition

X=A1⊔⋯⊔AkX=A_1\sqcup\cdots\sqcup A_k

such that each AiA_i meets every class once. With Y=A1Y=A_1, there are Borel isomorphisms ϕi:Y→Ai\phi_i:Y\to A_i, with ϕ1=id⁡Y\phi_1=\operatorname{id}_Y, which list each class.

Proof. A countable separating family embeds XX injectively and Borel measurably into the Cantor space by its membership bits. The preceding injective-image fact supplies a Borel order on XX, obtained from the lexicographic order of those bit sequences. Every finite class has a unique increasing listing.

Let T⊂XkT\subset X^k consist of the increasing kk-tuples all of whose entries are equivalent. It is Borel. Each coordinate projection pi:T→Xp_i:T\to X is injective: an entry determines its entire finite class, and hence its unique increasing tuple. The images Ai=pi(T)A_i=p_i(T) are Borel and partition XX. The maps ϕi=pi(p1∣T)−1\phi_i=p_i(p_1|_T)^{-1} are Borel bijections and list the class as claimed. □\square

For an invariant measure, the maps ϕi\phi_i preserve its restriction on YY, so

μ(Ai)=μ(Y)=1/k,β=k μ∣Y(5)\mu(A_i)=\mu(Y)=1/k,\qquad \beta=k\,\mu|_Y \tag{5}

is a probability measure. More precisely μ(ϕi(E))=μ(E)\mu(\phi_i(E))=\mu(E) for every Borel E⊂YE\subset Y.

Apply this lemma to every Rn\mathcal R_n. Its finitely many pair-coordinate graphs, as nn varies, cover R\mathcal R modulo the null set in (3). In particular all counting functions, kernel sums and null-set saturations used here can be evaluated through countably many Borel graphs.

3. The regular algebra and its trace

Put H=L2(R,ν)H=L^2(\mathcal R,\nu). Let Cn\mathcal C_n be the bounded measurable kernels supported on Rn\mathcal R_n, extended by zero outside it. The union C=⋃nCn\mathcal C=\bigcup_n\mathcal C_n is a unital convolution *-algebra:

(f∗g)(x,y)=∑z∼xf(x,z)g(z,y),f∗(x,y)=f(y,x)‾.(6)(f*g)(x,y)=\sum_{z\sim x}f(x,z)g(z,y),\qquad f^*(x,y)=\overline{f(y,x)}. \tag{6}

For f,gf,g from two stages, all nonzero terms lie in the larger subrelation, whose finite class size bounds the sums. The diagonal kernel 1Δ1_\Delta is the convolution identity.

Define left and right convolution by

(Lfξ)(x,y)=∑zf(x,z)ξ(z,y),(Qfξ)(x,y)=∑zξ(x,z)f(z,y).(7)(L_f\xi)(x,y)=\sum_z f(x,z)\xi(z,y),\qquad (Q_f\xi)(x,y)=\sum_z \xi(x,z)f(z,y). \tag{7}

These are bounded operators. For left convolution, if both absolute row and column sums of ff are bounded by CC, weighted Cauchy–Schwarz gives on each orbit

∑x∣∑zf(x,z)η(z)∣2≤C∑x,z∣f(x,z)∣ ∣η(z)∣2≤C2∑z∣η(z)∣2.(8)\sum_x\left|\sum_z f(x,z)\eta(z)\right|^2 \le C\sum_{x,z}|f(x,z)|\,|\eta(z)|^2 \le C^2\sum_z|\eta(z)|^2. \tag{8}

Integrating over the source coordinate proves ∥Lf∥≤C\|L_f\|\le C. For f∈Cnf\in\mathcal C_n we may take C=kn∥f∥∞C=k_n\|f\|_\infty. Flip invariance makes

(Jξ)(x,y)=ξ(y,x)‾(J\xi)(x,y)=\overline{\xi(y,x)}

antiunitary, and Qf=JLf∗JQ_f=J L_{f^*}J, proving the right bound as well. Finite-sum multiplication gives

Lf∗=Lf∗,Qf∗=Qf∗,LfQg=QgLf.(9)L_f^*=L_{f^*},\qquad Q_f^*=Q_{f^*},\qquad L_f Q_g=Q_g L_f. \tag{9}

Define the regular von Neumann algebra

M={Lf:f∈C}′′.(10)M=\{L_f:f\in\mathcal C\}''. \tag{10}

This is the associated groupoid algebra in the usual bounded-Schur-kernel definition, not a smaller algebra caused by (3). In fact let ff have bounded absolute row and column sums. Then ∣f∣≤C|f|\le C and f∈L2(ν)f\in L^2(\nu), since ∫∑x∣f(x,y)∣2 dμ(y)≤C2\int\sum_x|f(x,y)|^2\,d\mu(y)\le C^2. The same bound (8) defines its left operator. It commutes with each QgQ_g, g∈Cg\in\mathcal C: first check on kernel vectors ξ∈C\xi\in\mathcal C. Both composite sums are finite because gg and ξ\xi lie in finite-class stages. Interchanging their intermediate indices gives equality, which extends by density and boundedness. Its cutoffs fn=f1Rnf_n=f1_{\mathcal R_n} belong to Cn\mathcal C_n, converge to ff in L2(ν)L^2(\nu), and have the same uniform operator bound. The commuting right algebra used below has a dense orbit on the diagonal vector. Convergence on that vector therefore extends to strong convergence on all of HH, giving Lf∈ML_f\in M. The reverse inclusion is immediate because every finite-stage kernel is a Schur kernel. This also matches the source's left regular convolution construction.

Lemma 3.1. The diagonal vector Ω=1Δ\Omega=1_\Delta is cyclic and separating for MM, and

τ(x)=⟨Ω,xΩ⟩(11)\tau(x)=\langle\Omega,x\Omega\rangle \tag{11}

is a faithful normal tracial state. For f∈Cf\in\mathcal C,

τ(Lf)=∫Xf(x,x) dμ(x),∥Lf∥2,τ2=∫R∣f∣2 dν.(12)\tau(L_f)=\int_X f(x,x)\,d\mu(x),\qquad \|L_f\|_{2,\tau}^2=\int_{\mathcal R}|f|^2\,d\nu. \tag{12}

Proof. We have LfΩ=QfΩ=fL_f\Omega=Q_f\Omega=f. The bounded functions on Rn\mathcal R_n are dense in L2(Rn,ν)L^2(\mathcal R_n,\nu), and (3) makes their union dense in HH. Here ν(Rn)=kn<∞\nu(\mathcal R_n)=k_n<\infty. Thus both convolution algebras have a dense orbit on Ω\Omega. The right algebra commutes with MM, so xΩ=0x\Omega=0, x∈Mx\in M, forces xQfΩ=0xQ_f\Omega=0 on a dense set and hence x=0x=0. This proves separation and faithfulness; ∥Ω∥=1\|\Omega\|=1 and vector functionals are normal.

The first identity in (12) follows from LfΩ=fL_f\Omega=f. Invariance under the flip gives

∫X∑zf(x,z)g(z,x) dμ(x)=∫X∑zg(x,z)f(z,x) dμ(x).\int_X\sum_z f(x,z)g(z,x)\,d\mu(x) =\int_X\sum_z g(x,z)f(z,x)\,d\mu(x).

These are τ(LfLg)\tau(L_fL_g) and τ(LgLf)\tau(L_gL_f). Thus τ\tau is tracial on the unital generating -algebra. Bounded strong Kaplansky approximation extends this identity first in one variable and then in the other to MM. Finally ∥Lf∥2,τ=∥LfΩ∥=∥f∥L2(ν)\|L_f\|_{2,\tau}=\|L_f\Omega\|=\|f\|_{L^2(\nu)}. □\square

The dense right orbit just proved also justifies the strong-cutoff assertion preceding the lemma: for g∈Cg\in\mathcal C,

∥(Lfn−Lf)QgΩ∥≤∥Qg∥ ∥fn−f∥L2(ν).\|(L_{f_n}-L_f)Q_g\Omega\| \le\|Q_g\|\,\|f_n-f\|_{L^2(\nu)}.

Uniform boundedness and density complete that assertion.

Bounded 2-norm convergence here implies sigma-strong* convergence, also when MM is not a factor. Suppose za∈Mz_a\in M, ∥za∥≤C\|z_a\|\le C, and ∥za∥2,τ→0\|z_a\|_{2,\tau}\to0. Commutation with the right algebra gives

∥zaQgΩ∥≤∥Qg∥ ∥zaΩ∥=∥Qg∥ ∥za∥2,τ⟶0.\|z_aQ_g\Omega\|\le\|Q_g\|\,\|z_a\Omega\| =\|Q_g\|\,\|z_a\|_{2,\tau}\longrightarrow0.

The right orbit is dense, so the common bound extends convergence to every vector. Traciality gives ∥za∗∥2,τ=∥za∥2,τ\|z_a^*\|_{2,\tau}=\|z_a\|_{2,\tau}, and the same argument applies to the adjoints. Thus za→0z_a\to0 strongly*. Both za∗zaz_a^*z_a and zaza∗z_az_a^* are bounded and weakly null. Finite-rank approximation of a trace-class functional, with their common bound controlling its trace-norm tail, makes both products ultraweakly null. The concrete predual of MM is a quotient of the trace-class predual of B(H)B(H), so every normal positive functional on MM tends to zero on these products. These are precisely the sigma-strong* tests. The concrete-predual foundation remains explicit; this argument makes no factoriality assumption.

4. Finite stages are matrix fields

Fix a stage, and write k=knk=k_n, Y=A1Y=A_1 and ϕi\phi_i for its labels. Set vij=L1Gr⁡(ϕiϕj−1)v_{ij}=L_{1_{\operatorname{Gr}(\phi_i\phi_j^{-1})}}. Direct convolution gives

vijvℓm=δjℓvim,vij∗=vji,∑ivii=1.(13)v_{ij}v_{\ell m}=\delta_{j\ell}v_{im},\qquad v_{ij}^*=v_{ji},\qquad \sum_i v_{ii}=1. \tag{13}

For d∈L∞(X,μ)d\in L^\infty(X,\mu), its diagonal kernel gives the multiplication operator Ddξ(x,y)=d(x)ξ(x,y)D_d\xi(x,y)=d(x)\xi(x,y). This diagonal representation is normal and faithful.

Every kernel in Cn\mathcal C_n is determined by

Fij(t)=f(ϕi(t),ϕj(t)),t∈Y.(14)F_{ij}(t)=f(\phi_i(t),\phi_j(t)),\qquad t\in Y. \tag{14}

Convolution is matrix multiplication of these fields, and involution is matrix adjoint. Its operator is ∑i,jvi1DFij1Yv1j\sum_{i,j}v_{i1}D_{F_{ij}1_Y}v_{1j}. Consequently the stage algebra is

Mn={Lf:f∈Cn}≅Mk(L∞(Y,β)).(15)M_n=\{L_f:f\in\mathcal C_n\} \cong M_k\bigl(L^\infty(Y,\beta)\bigr). \tag{15}

This image is already a von Neumann algebra. To verify closedness, an operator TT belongs to it exactly when all v1iTvj1v_{1i}Tv_{j1} lie in the weakly closed diagonal corner DL∞(Y)D_{L^\infty(Y)}. The reverse implication follows by reconstructing TT with the finite matrix-unit sum (13). Each corner condition is ultraweakly closed. The entry maps and their inverse corner extraction are normal; faithfulness also follows from LfΩ=fL_f\Omega=f.

The trace is

τ(F)=1k∫YTr⁡k(F(t)) dβ(t),∥F∥2,τ2=1k∫Y∑i,j∣Fij(t)∣2 dβ(t).(16)\tau(F)=\frac1k\int_Y\operatorname{Tr}_k(F(t))\,d\beta(t),\qquad \|F\|_{2,\tau}^2=\frac1k\int_Y\sum_{i,j}|F_{ij}(t)|^2\,d\beta(t). \tag{16}

Indeed each ϕi\phi_i preserves μ∣Y\mu|_Y, and (5) gives the normalization. The algebras MnM_n are increasing and generate MM.

Lemma 4.1. For a finite set of elements of MnM_n and ε>0\varepsilon>0, one unital finite-dimensional subalgebra of MnM_n approximates every element within ε\varepsilon in ∥⋅∥2,τ\|\cdot\|_{2,\tau}.

Proof. The finite collection of bounded entries in (14) can be approximated simultaneously by one finite measurable partition P\mathcal P of YY: discretize their real and imaginary ranges and take the common refinement. Average each matrix field over each positive-measure cell of P\mathcal P, entry by entry. The resulting field EPFE_{\mathcal P}F lies in

BP=Mk⊗span⁡{1C:C∈P},(17)B_{\mathcal P} =M_k\otimes\operatorname{span}\{1_C:C\in\mathcal P\}, \tag{17}

a unital finite-dimensional algebra.

If each real and imaginary entry varies by at most δ\delta on a cell, its difference from its cell average has magnitude at most 2δ\sqrt2\delta. Formula (16) gives

∥F−EPF∥2,τ2≤2kδ2.(18)\|F-E_{\mathcal P}F\|_{2,\tau}^2\le2k\delta^2. \tag{18}

Choose δ\delta for the prescribed ε\varepsilon. Zero-measure cells are irrelevant. Matrix averaging is also contractive in operator norm, because the norm of an average is at most the average of the norms. No abstract conditional expectation theorem is needed for this finite-partition operation. □\square

Theorem 4.2. The regular algebra MM is finite and AFD. This conclusion does not require ergodicity.

Proof. Finiteness is supplied by the faithful normal trace. The increasing union of MnM_n is a unital *-algebra generating MM, so Kaplansky density approximates any finite family x1,…,xr∈Mx_1,\ldots,x_r\in M strongly*, by elements yjy_j in one common stage with ∥yj∥≤∥xj∥\|y_j\|\le\|x_j\|. In particular ∥xj−yj∥2,τ\|x_j-y_j\|_{2,\tau} can be made arbitrarily small. Lemma 4.1 then approximates the yjy_j by bj=EPyjb_j=E_{\mathcal P}y_j in one finite-dimensional algebra, with ∥bj∥≤∥yj∥\|b_j\|\le\|y_j\|. The triangle inequality makes every ∥xj−bj∥2,τ\|x_j-b_j\|_{2,\tau} arbitrarily small while ∥xj−bj∥≤2∥xj∥\|x_j-b_j\|\le2\|x_j\|. The bounded 2-norm argument in Section 3 therefore gives approximation in every prescribed sigma-strong* neighborhood. This proves AFD for the finite algebra, including its nonfactor cases. □\square

5. Ergodicity and type

Lemma 5.1. The center of MM consists exactly of the diagonal functions invariant under R\mathcal R.

Proof. Let z∈Z(M)z\in Z(M) and put η=zΩ\eta=z\Omega. For each bounded diagonal function dd, its left and right multiplications agree on Ω\Omega. Centrality of zz and commutation with the right algebra give

Ddη=Qdη,(d(x)−d(y))η(x,y)=0.(19)D_d\eta=Q_d\eta,\qquad (d(x)-d(y))\eta(x,y)=0. \tag{19}

A countable separating family on XX forces η\eta to vanish off the diagonal. Write η=h1Δ\eta=h1_\Delta, h∈L2(X,μ)h\in L^2(X,\mu). For every measurable E⊂XE\subset X,

∫E∣h∣2 dμ=∥zD1EΩ∥2≤∥z∥2μ(E).\int_E|h|^2\,d\mu =\|zD_{1_E}\Omega\|^2\le\|z\|^2\mu(E).

Hence h∈L∞(X,μ)h\in L^\infty(X,\mu), with ∥h∥∞≤∥z∥\|h\|_\infty\le\|z\|. The separating vector gives z=Dhz=D_h.

Commutation with every matrix unit vijv_{ij} at every stage says h(ϕi(t))=h(ϕj(t))h(\phi_i(t))=h(\phi_j(t)) almost everywhere. By (3) this is precisely h(x)=h(y)h(x)=h(y) for ν\nu-almost every arrow. Conversely that equality makes DhD_h commute with every convolution generator.

The countably many stage graphs preserve null sets. Thus an almost invariant level set of hh has an exactly saturated representative modulo a null set: take its saturation under those graphs; every newly added piece comes from a null violation of invariance. This justifies using the usual measured ergodicity definition. □\square

Theorem 5.2. An ergodic principal orbitally countable measured AF groupoid of type II1\mathrm{II}_1 has an AFD factor of type II1\mathrm{II}_1. Its predual is separable, and it is isomorphic to the tracial infinite tensor product of M2M_2.

Proof. Ergodicity makes every invariant bounded function constant, so Lemma 5.1 makes MM a factor. Its trace is finite and faithful.

The invariant probability μ\mu has no atoms. On a standard Borel space every probability atom contains a point of positive mass: use a countable separating family, take on each set the side carrying the atom's full measure, and intersect those sides. Their intersection has the atom's measure and contains at most one point. If such a point xx had mass c>0c>0, invariance applied to singleton arrows would give mass cc to every point in its orbit. That orbit would be finite. Its positive-measure saturation would be conull by ergodicity, putting the relation in type I, contrary to its specified type II1\mathrm{II}_1. Thus L∞(X,μ)⊂ML^\infty(X,\mu)\subset M is diffuse and infinite dimensional. A finite factor containing it cannot be a finite matrix algebra; it is of type II1\mathrm{II}_1.

AFD follows from Theorem 4.2. Each Rn\mathcal R_n is a standard Borel space with finite counting measure. Its L2L^2 space is separable, using simple functions from a countable Borel generator. Their increasing dense union makes HH separable. The concrete predual of MM is a quotient of the separable trace-class predual of B(H)B(H), so it is separable. The local finite AFD uniqueness theorem now identifies MM with the tracial M2M_2 product. □\square

This proof uses the given AF exhaustion. It does not need the theorem converting amenability of measured relations to approximate finiteness.

6. Exercises with complete solutions

Exercise 1. Why does a relation with classes of size two on X=Y×{1,2}X=Y\times\{1,2\}, with a nonatomic probability space YY, fail to have a finite-dimensional regular algebra?

Solution. Relate (t,1)(t,1) only to (t,2)(t,2), and give the two coordinates equal weight. Formula (15) gives M2(L∞(Y))M_2(L^\infty(Y)). Its center contains all scalar fields a(t)12a(t)1_2, an infinite-dimensional algebra because YY is nonatomic. Class finiteness controls matrix size, not the dimension of the coefficient algebra. Finite partitions of YY give the finite-dimensional approximants in (17).

Exercise 2. Verify the measure normalization in (16) for a single matrix-unit field.

Solution. For F=1EeijF=1_E e_{ij}, E⊂YE\subset Y, its L2L^2 norm squared is μ(E)\mu(E), since the kernel has one nonzero arrow per source point in ϕj(E)\phi_j(E), and μ(ϕj(E))=μ(E)\mu(\phi_j(E))=\mu(E). Formula (16) gives β(E)/k=μ(E)\beta(E)/k=\mu(E). Its trace is zero if i≠ji\ne j, and μ(E)\mu(E) if i=ji=j. In particular the identity has trace kμ(Y)=1k\mu(Y)=1, whereas a constant diagonal matrix unit has trace 1/k1/k.

Exercise 3. On a finite class of size three, check the orientation of convolution using the arrows (x1,x2)(x_1,x_2) and (x2,x3)(x_2,x_3).

Solution. Their graph kernels are matrix units e12e_{12} and e23e_{23}. In (6) the only surviving intermediate point is x2x_2, giving e12∗e23=e13e_{12}*e_{23}=e_{13}, the arrow (x1,x3)(x_1,x_3). Reversing their order gives zero. The involution reverses an arrow and complex conjugates its coefficient, so e12∗=e21e_{12}^*=e_{21}.

Exercise 4. Prove the strong convergence claim for Schur-kernel cutoffs without claiming operator-norm convergence.

Solution. Let fn=f1Rnf_n=f1_{\mathcal R_n}. Formula (3) and dominated convergence give ∥fn−f∥L2(ν)→0\|f_n-f\|_{L^2(\nu)}\to0; the Schur bounds give a common operator bound. For g∈Cg\in\mathcal C, commutation gives

(Lfn−Lf)QgΩ=Qg(fn−f),(L_{f_n}-L_f)Q_g\Omega=Q_g(f_n-f),

whose norm tends to zero. The vectors QgΩQ_g\Omega span a dense subspace. Approximate an arbitrary vector by this subspace and use the common bound to control the error. This proves strong convergence. It supplies no estimate forcing ∥Lfn−Lf∥→0\|L_{f_n}-L_f\|\to0.

Exercise 5. Show that the finite-partition matrix average in Lemma 4.1 preserves positivity and the identity.

Solution. If F(t)≥0F(t)\ge0 almost everywhere, then for every vector ζ∈Ck\zeta\in\mathbb C^k its cell average satisfies

⟨ζ,1β(C)∫CF(t) dβ(t) ζ⟩=1β(C)∫C⟨ζ,F(t)ζ⟩ dβ(t)≥0.\left\langle\zeta,\frac1{\beta(C)}\int_C F(t)\,d\beta(t)\,\zeta\right\rangle =\frac1{\beta(C)}\int_C\langle\zeta,F(t)\zeta\rangle\,d\beta(t)\ge0.

The same computation applies to matrices of such fields, giving complete positivity. The constant identity averages to the identity. This elementary finite integral explains the norm bound, without importing general von Neumann expectation theory.

Exercise 6. Why is a bounded invariant diagonal function central even before ergodicity is assumed?

Solution. For h(x)=h(z)h(x)=h(z) on almost every arrow, the products DhLfD_hL_f and LfDhL_fD_h have kernels h(x)f(x,z)h(x)f(x,z) and f(x,z)h(z)f(x,z)h(z). They agree for every generating kernel ff. Hence DhD_h commutes with their von Neumann algebra. Ergodicity is used only to make these central functions scalar.

Exercise 7. Identify exactly what fails if one tries to deduce a factor from a finite-class exhaustion without ergodicity.

Solution. The construction still gives a faithful finite trace and the finite-dimensional approximation proof still works. However a nontrivial invariant subset E⊂XE\subset X gives a central projection D1ED_{1_E}, by Lemma 5.1. Its trace is μ(E)∈(0,1)\mu(E)\in(0,1), so it is neither zero nor one. Thus the algebra is not a factor. The example in Exercise 1 has precisely this obstruction.

Exercise 8. If a probability measure assigns an atom of mass c>0c>0 to one point in an invariant measured relation, show that its orbit has at most 1/c1/c points.

Solution. For each equivalent point yy, the singleton partial bijection x↦yx\mapsto y preserves measure, so μ({y})=c\mu(\{y\})=c. Distinct orbit points are disjoint atoms. Any NN of them have total measure Nc≤1Nc\le1, so N≤1/cN\le1/c. The orbit is therefore finite. Ergodicity then concentrates the measure on that orbit, the type I case excluded in Theorem 5.2.

Exercise 9. Explain why changing to an equivalent invariant measure in (4) does not require multiplying left-convolution kernels by a density ratio.

Solution. Source-coordinate densities multiply a vector by h(y)−1/2h(y)^{-1/2}. Left convolution sums over the first coordinate while keeping yy fixed:

∑zf(x,z)h(y)−1/2ξ(z,y)=h(y)−1/2(Lfξ)(x,y).\sum_z f(x,z)h(y)^{-1/2}\xi(z,y) =h(y)^{-1/2}(L_f\xi)(x,y).

Thus VLf=LfVVL_f=L_fV between the two L2L^2 spaces. A right-convolution formula changes the source coordinate and would behave differently for a noninvariant measure. Only the invariant-probability model is used for the simple right formula (7).

Exercise 10. The algebras BPB_{\mathcal P} chosen for different finite tests need not form an increasing sequence. Why is this enough here, and how does one obtain the increasing matrix sequence for the final factor?

Solution. The definition of local AFD asks for one finite-dimensional algebra for each finite set and neighborhood; it does not demand that choices for different tests be nested. Theorem 4.2 proves exactly that property. In the separable II1\mathrm{II}_1 factor, the earlier finite AFD lesson's dyadic replacement and exact containment arguments convert successive local approximations into an increasing sequence of matrix subfactors. Its uniqueness proof then identifies the closure with the tracial M2M_2 product. A claim of nesting directly from unrelated partitions at unrelated relation stages would need a separate argument.

7. Elementary completion of finite-partition averaging

This section supplies the scalar integration, measurable partition, and matrix averaging details in Lemma 4.1 and Exercise 5. Its starting point is the unital matrix-field identification (15), with the usual field norm and order, and the normalized trace formula (16). In particular, β(Y)=1\beta(Y)=1,

A=Mk(L∞(Y,β)),∥F∥=ess sup⁡t∈Y∥F(t)∥op,∥F∥2,τ2=1k∫Y∑i,j=1k∣Fij(t)∣2 dβ(t).\mathcal A=M_k(L^\infty(Y,\beta)),\qquad \|F\|=\operatorname*{ess\,sup}_{t\in Y}\|F(t)\|_{\mathrm{op}},\qquad \|F\|_{2,\tau}^2=\frac1k\int_Y\sum_{i,j=1}^k|F_{ij}(t)|^2\,d\beta(t).

The argument applies to any probability measure space, including one with atoms and one whose sigma-algebra is completed. The Borel labeling, the faithful normal operator model, and the trace construction that establish (15)-(16) keep their separate prerequisite status.

Bounded scalar integration

For a complex simple function on a finite disjoint measurable partition, define

s=∑j=1mzj1Dj,I(s)=∑j=1mzjβ(Dj).s=\sum_{j=1}^m z_j1_{D_j},\qquad I(s)=\sum_{j=1}^m z_j\beta(D_j).

Two representations have a common refinement formed from the intersections of their cells. Finite additivity on that refinement shows that I(s)I(s) is independent of the representation and complex linear. The finite sums also give positivity for real nonnegative simple functions and

∣I(s)∣≤I(∣s∣)≤β(Y)∥s∥∞.|I(s)|\leq I(|s|)\leq\beta(Y)\|s\|_\infty.

Every bounded measurable complex function hh is a uniform limit of simple functions: divide its bounded real and imaginary ranges into finitely many half-open intervals, use their measurable inverse images, and let the interval widths tend to zero. If sn→hs_n\to h uniformly, the preceding bound makes I(sn)I(s_n) Cauchy. Define I(h)=lim⁡nI(sn)I(h)=\lim_n I(s_n). For another uniform simple approximation un→hu_n\to h, the same bound on sn−uns_n-u_n shows that the two limits agree. Approximating sums proves linearity. A nonnegative real function has nonnegative simple approximants, so positivity passes to the limit and real order bounds pass to integrals. Since ∣sn∣→∣h∣|s_n|\to|h| uniformly,

∣I(h)∣≤I(∣h∣)≤β(Y)∥h∥∞.|I(h)|\leq I(|h|)\leq\beta(Y)\|h\|_\infty.

The construction on a measurable subset CC gives ICI_C, with the bound ∣IC(h)∣≤β(C)∥h∥∞|I_C(h)|\leq\beta(C)\|h\|_\infty. A bounded function supported on a null set therefore has integral zero, and the integral depends only on the almost-everywhere class.

These integrals agree with the usual Lebesgue integrals of bounded functions. For a nonnegative bounded hh, choose grid approximants with sn≤h≤sn+ηns_n\leq h\leq s_n+\eta_n, where ηn↓0\eta_n\downarrow0. If uu is any nonnegative simple function below hh, then u≤sn+ηnu\leq s_n+\eta_n. Thus the supremum of the simple integrals below hh lies between I(sn)I(s_n) and I(sn)+β(Y)ηnI(s_n)+\beta(Y)\eta_n. These bounds have the same limit. Positive and negative parts extend the agreement to real functions; real and imaginary parts extend it to complex functions. All integrals used below can consequently be obtained from finite sums and uniform limits.

One common partition and a strict error bound

Let F(1),…,F(r)∈AF^{(1)},\ldots,F^{(r)}\in\mathcal A and ε>0\varepsilon>0. Choose measurable representatives for their finitely many entries. A single measurable null set contains every violation of chosen finite essential bounds on those entries. Redefine all entries as zero on that set. They are now bounded everywhere and represent the original fields. If the family is empty, use P={Y}\mathcal P=\{Y\}.

For a nonempty family set

δ=ε22k.\delta=\frac{\varepsilon}{2\sqrt{2k}}.

For each real and imaginary entry hh, take the inverse images of

[mδ,(m+1)δ),m∈Z.[m\delta,(m+1)\delta),\qquad m\in\mathbb Z.

Only finitely many bins meet the bounded range. The half-open convention assigns every value to one bin, including a value on a boundary. Take all intersections of the 2rk22rk^2 resulting partitions and discard empty intersections. This gives one finite measurable partition P\mathcal P of YY, on whose cells every real and imaginary entry has oscillation at most δ\delta.

On a cell with β(C)>0\beta(C)>0, define the matrix average entry by entry:

F‾C=1β(C)∫CF(t) dβ(t),EPF=∑β(C)>01CF‾C.\overline F_C=\frac1{\beta(C)}\int_C F(t)\,d\beta(t),\qquad E_{\mathcal P}F=\sum_{\beta(C)>0}1_C\overline F_C.

Boundedness and finite measure justify every scalar integral. Almost-everywhere equal representatives give the same averages. The formula makes no division on a null cell; assigning zero there gives the same L∞L^\infty field as any other assignment.

The average of a real coordinate whose values lie in [mδ,(m+1)δ)[m\delta,(m+1)\delta) lies in the closed interval [mδ,(m+1)δ][m\delta,(m+1)\delta], by positivity and real order bounds for the integral. Each real and imaginary difference from its average therefore has absolute value at most δ\delta, and each complex entry difference has squared magnitude at most 2δ22\delta^2. Formula (16) gives, for each original field,

∥F(a)−EPF(a)∥2,τ2≤1k∑β(C)>0∫Ck2(2δ2) dβ=2kδ2=ε24.\begin{aligned} \|F^{(a)}-E_{\mathcal P}F^{(a)}\|_{2,\tau}^2 &\leq\frac1k\sum_{\beta(C)>0}\int_C k^2(2\delta^2)\,d\beta\\ &=2k\delta^2=\frac{\varepsilon^2}{4}. \end{aligned}

Hence every error is at most ε/2<ε\varepsilon/2<\varepsilon. This proves the constant in (18) and the strict tolerance in Lemma 4.1.

Positive cells and representatives before completion

If there are ss positive-measure cells, their indicators are nonzero orthogonal central projections summing to 11 in L∞(Y,β)L^\infty(Y,\beta). Null cells are zero projections. The map

⨁j=1sMk(C)⟶BP,(A1,…,As)⟼∑j=1s1CjAj\bigoplus_{j=1}^s M_k(\mathbb C)\longrightarrow B_{\mathcal P}, \qquad (A_1,\ldots,A_s)\longmapsto\sum_{j=1}^s1_{C_j}A_j

is a unital ∗*-homomorphism onto the algebra in (17). It is injective because a nonzero constant matrix cannot vanish almost everywhere on a positive-measure cell. Thus BPB_{\mathcal P} is unital and has dimension sk2sk^2. There is a positive cell since β(Y)=1\beta(Y)=1. All null cells may be adjoined to one positive cell without changing its projection, its averages, or the estimates almost everywhere.

Suppose the given sigma-algebra is the completion of Σ0\Sigma_0. Each of the finitely many cells has a Σ0\Sigma_0-representative differing from it inside a Σ0\Sigma_0-measurable null set. Successively subtract earlier representatives to make them disjoint, then adjoin their uncovered complement to the first representative. Every change lies inside the finite union of those null sets. The resulting sets form an actual Σ0\Sigma_0-partition and determine the same projections and averages. In the standard Borel setting Σ0\Sigma_0 can be the Borel sigma-algebra. This finite replacement uses the definition of completion and finite set operations.

Contractivity and complete positivity

Let M=∥F∥M=\|F\|, so ∥F(t)∥op≤M\|F(t)\|_{\mathrm{op}}\leq M almost everywhere. For u,v∈Cku,v\in\mathbb C^k, linearity and the scalar integral bound give

∣u∗F‾Cv∣=∣1β(C)∫Cu∗F(t)v dβ(t)∣≤1β(C)∫C∣u∗F(t)v∣ dβ(t)≤M∥u∥∥v∥.\begin{aligned} |u^*\overline F_Cv| &=\left|\frac1{\beta(C)}\int_C u^*F(t)v\,d\beta(t)\right|\\ &\leq\frac1{\beta(C)}\int_C|u^*F(t)v|\,d\beta(t) \leq M\|u\|\|v\|. \end{aligned}

Taking the supremum over unit vectors proves ∥F‾C∥op≤M\|\overline F_C\|_{\mathrm{op}}\leq M and ∥EPF∥≤∥F∥\|E_{\mathcal P}F\|\leq\|F\|. This establishes the operator bound used in Theorem 4.2.

At matrix level qq, a matrix of fields is a field of qkqk-by-qkqk matrices, and the amplified map still averages each entry over the same cells. If that field GG is positive almost everywhere, then for every w∈Cqkw\in\mathbb C^{qk},

w∗G‾Cw=1β(C)∫Cw∗G(t)w dβ(t)≥0.w^*\overline G_Cw =\frac1{\beta(C)}\int_C w^*G(t)w\,d\beta(t)\geq0.

Each cell average is positive. This works for every qq, proving complete positivity and supplying the amplification step in Exercise 5. The same bilinear estimate proves contractivity at every matrix level.

The identity and all cell-constant fields are fixed, proving unitality and idempotence onto BPB_{\mathcal P}. Constant matrices may be brought through finite scalar integrals, so for b,d∈BPb,d\in B_{\mathcal P},

EP(bFd)=b(EPF)d.E_{\mathcal P}(bFd)=b(E_{\mathcal P}F)d.

Summing the cell integrals in (16) proves τ(EPF)=τ(F)\tau(E_{\mathcal P}F)=\tau(F). Moreover, the integral of every entry of F−F‾CF-\overline F_C on its cell is zero. Hence for cell-constant bb,

τ(b∗(F−EPF))=0.\tau\bigl(b^*(F-E_{\mathcal P}F)\bigr)=0.

Expanding the trace square gives

∥F∥2,τ2=∥EPF∥2,τ2+∥F−EPF∥2,τ2,\|F\|_{2,\tau}^2 =\|E_{\mathcal P}F\|_{2,\tau}^2 +\|F-E_{\mathcal P}F\|_{2,\tau}^2,

so this averaging is also contractive in the tracial 22-norm. These conclusions concern the finite-partition map constructed here.

The scalar finite-bin method can be compared with Sheldon Axler, Measure, Integration & Real Analysis, author revision of 12 June 2026, Theorem 2.89, printed p.65 / PDF p.80. The complete proof on that page constructs measurable simple approximants and proves uniform convergence for bounded real functions. The scalar integration and matrix arguments above are independently written. The Borel, operator-model, trace, Kaplansky, concrete-predual, and type foundations retain their separately stated status.

References and proof scope

Claire Anantharaman and Sorin Popa, An introduction to II₁ factors, author draft, §1.5.2, printed pp.19–21 (PDF pp.25–27), uses the same invariant source-counting measure and convolution construction. Its operator and tracial-vector assertions omit some details; Section 3 supplies them here in full. The full Proposition 1.5.5 proof, p.21, gives the actual center/factor comparison. Appendix B.3 and B.5 state the injective-image and countable-section inputs; complete transitive free proofs of those foundations remain pending. Section 12.5, p.209, assumes a nonatomic Lebesgue probability space; Section 5 here derives nonatomicity from its stated measured type hypothesis.

Alain Connes, Jacob Feldman and Benjamin Weiss, An amenable equivalence relation is generated by a single transformation, Ergodic Theory and Dynamical Systems 1(4) (1981), 431–450, §4, pp.436–439, gives invariant-mean and regular Cartan context. Its converse on p.439 is explicitly a sketch. Lemma 8 is in §5, pp.440–442; Lemma 9 and Theorem 10 are in §6, pp.442–444. Theorem 10 obtains a finite-subrelation exhaustion from amenability; this lesson already assumes an AF exhaustion with fixed finite class sizes and does not use that implication. Both comparisons concern principal equivalence-relation groupoids.

The finite labeling, matrix-field approximation and nonfactor topology bridge are complete local arguments relative to the declared Borel, operator and trace-class inputs. Kaplansky density, concrete preduals, type classification and the exact local hyperfinite uniqueness prerequisites remain pending full freely accessible closure. No source expression was imported.