De Finetti theorems for easy quantum groups

Teodor Banica, Stephen Curran, Roland Speicher

Introduction

In the study of probabilistic symmetries, the classicalgroups SnS_{n} and OnO_{n} play central roles. De Finetti’s fundamental theorem states that an infinite sequence of random variables whose joint distribution is invariant under finite permutations must be conditionally independent and identically distributed. In fre1 , Freedman considered sequences of real-valued random variables whose joint distribution is invariant under orthogonal transformations, and proved that any infinite sequence with this property must form a conditionally independent Gaussian family with mean zero and common variance. Although these results fail for finite sequences, approximation results may still be obtained (see df1 , df2 ). For a thorough treatment of probabilistic symmetries, the reader is referred to the recent text of Kallenberg kal .

The free analogues Sn+S_{n}^{+} and On+O_{n}^{+} of the permutation and orthogonal groups were constructed by Wang in wang1 , wang2 . These are compact quantum groups in the sense of Woronowicz wor1 . In ksp , Köstler and Speicher discovered that de Finetti’s theorem has a natural free analogue: an infinite sequence of noncommutative random variables has a joint distribution which is invariant under “quantum permutations” coming from Sn+S_{n}^{+} if and only if the variables are freely independent and identically distributed with amalgamation, that is, with respect to a conditional expectation. This was further studied in cur1 , where this result was extended to more general sequences and an approximation result was given for finite sequences. The free analogue of Freedman’s result was obtained in cur2 , where it was shown that an infinite sequence of self-adjoint noncommutative random variables has a joint distribution which is invariant under “quantum orthogonal transformations” if and only if the variables form an operator-valued free semicircular family with mean zero and common variance.

In this paper, we present a unified approach to de Finetti theorems by using the “easiness” formalism from bsp . Stated roughly, a quantum group Sn⊂G⊂On+S_{n}\subset G\subset O_{n}^{+} is called easy if its tensor category is spanned by certain partitions coming from the tensor category of SnS_{n}. This might look, of course, to be a quite technical condition. However, we feel that this provides a good framework for understanding certain probabilistic and representation theory aspects of orthogonal quantum groups. There are 14 natural examples of easy quantum groups, listed as follows: {longlist}[(3)]

Groups: On,Sn,Hn,Bn,Sn′,Bn′O_{n},S_{n},H_{n},B_{n},S_{n}^{\prime},B_{n}^{\prime}.

Free versions: On+,Sn+,Hn+,Bn+,Sn′+,Bn′+O_{n}^{+},S_{n}^{+},H_{n}^{+},B_{n}^{+},S_{n}^{\prime+},B_{n}^{\prime+}.

As explained in bsp , bcs1 , our motivating belief is that “any result which holds for Sn,OnS_{n},O_{n} should have a suitable extension to all easy quantum groups.” This is, of course, a quite vague statement, whose target is formed by several results at the borderline of representation theory and probability. This paper represents the first application of this philosophy.

If GG is an easy quantum group, there is a natural notion of GG-invariance for a sequence of noncommutative random variables, which agrees with the usual definition when GG is a classical group. Our main result is the following de Finetti type theorem, which characterizes the joint distributions of infinite GG-invariant sequences for the 10 natural easy quantum groups discussed above.

The notion of half-independence, appearing in (2) above, will be introduced in Section 2. The basic example of a half-independent family of noncommutative random variables is (xi)i∈I(x_{i})_{i\in I},

The paper is organized as follows. Section 1 contains preliminaries. Here we collect the basic notions from the combinatorial theory of classical and free probability. We also recall some basic notions and results from bsp about the class of “easy” quantum groups. In Section 2, we introduce half-independence and develop its basic combinatorial theory. In Section 3, we recall the Weingarten formula from bsp for computing integrals on easy quantum groups, and give a new estimate on the asymptotic behavior of these integrals. This will be essential to the proofs of our main results, and we believe that this estimate will also find applications to other problems involving easy quantum groups. In Section 4, we define quantum invariance for finite sequences, prove a converse to Theorem 1, and give approximate de Finetti type results. Section 5 contains the proof of Theorem 1, and a discussion of the situation for unbounded random variables in the classical and half-liberated cases. Section 6 contains concluding remarks.

Background and notation

We begin by recalling the basic notions of noncommutative probability spaces and distributions of random variables. For further details, see the texts vdn , ns .

A W∗-probability space (M,φ)(M,\varphi) is a von Neumann algebra MM together with a faithful normal state φ\varphi. We will not assume that φ\varphi is a trace.

Let (Ω,Σ,μ)(\Omega,\Sigma,\mu) be a (classical) probability space. {longlist}[(2)]

Note that the joint distribution of (xi)i∈I(x_{i})_{i\in I} is determined by the collection of joint moments

In the classical de Finetti’s theorem, the independence which occurs is only after conditioning. Likewise the free de Finetti’s theorem is a statement about freeness with amalgamation. Both of these concepts may be expressed in terms of operator-valued probability spaces, which we now recall.

An operator-valued probability space (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) consists of a unital algebra A\mathcal{A}, a subalgebra 1∈B⊂A1\in\mathcal{B}\subset\mathcal{A}, and a conditional expectation E\dvtxA→BE\dvtx\mathcal{A}\to\mathcal{B}, that is, EE is a linear map such that E=1E=1 and

for all b1,b2∈Bb_{1},b_{2}\in\mathcal{B} and a∈Aa\in\mathcal{A}.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and let (xi)i∈I(x_{i})_{i\in I} be a family in A\mathcal{A}. The BB-valued joint distribution of the family (xi)i∈I(x_{i})_{i\in I} is the linear map Ex\dvtxB⟨ti\dvtxi∈I⟩→BE_{x}\dvtx\mathcal{B}\langle t_{i}\dvtx i\in I\rangle\to\mathcal{B} defined by

Observe that the joint distribution is determined by the B\mathcal{B}-valued joint moments

for b0,…,bk∈Bb_{0},\ldots,b_{k}\in\mathcal{B} and i1,…,ik∈Ii_{1},\ldots,i_{k}\in I. Observe that if B\mathcal{B} commutes with the variables (xi)i∈I(x_{i})_{i\in I}, then

so that the B\mathcal{B}-valued joint distribution is determined simply by the collection of moments E[xi1⋯xik]E[x_{i_{1}}\cdots x_{i_{k}}] for i1,…,ik∈Ii_{1},\ldots,i_{k}\in I.

Let (xi)i∈I(x_{i})_{i\in I} be a family in the operator-valued probability space (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}). {longlist}[(2)]

If the algebra generated by B\mathcal{B} and {xi\dvtxi∈I}\{x_{i}\dvtx i\in I\} is commutative, then the variables are called conditionally independent given BB if

whenever i1,…,iki_{1},\ldots,i_{k} are distinct and p1,…,pkp_{1},\ldots,p_{k} are polynomials in B⟨t⟩\mathcal{B}\langle t\rangle.

The variables (xi)i∈I(x_{i})_{i\in I} are called free with amalgamation over B\mathcal{B}, or free with respect to EE, if

whenever i1,…,ik∈Ii_{1},\ldots,i_{k}\in I are such that il≠il+1i_{l}\neq i_{l+1} for 1≤l<k1\leq l<k, and p1,…,pk∈B⟨t⟩p_{1},\ldots,p_{k}\in\mathcal{B}\langle t\rangle are such that E[pl(xil)]=0E[p_{l}(x_{i_{l}})]=0 for 1≤l≤k1\leq l\leq k.

Voiculescu first defined freeness with amalgamation, and developed its basic theory in voi . Conditional independence and freeness with amalgamation also have rich combinatorial theories, which we now recall. In the free case this is due to Speicher sp2 ; see also ns .

A partition π\pi of a set SS is a collection of disjoint, nonempty sets V1,…,VrV_{1},\ldots,V_{r} such that V1∪⋯∪Vr=SV_{1}\cup\cdots\cup V_{r}=S. V1,…,VrV_{1},\ldots,V_{r} are called the blocks of π\pi, and we set ∣π∣=r|\pi|=r. The collection of partitions of SS will be denoted P(S)P(S), or in the case that S={1,…,k}S=\{1,\ldots,k\} by P(k)P(k).

Given π,σ∈P(S)\pi,\sigma\in P(S), we say that π≤σ\pi\leq\sigma if each block of π\pi is contained in a block of σ\sigma. There is a least element of P(S)P(S) which is larger than both π\pi and σ\sigma, which we denote by π∨σ\pi\vee\sigma.

If SS is ordered, we say that π∈P(S)\pi\in P(S) is noncrossing if whenever V,WV,W are blocks of π\pi and s1<t1<s2<t2s_{1}<t_{1}<s_{2}<t_{2} are such that s1,s2∈Vs_{1},s_{2}\in V and t1,t2∈Wt_{1},t_{2}\in W, then V=WV=W. The set of noncrossing partitions of SS is denoted by NC(S)\mathit{NC}(S), or by NC(k)\mathit{NC}(k) in the case that S={1,…,k}S=\{1,\ldots,k\}.

The noncrossing partitions can also be defined recursively, a partition π∈P(S)\pi\in P(S) is noncrossing if and only if it has a block VV which is an interval, such that π∖V\pi\setminus V is a noncrossing partition of S∖VS\setminus V.

Given i1,…,iki_{1},\ldots,i_{k} in some index set II, we denote by ker⁡i\ker\mathbf{i} the element of P(k)P(k) whose blocks are the equivalence classes of the relation

Note that if π∈P(k)\pi\in P(k), then π≤ker⁡i\pi\leq\ker\mathbf{i} is equivalent to the condition that whenever ss and tt are in the same block of π\pi, isi_{s} must equal iti_{t}.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space. {longlist}[(2)]

A B\mathcal{B}-functional is a nn-linear map ρ\dvtxAn→B\rho\dvtx\mathcal{A}^{n}\to\mathcal{B} such that

for all b0,…,bn∈Bb_{0},\ldots,b_{n}\in\mathcal{B} and a1,…,ana_{1},\ldots,a_{n}. Equivalently, ρ\rho is a linear map from A⊗Bn\mathcal{A}^{\otimes_{\mathcal{B}}n} to B\mathcal{B}, where the tensor product is taken with respect to the natural B−B\mathcal{B}-\mathcal{B}-bimodule structure on A\mathcal{A}.

where if V=(i1<⋯<is)V=(i_{1}<\cdots<i_{s}) is a block of π\pi then

If B\mathcal{B} is noncommutative, there is no natural order in which to compute the product appearing in the above formula for ρ(π)\rho^{(\pi)}. However, the nesting property of noncrossing partitions allows for a natural definition of ρ(π)\rho^{(\pi)} for π∈NC(n)\pi\in\mathit{NC}(n), which we now recall from sp2 .

If π=1n\pi=1_{n} is the partition containing only one block, define ρ(π)=ρ(n)\rho^{(\pi)}=\rho^{(n)}.

Otherwise, let V={l+1,…,l+s}V=\{l+1,\ldots,l+s\} be an interval of π\pi and define

then the corresponding ρ(π)\rho^{(\pi)} is given by

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and let (xi)i∈I(x_{i})_{i\in I} be a family of random variables in A\mathcal{A}. {longlist}[(2)]

The operator-valued classical cumulants cE(k)\dvtxAk→Bc_{E}^{(k)}\dvtx\mathcal{A}^{k}\to\mathcal{B} are the B\mathcal{B}-functionals defined by the classical moment-cumulant formula

Note that the right-hand side of the equation is equal to cE(n)[a1,…,an]c_{E}^{(n)}[a_{1},\ldots,a_{n}] plus lower order terms, and hence cE(n)c_{E}^{(n)} can be solved for recursively.

The operator-valued free cumulants κE(k)\dvtxAk→B\kappa_{E}^{(k)}\dvtx\mathcal{A}^{k}\to\mathcal{B} are the B\mathcal{B}-functionals defined by the free moment-cumulant formula

As above, this equation can be solved recursively for κE(n)\kappa_{E}^{(n)}.

While the definitions of conditional independence and freeness with amalgamation given above appear at first to be quite different, they have very similar expressions in terms of cumulants. In the free case, the following theorem is due to Speicher sp2 .

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and (xi)i∈I(x_{i})_{i\in I} a family of random variables in A\mathcal{A}. {longlist}[(2)]

If the algebra generated by B\mathcal{B} and (xi)i∈I(x_{i})_{i\in I} is commutative, then the variables are conditionally independent given BB if and only if

whenever there are 1≤k,l≤n1\leq k,l\leq n such that ik≠ili_{k}\neq i_{l}.

The variables are free with amalgamation over B\mathcal{B} if and only if

whenever there are 1≤k,l≤n1\leq k,l\leq n such that ik≠ili_{k}\neq i_{l}.

Note that the condition in (1) is equivalent to the statement that if π∈P(n)\pi\in P(n), then

unless π≤ker⁡i\pi\leq\ker\mathbf{i}, and likewise in (2) for π∈NC(n)\pi\in\mathit{NC}(n). Stronger characterizations of the joint distribution of (xi)i∈I(x_{i})_{i\in I} can be given by specifying what types of partitions may contribute nonzero cumulants.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and let (xi)i∈I(x_{i})_{i\in I} be a family of random variables in A\mathcal{A}. {longlist}[(2)]

Suppose that B\mathcal{B} and (xi)i∈I(x_{i})_{i\in I} generate a commutative algebra. The B\mathcal{B}-valued joint distribution of (xi)i∈I(x_{i})_{i\in I} has the property corresponding to DD in the table below if and only if for any π∈P(n)\pi\in P(n)

unless π∈D(n)\pi\in D(n) and π≤ker⁡i\pi\leq\ker\mathbf{i}.

The B\mathcal{B}-valued joint distribution of (xi)i∈I(x_{i})_{i\in I} has the property corresponding to DD in the the table below if and only if for any π∈NC(n)\pi\in\mathit{NC}(n)

unless π∈D(n)\pi\in D(n) and π≤ker⁡i\pi\leq\ker\mathbf{i}.

These results are well known. In the classical case, note that the results for P2,PbP_{2},P_{b} are equivalent to the Wick formula for computing moments of independent Gaussian families. In the free case, see sp2 , ns .

It is clear from the definitions that the classical and free cumulants can be solved for from the joint moments. In fact, a combinatorial formula for the cumulants in terms of the moments can be given. First we recall the definition of the Möbius function on a partially ordered set.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and let (xi)i∈I(x_{i})_{i\in I} be a family of random variables. Define the B\mathcal{B}-valued moment functionals E(n)E^{(n)} by

Suppose that B\mathcal{B} is commutative. Then for any σ∈P(n)\sigma\in P(n) and a1,…,an∈Aa_{1},\ldots,\allowbreak a_{n}\in\mathcal{A}, we have

For any σ∈NC(n)\sigma\in\mathit{NC}(n) and a1,…,an∈Aa_{1},\ldots,a_{n}\in\mathcal{A}, we have

This follows from the Möbius inversion formula; see sp2 , ns .

Easy quantum groups

We will now briefly recall some notions and results from bsp .

Consider a compact group G⊂OnG\subset O_{n}. By the Stone–Weierstrauss theorem, C(G)C(G) is generated by the n2n^{2} coordinate functions uiju_{ij} sending a matrix in GG to its (i,j)(i,j) entry. The structure of GG as a compact group is captured by the commutative Hopf C∗-algebra C(G)C(G) together with comultiplication, counit and antipode determined by

Dropping the condition of commutativity, we obtain the following definition, adapted from the fundamental paper of Woronowicz wor1 .

An orthogonal Hopf algebra is a unital C∗-algebra AA generated by n2n^{2} self-adjoint elements uiju_{ij}, such that the following conditions hold: {longlist}[(3)]

The inverse of u=(uij)∈Mn(A)u=(u_{ij})\in M_{n}(A) is the transpose ut=(uji)u^{t}=(u_{ji}).

Δ(uij)=∑kuik⊗ukj\Delta(u_{ij})=\sum_{k}u_{ik}\otimes u_{kj} determines a morphism Δ\dvtxA→A⊗A\Delta\dvtx A\to A\otimes A.

S(uij)=ujiS(u_{ij})=u_{ji} defines a morphism S\dvtxA→AopS\dvtx A\to A^{op}.

It follows from the definitions that Δ,ε,S\Delta,\varepsilon,S satisfy the usual Hopf algebra axioms. If AA is an orthogonal Hopf algebra, we use the heuristic formula “A=C(G)A=C(G),” where GG is an compact orthogonal quantum group. Of course if AA is noncommutative, then GG cannot exist as a concrete object, and all statements about GG must be interpreted in terms of the Hopf algebra AA.

The following two examples, constructed by Wang in wang1 , wang2 , are fundamental to our considerations.

Ao(n)A_{o}(n) is the universal C∗-algebra generated by n2n^{2} self-adjoint elements uiju_{ij}, such that u=(uij)∈Mn(Ao(n))u=(u_{ij})\in M_{n}(A_{o}(n)) is orthogonal.

As(n)A_{s}(n) is the universal C∗-algebra generated by n2n^{2} projections uiju_{ij}, such that the sum along any row or column of u=(uij)∈Mn(As(n))u=(u_{ij})\in M_{n}(A_{s}(n)) is the identity.

As discussed above, we use the notation Ao(n)=C(On+)A_{o}(n)=C(O_{n}^{+}), As(n)=C(Sn+)A_{s}(n)=C(S_{n}^{+}), and call On+O_{n}^{+} and Sn+S_{n}^{+} the free orthogonal group and free permutation group, respectively.

Here the δ\delta symbol appearing on the right-hand side is 1 when the indices “fit,” that is, if each block of π\pi contains equal indices, and 0 otherwise.

It follows from the above discussion that Hom⁡(u⊗k,u⊗l)\operatorname{Hom}(u^{\otimes k},u^{\otimes l}) consists of certain linear combinations of the operators TπT_{\pi}, with π∈P(k,l)\pi\in P(k,l). We call GG “easy” if these spaces are spanned by partitions.

There are four natural examples of classical groups which are easy:

There is a one-to-one correspondence between classical easy groups and free quantum groups, which on a combinatorial level corresponds to restricting to noncrossing partitions:

There are also free versions of Sn′,Bn′S_{n}^{\prime},B_{n}^{\prime}, constructed in bsp .

In general, the class of easy quantum groups appears to be quite rigid (see bcs1 for a discussion here). However, two more examples can be obtained as “half-liberations.” The idea is that instead of removing the commutativity relations from the generators uiju_{ij} of C(G)C(G) for a classical easy group GG, which would produce C(G+)C(G^{+}), we instead require that the the generators “half-commute,” that is, abc=cbaabc=cba for a,b,c∈{uij}a,b,c\in\{u_{ij}\}. More precisely, we define C(G∗)=C(G+)/IC(G^{*})=C(G^{+})/I, where II is the ideal generated by the relations abc=cbaabc=cba for a,b,c∈{uij}a,b,c\in\{u_{ij}\}. For G=Sn,Sn′,Bn,Bn′G=S_{n},S_{n}^{\prime},B_{n},B_{n}^{\prime} we have G∗=GG^{*}=G, however for On,HnO_{n},H_{n}, we obtain new quantum groups On∗,Hn∗O_{n}^{*},H_{n}^{*}. The corresponding partition categories E2,EhE_{2},E_{h} consist of all pair partitions, respectively all partitions, which are balanced in the sense that each block contains as many odd as even legs.

Half independence

In this section, we introduce a new kind of independence which appears in the de Finetti theorems for the half-liberated quantum groups H∗H^{*} and O∗O^{*}. To define this notion, we require that the variables have a certain degree of commutativity.

Let (xi)i∈I(x_{i})_{i\in I} be a family of noncommutative random variables. We say that the variables half-commute if

Observe that if (xi)i∈I(x_{i})_{i\in I} half-commute, then in particular xi2x_{i}^{2} commutes with xjx_{j} for any i,j∈Ii,j\in I.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and suppose that B\mathcal{B} is contained in the center of A\mathcal{A}. Let (xi)i∈I(x_{i})_{i\in I} be a family of random variables in A\mathcal{A} which half-commute. We say that (xi)i∈I(x_{i})_{i\in I} are conditionally half-independent given B\mathcal{B}, or half-independent with respect to EE, if the following conditions are satisfied: {longlist}[(2)]

The variables (xi2)i∈I(x_{i}^{2})_{i\in I} are conditionally independent given B\mathcal{B}.

For any i1,…,ik∈Ii_{1},\ldots,i_{k}\in I, we have

As a first remark, we note that half-independence is defined only between random variables and not at the level of algebras, in contrast with classical and free independence. In fact, it is known from sp1 there are no other good notions of independence between unital algebras other than classical and free.

The conditions may appear at first to be somewhat artificial, but are motivated by the following natural example.

Let (Ω,Σ,μ)(\Omega,\Sigma,\mu) be a (classical) probability space, and let L(μ)L(\mu) denote the algebra of complex-valued random variables on Ω\Omega with finite moments of all orders. {longlist}[(2)]

Let (ξi)i∈I(\xi_{i})_{i\in I} be a family of independent random variables in L(μ)L(\mu). Suppose that for each i∈Ii\in I, the distribution of ξi\xi_{i} is such that

A simple computation shows that the variables (xi)i∈I(x_{i})_{i\in I} half-commute. Since

Observe also that the distribution of xix_{i} is equal to that of (ξiξi‾)1/2(\xi_{i}\overline{\xi_{i}})^{1/2}, where the square root is chosen such that the distribution is even. We call this the squeezed version of the complex distribution ξi\xi_{i} (cf. bsp ).

Of particular interest is the case that the (ξi)i∈I(\xi_{i})_{i\in I} have complex Gaussian distributions. Here the distribution of xix_{i} is the squeezed version of the complex Gaussian ξi\xi_{i}, which is a symmetrized Rayleigh distribution.

We will show in Proposition 2.8 below that any half-independent family can be modeled as in the example above. First, we will show that, as for classical and free independence, the joint distribution of a family of half-independent random variables (xi)i∈I(x_{i})_{i\in I} is determined by the distributions of xix_{i} for i∈Ii\in I. It is convenient to first introduce the following family of permutations which are related to the half-commutation relation.

We say that a permutation ω∈Sn\omega\in S_{n} preserves parity if ω(i)≡i (mod⁡2)\omega(i)\equiv i~{}(\operatorname{mod}2) for 1≤i≤n1\leq i\leq n.

The collection of parity preserving partitions in SnS_{n} clearly form a subgroup, which is simply S({1,3,…})×S({2,4,…})S(\{1,3,\ldots\})\times S(\{2,4,\ldots\}). Moreover, this subgroup is generated by the transpositions (i  i+2)(i\;i+2) for 1≤i≤n−21\leq i\leq n-2. It follows that if (xi)i∈I(x_{i})_{i\in I} half-commute, then

whenever ω∈Sn\omega\in S_{n} preserves parity.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space such that B\mathcal{B} is contained in the center of A\mathcal{A}. Suppose that (xi)i∈I(x_{i})_{i\in I} is a family of random variables in A\mathcal{A} which are conditionally half-independent given B\mathcal{B}. Then the B\mathcal{B}-valued joint distribution of (xi)i∈I(x_{i})_{i\in I} is uniquely determined by the B\mathcal{B}-valued distributions of xix_{i} for i∈Ii\in I.

Let i1,…,ik∈Ii_{1},\ldots,i_{k}\in I. We know that

unless we have that for each i∈Ii\in I, the set of 1≤j≤k1\leq j\leq k such that ij=ii_{j}=i has as many odd as even elements. So suppose that this the case. By the remark above, we know that xi1⋯xik=xiω(1)⋯xiω(k)x_{i_{1}}\cdots x_{i_{k}}=x_{i_{\omega(1)}}\cdots x_{i_{\omega(k)}} whenever ω∈Sk\omega\in S_{k} is parity preserving. With an appropriate choose of ω\omega, it follows that

Let (Xi)i∈I(X_{i})_{i\in I} be a family of independent random variables such that XiX_{i} has the same distribution as xix_{i}. Let (Ui)i∈I(U_{i})_{i\in I} be a family of independent Haar unitary random variables which are independent from (Xi)i∈I(X_{i})_{i\in I}, and let ξi=UiXi\xi_{i}=U_{i}X_{i}. Then (ξi)i∈I(\xi_{i})_{i\in I} are independent and

From Example 2.4, the variables (yi)i∈I(y_{i})_{i\in I} defined by

are half-independent, and yiy_{i} has the same distribution as xix_{i} for each i∈Ii\in I. By Lemma 2.7, (yi)i∈I(y_{i})_{i\in I} has the same joint distribution as (xi)i∈I(x_{i})_{i\in I}.

We will now develop a combinatorial theory for half-independence, based on the family EhE_{h} of balanced partitions.

Let (A,E\dvtxA→B)(\mathcal{A},E\dvtx\mathcal{A}\to\mathcal{B}) be an operator-valued probability space, and suppose that B\mathcal{B} is contained in the center of A\mathcal{A}. Let (xi)i∈I(x_{i})_{i\in I} be a family of random-variables in A\mathcal{A}, and suppose that

for any odd kk and i1,…,ik∈Ii_{1},\ldots,i_{k}\in I. Define the half-liberated cumulants γE(n)\gamma_{E}^{(n)} by the half-liberated moment-cumulant formula

where γE(π)[xi1,…,xik]\gamma_{E}^{(\pi)}[x_{i_{1}},\ldots,x_{i_{k}}] is defined, as in the classical case, by the formula

Observe that both sides of the moment-cumulant formula above are equal to zero for odd values of kk, and for even values the right hand side is equal to γE(k)[xi1,…,xik]\gamma_{E}^{(k)}[x_{i_{1}},\ldots,x_{i_{k}}] plus products of lower ordered terms and hence γE(k)\gamma_{E}^{(k)} may be solved for recursively. As in the free and classical cases, we may apply the Möbius inversion formula to obtain the following equation for γE(π)\gamma_{E}^{(\pi)}, π∈Eh(k)\pi\in E_{h}(k):

E[xi1⋯xik]=0E[x_{i_{1}}\cdots x_{i_{k}}]=0 whenever kk is odd, and

for any π∈Eh(k)\pi\in E_{h}(k) such that π≰ker⁡i\pi\not\leq\ker\mathbf{i}.

First, suppose that condition (2) holds. From the moment-cumulant formula, we have

so that (xi2)i∈I(x_{i}^{2})_{i\in I} are independent and hence (xi)i∈I(x_{i})_{i\in I} are half-independent.

The implication (1)⇒(2)(1)\Rightarrow(2) actually follows from (2)⇒(1)(2)\Rightarrow(1). Indeed, suppose that (xi)i∈I(x_{i})_{i\in I} are half-independent. Consider the algebra A′=B⟨yi\dvtxi∈I⟩/⟨yiyjyk=ykyjyi⟩\mathcal{A}^{\prime}=\mathcal{B}\langle y_{i}\dvtx i\in I\rangle/\langle y_{i}y_{j}y_{k}=y_{k}y_{j}y_{i}\rangle of polynomials in half-commuting indeterminates (yi)i∈I(y_{i})_{i\in I} and coefficients in B\mathcal{B}. Define a conditional expectation E′\dvtxA′→BE^{\prime}\dvtx\mathcal{A}^{\prime}\to\mathcal{B} by

(It is easy to see that E′E^{\prime} is well defined, that is, compatible with the half-commutation relations.) Since the half-liberated cumulants are uniquely determined by the moment-cumulant formula, it follows that

By the first part, it follows that (yi)i∈I(y_{i})_{i\in I} are half-independent with respect to E′E^{\prime}. Since yiy_{i} has the same B\mathcal{B}-valued distribution as xix_{i}, it follows from Lemma 2.7 that (yi)i∈I(y_{i})_{i\in I} have the same joint distribution as (xi)i∈I(x_{i})_{i\in I}. It then follows from the moment-cumulant formula that these families have the same half-liberated cumulants, and hence γE(π)[xi1,…,xik]=0\gamma_{E}^{(\pi)}[x_{i_{1}},\ldots,x_{i_{k}}]=0 unless π≤ker⁡i\pi\leq\ker\mathbf{i}.

Recall that (centered) Gaussian and semicircular distributions are characterized by the property that their nonvanishing cumulants are those corresponding to pair and noncrossing pair partitions, respectively. We will now show that for half-independence, it is the symmetrized Rayleigh distribution which has this property. This follows from the considerations in bsp , but we include here a direct proof.

Let xx be a random variable in (A,φ)(\mathcal{A},\varphi) which has an even distribution. Then xx has a symmetrized Rayleigh distribution if and only if

for any π∈Eh(k)\pi\in E_{h}(k) such that π∉E2(k)\pi\notin E_{2}(k).

Since the distribution of xx is determined uniquely by its half-liberated cumulants, it suffices to show that if the cumulants have the stated property then xx has a symmetrized Rayleigh distribution. Suppose that this is the case, then

It is easy to see that the number of partitions in E2(k)E_{2}(k) is m!m! if k=2mk=2m is even and is zero if kk is odd. Since these agree with the moments of a symmetrized Rayleigh distribution, the result follows.

Weingarten estimate

If G⊂OnG\subset O_{n} is a compact group, then the Haar state on C(G)C(G) is given by integrating against the Haar measure on GG.

One quite useful aspect of the easiness condition for a compact orthogonal quantum group is that it leads to a combinatorial Weingarten formula for computing the Haar state, which we now recall from bsp .

GknG_{kn} is invertible for nn sufficiently large (see Proposition 3.4), define the Weingarten matrix WknW_{kn} to be its inverse.

Let G⊂On+G\subset O_{n}^{+} be an easy quantum group and let D(k)⊂P(0,k)D(k)\subset P(0,k) be the corresponding collection of partitions having no upper points. If GknG_{kn} is invertible, then

The statement of the theorem above is from bsp , but goes back to work of Weingarten wein and was developed in a series of papers col , cos , bc1 , bc2 . Note that this reduces the problem of evaluating integrals over GG to computing the entries of the Weingarten matrix. We will now give an estimate on the asymptotic behavior of WknW_{kn} as n→∞n\to\infty. This unifies and extends the estimates given in bc1 and cur3 for O+,S+O^{+},S^{+}.

Wkn(π,σ)=O(n∣π∨σ∣−∣π∣−∣σ∣)W_{kn}(\pi,\sigma)=O(n^{|\pi\vee\sigma|-|\pi|-|\sigma|}).

where μD(k)\mu_{D(k)} is the Möbius function on the partially ordered set D(k)D(k) under the restriction of the order on P(k)P(k).

We use a standard method from col , cos , further developed in bc1 , bc2 , cur1 .

Note that the entries of BknB_{kn} are O(n−1/2)O(n^{-1/2}), it follows that for nn sufficiently large 1+Bkn1+B_{kn} is invertible and

So to prove (1), it suffices to show that if ν1,…,νl∈D(k)\nu_{1},\ldots,\nu_{l}\in D(k), then

We will use the fact that P(k)P(k) is a semi-modular lattice (birk , Section I.8, Example 9): If ν,τ∈P(k)\nu,\tau\in\mathcal{P}(k), then

We will now prove the claim by induction on ll, for l=1l=1 we may apply the formula above to find

Also ∣νl∨σ∣≤∣π∨σ∣+∣νl∣−∣π∨νl∣|\nu_{l}\vee\sigma|\leq|\pi\vee\sigma|+|\nu_{l}|-|\pi\vee\nu_{l}|, and the result follows.

To prove (2), suppose π,σ∈D(k)\pi,\sigma\in D(k) and π≤σ\pi\leq\sigma. The terms which contribute to order n−∣π∣n^{-|\pi|} in the expansion come from sequences ν1,…,νl∈D(k)\nu_{1},\ldots,\nu_{l}\in D(k) such that π≠ν1≠⋯≠νl≠σ\pi\neq\nu_{1}\neq\cdots\neq\nu_{l}\neq\sigma and

Since ∣π∨ν1∣≤∣ν1∣|\pi\vee\nu_{1}|\leq|\nu_{1}|, ∣ν1∨ν2∣≤∣ν2∣,…,∣νl∨σ∣≤σ|\nu_{1}\vee\nu_{2}|\leq|\nu_{2}|,\ldots,|\nu_{l}\vee\sigma|\leq\sigma, it follows that each of these must be an equality, which implies π<ν1<⋯<νl<σ\pi<\nu_{1}<\cdots<\nu_{l}<\sigma. Conversely, any ν1,…,νl∈D(k)\nu_{1},\ldots,\nu_{l}\in D(k) such that π<ν1<⋯<νl<σ\pi<\nu_{1}<\cdots<\nu_{l}<\sigma clearly satisfy this equation. Therefore, the coefficient of n−∣π∣n^{-|\pi|} in Wkn(π,σ)W_{kn}(\pi,\sigma) is

which is precisely μD(k)(π,σ)\mu_{D(k)}(\pi,\sigma).

Recall that the free, half-liberated and classical cumulants are obtained from moment functionals by using the Möbius functions on NC,Eh\mathit{NC},E_{h} and PP, respectively. To show that this is compatible with Proposition 3.4, we will need the following result.

If D=NC,NC2,NCb,NChD=\mathit{NC},\mathit{NC}_{2},\mathit{NC}_{b},\mathit{NC}_{h}, then

Let Q=NC,Eh,PQ=\mathit{NC},E_{h},P according to cases (1), (2), (3). It is easy to see in each case that D(k)D(k) is closed under taking intervals in Q(k)Q(k), that is, if π1,π2∈D(k)\pi_{1},\pi_{2}\in D(k), σ∈Q(k)\sigma\in Q(k) and π1<σ<π2\pi_{1}<\sigma<\pi_{2} then σ∈D(k)\sigma\in D(k). The result now follows immediately from the definition of the Möbius function.

Finite quantum invariant sequences

We begin this section by defining the notion of quantum invariance for a sequence of noncommutative random variables under “transformations” coming from an orthogonal quantum group Gn⊂On+G_{n}\subset O_{n}^{+}.

It is easily verified that αn\alpha_{n} is an action of GnG_{n}, that is,

for all p∈Pnp\in\mathscr{P}_{n}. More explicitly, the sequence (x1,…,xn)(x_{1},\ldots,x_{n}) is GnG_{n}-invariant if

Suppose that Gn⊂OnG_{n}\subset O_{n} is a compact group. By evaluating both sides of the above equation at g∈Gng\in G_{n}, we see that a sequence (x1,…,xn)(x_{1},\ldots,x_{n}) is GnG_{n}-invariant if and only if

We will now prove a converse to Theorem 1, which holds for finite sequences and in a purely algebraic context. The proof is adapted from the method of ksp , Proposition 3.1.

Let (A,φ)(\mathcal{A},\varphi) be a noncommutative probability space, 1∈B⊂A1\in\mathcal{B}\subset\mathcal{A} a unital subalgebra and E\dvtxA→BE\dvtx\mathcal{A}\to\mathcal{B} a conditional expectation which preserves φ\varphi. Let (x1,…,xn)(x_{1},\ldots,x_{n}) be a sequence in A\mathcal{A}.

If x1,…,xnx_{1},\ldots,x_{n} are freely independent and identically distributed with amalgamation over B\mathcal{B}, then the sequence is Sn+S_{n}^{+}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are freely independent and identically distributed with amalgamation over B\mathcal{B}, and have even distributions with respect to EE, then the sequence is Hn+H_{n}^{+}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are freely independent and identically distributed with amalgamation over B\mathcal{B}, and have semicircular distributions with respect to EE, then the sequence is Bn+B_{n}^{+}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are freely independent and identically distributed with amalgamation over B\mathcal{B}, and have centered semicircular distributions with respect to EE, then the sequence is On+O_{n}^{+}-invariant.

Half-liberated case: Suppose that (x1,…,xn)(x_{1},\ldots,x_{n}) half-commute, and that B\mathcal{B} is central in A\mathcal{A}. {longlist}[(b)]

If x1,…,xnx_{1},\ldots,x_{n} are half-independent and identically distributedgiven B\mathcal{B}, then the sequence is Hn∗H_{n}^{*}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are half-independent and identically distributedgiven B\mathcal{B}, and have symmetrized Rayleigh distributions with respect to EE, then the sequence is On∗O_{n}^{*}-invariant.

Suppose that B\mathcal{B} and x1,…,xnx_{1},\ldots,x_{n} generate a commutative algebra. {longlist}[(b)]

If x1,…,xnx_{1},\ldots,x_{n} are conditionally independent and identically distributed given B\mathcal{B}, then the sequence is SnS_{n}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are conditionally independent and identically distributed given B\mathcal{B}, and have even distributions with respect to EE, then the sequence is HnH_{n}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are conditionally independent and identically distributed given B\mathcal{B}, and have Gaussian distributions with respect to EE, then the sequence is BnB_{n}-invariant.

If x1,…,xnx_{1},\ldots,x_{n} are conditionally independent and identically distributed given B\mathcal{B}, and have centered Gaussian distributions with respect to EE, then the sequence is OnO_{n}-invariant.

where ξ\xi denotes the free, half-liberated or classical cumulants in cases (1), (2) and (3), respectively. It follows from the considerations in bsp , or by direct computation, that if π∈D(k)\pi\in D(k) then

To prove the approximation result for finite sequences, we will require more analytic structure. Throughout the rest of the section, we will assume that Gn⊂On+G_{n}\subset O_{n}^{+} is a compact quantum group, (M,φ)(M,\varphi) is a W∗-probability space and (x1,…,xn)(x_{1},\ldots,x_{n}) is a sequence of self-adjoint random variables in MM. We denote the von Neumann algebra generated by (x1,…,xn)(x_{1},\ldots,x_{n}) by MnM_{n}, and define the GnG_{n}-invariant subalgebra by

where Pnαn\mathscr{P}_{n}^{\alpha_{n}} denotes the fixed point algebra of the action αn\alpha_{n}, that is,

We now begin the technical preparations for our approximation result. First, we will need to extend the action αn\alpha_{n} to the von Neumann algebra context. L∞(Gn)L^{\infty}(G_{n}) will denote the von Neumann algebra obtained by taking the weak closure of πn(C(Gn))\pi_{n}(C(G_{n})), where πn\pi_{n} is the GNS representation of C(Gn)C(G_{n}) on the GNS Hilbert space L2(Gn)L^{2}(G_{n}) for the Haar state. L∞(Gn)L^{\infty}(G_{n}) is a Hopf von Neumann algebra, with the natural structure induced from C(Gn)C(G_{n}).

Suppose that (x1,…,xn)(x_{1},\ldots,x_{n}) is GnG_{n}-invariant. Then there is a right coaction α~n\dvtxMn→Mn⊗L∞(Gn)\widetilde{\alpha}_{n}\dvtx M_{n}\to M_{n}\otimes L^{\infty}(G_{n}) determined by

for p∈Pnp\in\mathscr{P}_{n}. Moreover, the fixed point algebra of α~n\widetilde{\alpha}_{n} is precisely the GnG_{n}-invariant subalgebra Bn\mathcal{B}_{n}.

There is a natural conditional expectation En\dvtxMn→BnE_{n}\dvtx M_{n}\to\mathcal{B}_{n} given by integrating the coaction α~n\widetilde{\alpha}_{n} with respect to the Haar state, that is,

By using the Weingarten calculus, we can give a simple combinatorial formula for the moment functionals with respect to EnE_{n} if GnG_{n} is one of the easy quantum groups under consideration. In the half-liberated case, we must first show that Bn\mathcal{B}_{n} is central in MnM_{n}.

Suppose that (x1,…,xn)(x_{1},\ldots,x_{n}) half-commute. If Hn∗⊂GnH_{n}^{*}\subset G_{n}, then the GnG_{n}-invariant subalgebra Bn\mathcal{B}_{n} is contained in the center of MnM_{n}.

Since xi2x_{i}^{2} is central in MnM_{n} for 1≤i≤n1\leq i\leq n, the result follows.

Suppose that (x1,…,xn)(x_{1},\ldots,x_{n}) is GnG_{n}-invariant, and that one of the following conditions is satisfied: {longlist}[(3)]

GnG_{n} is a free quantum group On+,Sn+,Hn+O_{n}^{+},S_{n}^{+},H_{n}^{+} or Bn+B_{n}^{+}.

GnG_{n} is a half-liberated quantum group On∗O_{n}^{*} or Hn∗H_{n}^{*} and (x1,…,xn)(x_{1},\ldots,x_{n}) half-commute.

GnG_{n} is an easy group On,Sn,HnO_{n},S_{n},H_{n} or BnB_{n} and (x1,…,xn)(x_{1},\ldots,x_{n}) commute. Then for any π\pi in the partition category D(k)D(k) for the easy quantum group GnG_{n}, and any b0,…,bk∈Bnb_{0},\ldots,b_{k}\in\mathcal{B}_{n}, we have

which holds if nn is sufficiently large that the Gram matrix GknG_{kn} is invertible.

We prove this by induction on the number of blocks of π\pi. First, suppose that π=1k\pi=1_{k} is the partition with only one block. Then

where we have used the fact that b0,…,bkb_{0},\ldots,b_{k} are fixed by the coaction α~n\widetilde{\alpha}_{n}. Applying the Weingarten integration formula in Proposition 3.2, we have

Observe that Gkn(σ,1k)=n∣σ∨1k∣=nG_{kn}(\sigma,1_{k})=n^{|\sigma\vee 1_{k}|}=n for any σ∈D(k)\sigma\in D(k). It follows that for any π∈D(k)\pi\in D(k), we have

If condition (2) or (3) are satisfied, then the general case follows from the formula

where in the half-liberated case we are applying the previous lemma. The one thing we must check here is that if π∈D(k)\pi\in D(k) and VV is a block of π\pi with ss elements, then 1s∈D(s)1_{s}\in D(s). This is easily verified, in each case, for D=P,P2,Ph,Pb,Eh,E2D=P,P_{2},P_{h},P_{b},E_{h},E_{2}.

Suppose now that condition (1) is satisfied. Let π∈D(k)\pi\in D(k). Since π\pi is noncrossing, π\pi contains an interval V={l+1,…,l+s+1}V=\{l+1,\ldots,l+s+1\}. We then have

To apply induction, we must check that π∖V∈D(k−s)\pi\setminus V\in D(k-s) and 1s∈D(s)1_{s}\in D(s). Indeed, this is easily verified for NC,NC2,NCh\mathit{NC},\mathit{NC}_{2},\mathit{NC}_{h} and NCb\mathit{NC}_{b}. Applying induction, we have

We are now prepared to prove the approximation result for finite sequences.

Suppose that (x1,…,xn)(x_{1},\ldots,x_{n}) is GnG_{n}-invariant, and that one of the following conditions is satisfied: {longlist}[(3)]

GnG_{n} is a free quantum group On+,Sn+,Hn+O_{n}^{+},S_{n}^{+},H_{n}^{+} or Bn+B_{n}^{+}.

GnG_{n} is a half-liberated quantum group On∗O_{n}^{*} or Hn∗H_{n}^{*} and (x1,…,xn)(x_{1},\ldots,x_{n}) half-commute.

GnG_{n} is an easy group On,Sn,HnO_{n},S_{n},H_{n} or BnB_{n} and (x1,…,xn)(x_{1},\ldots,x_{n}) commute. Let (y1,…,yn)(y_{1},\ldots,y_{n}) be a sequence of Bn\mathcal{B}_{n}-valued random variables with Bn\mathcal{B}_{n}-valued joint distribution determined as follows:

G=O+G=O^{+}: Free semicircular, centered with same variance as x1x_{1}.

G=S+G=S^{+}: Freely independent, yiy_{i} has same distribution as x1x_{1}.

G=H+G=H^{+}: Freely independent, yiy_{i} has same distribution as x1x_{1}.

G=B+G=B^{+}: Free semicircular, same mean and variance as x1x_{1}.

G=O∗G=O^{*}: Half-liberated Gaussian, same variance as x1x_{1}.

G=H∗G=H^{*}: Half-independent, yiy_{i} has same distribution as x1x_{1}.

G=OG=O: Independent Gaussian, centered with same variance as x1x_{1}.

G=SG=S: Independent, yiy_{i} has same distribution as x1x_{1}.

G=HG=H: Independent, yiy_{i} has same distribution as x1x_{1}.

G=BG=B: Independent Gaussian, same mean and variance as x1x_{1}.

If 1≤j1,…,jk≤n1\leq j_{1},\ldots,j_{k}\leq n and b0,…,bk∈Bnb_{0},\ldots,b_{k}\in\mathcal{B}_{n}, then

where Ck(G)C_{k}(G) is a universal constant which depends only on kk and the easy quantum group GG.

First, we note that it suffices to prove the statement for nn sufficiently large, in particular we will assume throughout that nn is sufficiently large for the Gram matrix GknG_{kn} to be invertible.

Let 1≤j1,…,jk≤n1\leq j_{1},\ldots,j_{k}\leq n and b0,…,bk∈Bnb_{0},\ldots,b_{k}\in\mathcal{B}_{n}. We have

On the other hand, it follows from the assumptions on (y1,…,yn)(y_{1},\ldots,y_{n}) and the various moment-cumulant formulae that

where ξ\xi denotes the relevant free, classical or half-liberated cumulants. The right-hand side can be expanded, via Möbius inversion, in terms of expectation functionals En(π)[b0x1b1,…,x1bk]E_{n}^{(\pi)}[b_{0}x_{1}b_{1},\ldots,x_{1}b_{k}] where π\pi is a partition in NC,Eh,P\mathit{NC},E_{h},P according to cases (1), (2), (3), and π≤σ\pi\leq\sigma for some σ∈D(k)\sigma\in D(k). Now if π∉D(k)\pi\notin D(k) then we claim that this expectation functional is zero. Indeed this is only possible if D=NC2,NCh,P2,PhD=\mathit{NC}_{2},\mathit{NC}_{h},P_{2},P_{h} and π\pi has a block with an odd number of legs. But it is easy to see that in these cases x1x_{1} has an even distribution with respect to EnE_{n}, and therefore En(π)[b0x1b1,…,x1bk]=0E_{n}^{(\pi)}[b_{0}x_{1}b_{1},\ldots,x_{1}b_{k}]=0 as claimed. This observation, together with Proposition 3.5, allows to to rewrite the above equation as

Comparing these two equations, we find that

Now since x1,…,xnx_{1},\ldots,x_{n} are identically distributed with respect to the faithful state φ\varphi, it follows that these variables have the same norm. Therefore,

for any π∈D(k)\pi\in D(k). Combining this with former equation, we have

which is finite by Proposition 3.4, completes the proof.

Infinite quantum invariant sequences

In this section, we will prove Theorem 1. Throughout this section, we will assume that GG is one of the easy quantum groups O,S,H,B,O∗,H∗,O+,S+,H+O,S,H,B,O^{*},H^{*},O^{+},S^{+},H^{+} or B+B^{+}. We will make use of the inclusions Gn↪GmG_{n}\hookrightarrow G_{m} for n<mn<m, which correspond to the Hopf algebra morphisms ωn,m\dvtxC(Gm)→C(Gn)\omega_{n,m}\dvtx C(G_{m})\to C(G_{n}) determined by

The existence of ωn,m\omega_{n,m} may be verified in each case by using the universal relations of C(Gn)C(G_{n}).

We begin by extending the notion of GnG_{n}-invariance to infinite sequences.

It is clear that βn\beta_{n} is an action of GnG_{n}, moreover we have the relations

where P∞βn\mathscr{P}_{\infty}^{\beta_{n}} is the fixed point algebra of the action βn\beta_{n}. Since

it follows that Bn+1⊂Bn\mathcal{B}_{n+1}\subset\mathcal{B}_{n} for all n≥1n\geq 1. We then define the GG-invariant subalgebra by

for m∈Mm\in M. By taking the limit as n→∞n\to\infty, we obtain a φ\varphi-preserving conditional expectation onto the GG-invariant subalgebra.

For any m∈Mm\in M, the sequence En[m]E_{n}[m] converges in ∣⋅∣2|\cdot|_{2} and the strong topology to a limit E[m]E[m] in B\mathcal{B}. Moreover, EE is a φ\varphi-preserving conditional expectation of MM onto B\mathcal{B}.

Fix π∈NC(k)\pi\in\mathit{NC}(k) and m1,…,mk∈Mm_{1},\ldots,m_{k}\in M, then

The proof follows from cur2 , Proposition 4.7. Note that (1) is just a simple noncommutative reversed martingale convergence theorem. More sophisticated convergence theorems for noncommutative martingales have been obtained; see, for example, gold1 , gold2 .

By Proposition 4.7, and using the compatibility

where ι~n\dvtxW∗(x1,…,xn)→M\widetilde{\iota}_{n}\dvtx W^{*}(x_{1},\ldots,x_{n})\to M is the obvious inclusion and α~n\widetilde{\alpha}_{n} is as in the previous section, we have

As discussed in the proof of Theorem 4.8, we can replace the sum of expectation functionals by cumulants to obtain

where ξ\xi denotes the relevant free, half-liberated or classical cumulants. Since the cumulants are determined by the moment-cumulant formulae, we find that

The result then follows from the characterizations of these joint distributions in terms of cumulants given in Theorem 1.17 and Propositions 2.11 and 2.12.

For simplicity, we have restricted to elements of a von Neumann algebra, that is, bounded random variables, in the statement of Theorem 1. However, for the easy quantum groups O,BO,B and O∗O^{*} the result implies that the variables must have unbounded distributions. In the classical setting, the boundedness assumption can be easily replaced by the condition that x1x_{1} has finite moments of all orders. The key differences are as follows:

First, in the classical case one can replace the uniform bound in Theorem 4.8 by the LpL^{p} estimate

where ∣⋅∣p|\cdot|_{p} denotes the LpL^{p}-norm. The proof is identical, except that one uses Hölder’s identity ∣xi1⋯xik∣p≤∣x1∣pkk|x_{i_{1}}\cdots x_{i_{k}}|_{p}\leq|x_{1}|_{pk}^{k} for any 1≤i1,…,ip≤n1\leq i_{1},\ldots,i_{p}\leq n.

Second, Proposition 5.3 is replaced by a standard LpL^{p} reversed martingale convergence theorem (the statement for expectation functionals requiring another application of Hölder).

With these technical modifications, the proof of Theorem 1 shows that any infinite BB (resp., OO) invariant sequence of classical random variables with finite moments of all orders has the same joint moments with respect to B\mathcal{B} as a conditionally i.i.d. (centered) Gaussian family. But this is sufficient to determine the joint distribution with respect to B\mathcal{B}, since the Gaussian distribution is characterized by its moments.

Concluding remarks

We have seen in this paper that the “easiness” condition from bsp provides a good framework for the study of de Finetti type theorems for orthogonal quantum groups.

A first natural question is what happens in the unitary case. For the classical unitary group UnU_{n}, it is well known that an infinite sequence of complex-valued random variables is unitarily invariant if and only if they are conditionally i.i.d. centered complex Gaussians. For the free unitary group Un+U_{n}^{+} this is considered in cur2 , where it is shown that an infinite sequence of noncommutative random variables is quantum unitarily invariant if and only if they form an operator-valued free circular family with mean zero and common variance. However, the study and classification of easy quantum groups seems to be a quite difficult combinatorial problem in the unitary case, we refer to the concluding section of bsp for a discussion here.

A third question is whether the approximation result in Theorem 4.8 can be strengthened. The main tool that we have available at this time, namely the Weingarten formula, is only suitable for estimates on the joint moments. In df1 , Diaconis and Freedman give refined estimates on the variation norm between the distribution of the coordinates (u11,…,u1k)(u_{11},\ldots,u_{1k}) on SnS_{n} (resp., OnO_{n}) and an independent Bernoulli (resp., Gaussian) distribution. This is used to prove finite de Finetti type results, where the approximations hold in variation norm. It is known from bc1 , bc2 that the coordinates (u11,…,u1k)(u_{11},\ldots,u_{1k}) on Sn+S_{n}^{+} and On+O_{n}^{+} converge in moments to freely independent Bernoulli and semicircular distributions, and it is a natural question whether these converge in a stronger sense. For k=1k=1, it is known from bcz that the distribution of n1/2u11n^{1/2}u_{11} in C(On+)C(O_{n}^{+}) “superconverges” (in the sense of bev ) to the semicircle law, but nothing is currently known for k>1k>1.

Another question is whether the results of Aldous ald for invariant arrays of random variables have suitable extensions to easy quantum groups. We will consider this problem first for free quantum groups in a forthcoming paper cs2 .

Another basic symmetry for a sequence of classical random variables is spreadability, that is, invariance under taking subsequences. Ryll-Nardzewski proved in rn that de Finetti’s theorem in fact holds under this apparently weaker condition. A free analogue of this condition, and of Ryll-Nardzewski’s theorem, has been obtained in cur3 .

Finally, there is the general question of applying our “Sn,OnS_{n},O_{n} philosophy” to other situations. In bcs2 , we have developed a global approach, using the “easiness” formalism, to the fundamental stochastic eigenvalue computations of Diaconis and Shahshahani dsh .

References