Complex Obtuse Random Walks and their Continuous-Time Limits

S. Attal, J. Deschamps, C. Pellegrini

Introduction and Motivations

Since this initial work of was only motivated by Probability Theory and Stochastic Process considerations, there was no real need for an extension of this notion to the complex case. The need for such an extension has appeared naturally through considerations in Quantum Statistical Mechanics. More precisely, the underlying motivation is to characterize the onset of classical noises emerging from quantum baths, in the so-called model of Repeated Quantum Interactions.

Repeated quantum interaction models are physical models, introduced and developed in , which consist in describing the Hamiltonian dynamics of a quantum system undergoing a sequence of interactions with an environment made of a chain of identical systems. These models were developed for they furnish toy models for quantum dissipative systems, they are at the same time Hamiltonian and Markovian, they spontaneously give rise to quantum stochastic differential equations in the continuous time limit. It has been proved in and that they constitute a good toy model for a quantum heat bath in some situations and that they can also give an account of the diffusive behavior of an electron in an electric field, when coupled to a heat bath. When adding to each step of the dynamics a measurement of the piece of the environment which has just interacted, we recover all the discrete-time quantum trajectories for quantum systems (, , ). Physically, this model corresponds exactly to physical experiments such as the ones performed by S. Haroche et al on the quantum trajectories of a photon in a cavity (, , ).

The discrete-time dynamics of these repeated interaction systems, as well as their continuous-time limits, give rise to time evolutions driven by quantum noises coming from the environment. These quantum noises emerging from the environment describe all the possible actions inside the environment (excitation, return to ground state, jumps in between two energy levels, …). It is a remarkable fact that these quantum noises can also be combined together in order to give rise to classical noises. In discrete-time they give rise to any random walk, in continuous-time they give rise to many well-known stochastic processes among which are all the Levy processes.

Surprisingly, the extension of obtuse random variables, obtuse random walks and their continuous-time limits, to the complex case is far from obvious. The algebraical properties of the associated 3-tensors give rise to the same kind of behaviors as in the real case, but, as we shall see in this article, many aspects (such as the diagonalization theorem) become now really non-trivial.

2 Examples

Let us have here a more detailed discussion on these physical motivations underlying our study. These motivations do not appear anymore in the rest of the article which is devoted entirely to the probabilistic properties of complex obtuse random walks and their continuous-time limits, but we have felt that it could be of interest for the reader to have a clearer picture of the physical motivations which have brought us to consider the complex case extension of obtuse random walks. This part can be skipped by the reader, it has no influence whatsoever on the rest of the article, these physical applications are developed in detail in .

Assume that the interaction between these two parts lasts for a small amount of time hh, then the associated unitary evolution operator is U=e−ihHtotU=e^{-ihH_{\rm tot}} which can be decomposed as U=∑i,j=01Uji⊗ajiU=\sum_{i,j=0}^{1}U^{i}_{j}\otimes a^{i}_{j} for some operators UjiU^{i}_{j} on HS\mathcal{H}_{\mathcal{S}}.

The action of the environment (the spin chain) by acting repeatedly of the system HS\mathcal{H}_{\mathcal{S}}, spin by spin, each time for a time duration hh, gives rises to a time evolution driven by a sequence of unitary operators (Vn)(V_{n}) which satisfies (cf for details)

This describes a rather general discrete time evolution for a quantum system and the operators aji(n)a^{i}_{j}(n) here play the role of discrete time quantum noises, they describe all the possible innovations brought by the environment.

In it is shown that if the total Hamiltonian HtotH_{\rm tot} is renormalized under the form

(this can be understood as follows: if the time duration of the interactions hh tends to 0, then then the interaction needs to be strengthen adequately if one wishes to obtain a non-trivial limit) then the time evolution (Vnh)(V_{nh}) converges, when hh tends to 0, to a continuous-time unitary evolution (Vt)(V_{t}) satisfying an equation of the form

which is a quantum stochastic differential equation driven by quantum noises da(t)da(t) and da∗(t)da^{*}(t) on some appropriate Fock space. In other words, we obtain a perturbation of a Schrödinger equation by some additional quantum noise terms.

The point now is that in the special case where L=L∗L=L^{*} then the discrete-time evolution and its continuous-time limit are actually driven by classical noises, for some of the terms in the evolution equation factorize nicely and make appearing classical noises instead of quantum noises (the noises get grouped in order to furnish a family of commuting self-adjoint operators, that is, a classical stochastic process). Indeed, one can show (cf and ) that the discrete time evolution can be written under the form of classical random walk on the unitary group U(HS)\mathcal{U}(\mathcal{H}_{\mathcal{S}}):

where (Xn)(X_{n}) is a sequence of i.i.d. symmetric Bernoulli random variables. The continuous time limit, with the same renormalization as above, gives rise to a unitary evolution driven by a classical Brownian motion (Wt)(W_{t}):

The equation above is the typical one for the perturbation of a Schrödinger equation by means of a Brownian additional term, if one wants the evolution to keep unitary at all times.

This example is a very simple one and belongs to those which were already well-known (cf ); they involve real obtuse random variables and real normal martingales.

which is self-adjoint under the condition B=−(1/2)(A+(1+2i)A∗)B=-(1/2)(A+(1+2i)A^{*}).

In this case the quantum dynamics in discrete time happens to be driven by a classical noise too, but this does not appear obviously here! We will understand, with the tools developed in this article, that the resulting discrete time dynamics is of the form

with probabilities p1=1/3p_{1}=1/3, p2=1/4p_{2}=1/4 and p3=5/12p_{3}=5/{12} respectively.

Putting a 1/h1/\sqrt{h} normalization factor in front of AA and BB and taking the limit hh goes to 0, we will show in this article, that this gives rise to a continuous time dynamics of the form

where (W1 , W2)(W^{1}\,,\,W^{2}) is a 2-dimensional real Brownian motion.

The way these random walks and their characteristics are identified, the way the continuous-time limits and their characteristics are identified, are non-trivial and make use of all the tools we develop along this article: associated doubly-symmetric 3-tensor, diagonalisation of the 3-tensor, probabilistic characteristics of the associated random walk, passage to the limit on the tensor, passage to the limit on the discrete-time martingale, identification of the law of the limit martingale, etc.

3 Structure of the Article

In Section 3 we establish the important symmetries shared by the 3-tensors of obtuse random variables and we show one of our main results: these symmetries are the necessary and sufficient conditions for the 3-tensor to be diagonalizable in some orthonormal basis. We show how to recover the real case, which remarkably does not correspond to the real character of the 3-tensor but to a certain supplementary symmetry.

Section 4 is kind of preparatory to the continuous-time limit of complex obtuse random walks. In this section we show an important connection between complex obtuse random variables and real ones. This connection will be the key for understanding the continuous-time limits. In Section 4 we gather all the results concerning this connection with the real obtuse random variables and its consequences. We recall basic results on real normal martingales and deduce the corresponding ones for the complex normal martingales. In particular we establish what is the complex extension of a structure equation. We connect the behavior of the complex normal martingale to the diagonalization of its associated 3-tensor.

In Section 5 we finally prove our continuous-time convergence theorems. First of all, via the convergence of the tensors, exploiting the results of , we prove a convergence in law for the processes. Secondly, in the framework of Fock space approximation by spin chains developed in , we prove the convergence of the associated multiplication operators, with explicit formulas in terms of quantum noises.

We finally illustrate our results in Section 6 through 2 examples, showing up the different types of behavior.

Complex Obtuse Random Variables

As the v^j\widehat{v}_{j}’s form a basis, this means that

This implies the two announced equalities. □\square

that is, the announced equality. □\square

2 Obtuse Random Variables

We shall also consider the deterministic random variable X0X^{0} on (Ω,F,P)(\Omega,\mathcal{F},P), which is always equal to 11. For i=0,…,Ni=0,\ldots,N let X~i\widetilde{X}^{i} be the random variable defined by

for all i=0,…,Ni=0,\ldots,N and all j=1,…,N+1j=1,\ldots,N+1.

2) The (N+1)×(N+1)(N+1)\times(N+1)-matrix (X~i(j))i,j\left(\widetilde{X}^{i}(j)\right)_{i,j} is a unitary matrix.

3) The (N+1)×(N+1)(N+1)\times(N+1)-matrix (pi v^ij)i,j\left(\sqrt{p_{i}}\,\widehat{v}_{i}^{j}\right)_{i,j} is a unitary matrix.

4) The family {v1,…,vN+1}\{v_{1},\dots,v_{N+1}\} is an obtuse system with

1) ⇒\Rightarrow 2): Since the random variable XX is centered and normalized, each component XiX^{i} has a zero mean and the scalar product between two components XiX^{i}, XjX^{j} is given by the matrix II. Hence, for all ii in {1,…,N}\left\{1,\dots,N\right\}, we get

Now, using Eqs. (4) and (5), we get, for all i,j=1,…,Ni,j=1,\ldots,N

2) ⇒\Rightarrow 1): Conversely, if the matrix (X~i(j))i,j\left(\widetilde{X}^{i}(j)\right)_{i,j} is unitary, the scalar products of column vectors give the mean and the covariance II for the random variable XX.

2) ⇔\Leftrightarrow 3): The matrix (pj v^ij)i,j\left(\sqrt{p_{j}}\,\widehat{v}_{i}^{j}\right)_{i,j} is the transpose matrix of (X~i(j))i,j\left(\widetilde{X}^{i}(j)\right)_{i,j}. Therefore, if one of these two matrices is unitary, its transpose matrix is unitary too.

3) ⇔\Leftrightarrow 4): The matrix (pj v^ji)i,j\left(\sqrt{p_{j}}\,\widehat{v}^{i}_{j}\right)_{i,j} is unitary if and only if

for all i,j=1,…,N+1i,j=1,\ldots,N+1. On the other hand, the condition ⟨pi v^i , pi v^i⟩=1\left\langle\sqrt{p_{i}}\,\widehat{v}_{i}\,,\,\sqrt{p_{i}}\,\widehat{v}_{i}\right\rangle=1 is equivalent to pi (1+∥vi∥2)=1p_{i}\,(1+\|v_{i}\|^{2})=1, whereas the condition ⟨pi v^i , pj v^j⟩=0\left\langle\sqrt{p_{i}}\,\widehat{v}_{i}\,,\,\sqrt{p_{j}}\,\widehat{v}_{j}\right\rangle=0 is equivalent to pi pj (1+⟨vi , vj⟩)=0\sqrt{p_{i}}\,\sqrt{p_{j}}\,(1+\left\langle v_{i}\,,\,v_{j}\right\rangle)=0, that is, ⟨vi , vj⟩=−1 .\left\langle v_{i}\,,\,v_{j}\right\rangle=-1\,. This gives the result. □\square

3 Generic Character of Obtuse Random Variables

In the converse direction, let v1,…,vN+1v_{1},\ldots,v_{N+1} be the possible values of XX, associated to the probabilities p1,…,pN+1p_{1},\ldots,p_{N+1} respectively. Let w1,…,wN+1w_{1},\ldots,w_{N+1} be the ones associated to YY. In particular, the vectors

for all i=1,…,N+1i=1,\ldots,N+1. This gives in particular

As the vi^\widehat{v_{i}}’s are linearly independent then so are the p1v1^−pivi^\sqrt{p_{1}}\widehat{v_{1}}-\sqrt{p_{i}}\widehat{v_{i}}, for i=2,…,N+1i=2,\ldots,N+1. Furthermore, we have

this means that the v1−viv_{1}-v_{i}’s, for i=2,…,N+1i=2,\ldots,N+1, are linearly independent.

As a consequence the unique solution of the system (6) is Vj0=0V^{0}_{j}=0 for all j=1,…,Nj=1,\ldots,N. This implies V00=1V^{0}_{0}=1 obviously.

The same kind of reasoning applied to the relation vi^=V∗wi^\widehat{v_{i}}=V^{*}\widehat{w_{i}} shows that the column coefficients V0jV^{j}_{0}, j=1,…,Nj=1,\ldots,N are also all vanishing. Finally the operator VV is of the form

for all i=1,…,di=1,\ldots,d, all j=1,…,nj=1,\ldots,n. In particular, for each fixed i=1,…,di=1,\ldots,d, we have the following subsystem of n−1n-1 equations with n−1n-1 variables A1i,…,An−1iA^{i}_{1},\ldots,A^{i}_{n-1}:

are linearly independent. Thus so are the vectors

Hence the system (8) can be solved and furnishes the coefficients AkiA^{i}_{k}, k=1,…,n−1k=1,\ldots,n-1. We have to check that these coefficients are compatible with all the equations of (8). Actually, the only equation from (7) that we have forgotten in (8) is

But this equation comes easily from the n−1n-1 first equations if we sum them after multiplication by pjp_{j}:

4 Associated 3-Tensors

Obtuse random variables are naturally associated to some 3-tensors with particular symmetries. This is what we shall prove here.

for all i,j=0,…,Ni,j=0,\ldots,N. This 33-tensor SS is given by

We also have the relation, for all i,j=0,…,Ni,j=0,\ldots,N

for all i,j=0,…,Ni,j=0,\ldots,N. In particular we have

Finally, we have, by the orthonormality of the XkX^{k}’s

by (10). This gives the last identity. □\square

This 3-tensor SS has quite some symmetries, let us detail them.

Equation (13) comes directly from Formula (10) which shows a clear symmetry in (i,j)(i,j).

But the left hand side is clearly symmetric in (i,k)(i,k) and (14) follows.

In order to prove (15), we write, using (11)

But the left hand side is clearly symmetric in (i,k)(i,k) and (15) is proved. □\square

5 Representation of Multiplication Operators

These multiplication operators carry all the probabilistic informations on XX, even through a unitary transform such as USU_{S}, for we have, by the usual functional calculus for normal operators

The operator of multiplication by Xi‾\overline{X^{i}} is given by

Proof: We have, for any fixed i∈{0,…,N}i\in\{0,\ldots,N\}, for all j=0,…,Nj=0,\ldots,N

Hence the operator US MXi US∗U_{S}\,\mathcal{M}_{X^{i}}\,U_{S}^{*} has the same action on the orthonormal basis {e0,…,eN}\{e_{0},\ldots,e_{N}\} as the operator

The last identity is just an immediate translation of the relation (11). □\square

6 Back to the Example

Let us illustrate the previous subsections with our example. To the obtuse system

These matrices are not symmetric (we shall see in Subsection 3.3 what the symmetry of the matrices SjS^{j} corresponds to). We recognize the particular form of S0S^{0}, for it corresponds to MX0=I\mathcal{M}_{X^{0}}=I.

Complex Doubly-Symmetric 3-Tensors

We are going to leave for a moment the obtuse random variables and concentrate on the symmetries we have obtained above. The relation (12) is really specific to obtuse random variables, we shall leave it for a moment. We concentrate on the relation (13), (14) and (15) which have important consequences for the 3-tensor.

Hence the λm\lambda_{m}’s are only determined up to a phase; only their modulus is determined by the representation (19).

for all mm. In terms of the vmv_{m}’s, the decomposition (19) of SS becomes

This is the form of diagonalization we shall retain for 3-tensors. Be aware that in the above representation the vectors are orthogonal, but not normalized anymore. Also note that they represent the eigenvectors of SS associated only to the non-vanishing eigenvalues of SS.

and the symmetry in (i,k)(i,k) is obvious. This gives (14).

and the symmetry in (i,k)(i,k) is obvious. This gives (15).

defines a complex doubly-symmetric 3-tensor if V\mathcal{V} is any family of (non-vanishing) orthogonal vectors.

Second step: now given a complex doubly-symmetric 3-tensor SS of the form (21), we shall prove that the set V\mathcal{V} coincides with the set

Clearly, if y∈Vy\in\mathcal{V} we have by (21)

This proves that V⊂V^\mathcal{V}\subset\widehat{\mathcal{V}}. Now, let v∈V^v\in\widehat{\mathcal{V}}. On one side we have

In particular, applying ⟨y∣∈S∗\langle y|\in\mathcal{S}^{*} to both sides, we get

and thus either vv is orthogonal to yy or v=yv=y. This proves that vv is one of the elements yy of V\mathcal{V}, for it were orthogonal to all the y∈Sy\in\mathcal{S} we would get v⊗v=S(v)=0v\otimes v=S(v)=0 and vv would be the null vector.

We have proved that V\mathcal{V} coincides with the set

are symmetric. But, as they are complex-valued matrices, this does not imply any property of diagonalization. Rather we have the following theorem ().

Let M be a complex symmetric matrix, there exist a unitary UU matrix and a diagonal matrix DD such that

Secondly, we shall need to simultaneously “factorize” the SkS_{k}’s as above. We shall make use of the following criteria (same reference).

This is the first part of Step three: proving that in our case the matrices Si‾ Sj\overline{S_{i}}\,S_{j} commute. Using the 3 symmetry properties of SS we get

This proves that Si‾ Sj Sk‾ Sl=Sk‾ Sl Si‾ Sj\overline{S_{i}}\,S_{j}\,\overline{S_{k}}\,S_{l}=\overline{S_{k}}\,S_{l}\,\overline{S_{i}}\,S_{j}. The family \big{\{}\overline{S_{i}}S_{j},i,j=1,\cdots,N\big{\}} is commuting. Thus, by Theorem 3.3, the matrices SkS_{k} can be simultaneously Takagi-factorized. There exists then a unitary matrix U=(uij)i,j=0,⋯ ,NU=(u^{ij})_{i,j=0,\cdots,N} such that, for all kk in {0,⋯ ,N}\left\{0,\cdots,N\right\},

where the matrix DkD_{k} is a diagonal matrix, Dk=diag(λk1,⋯ ,λkN)D_{k}=diag(\lambda_{k}^{1},\cdots,\lambda_{k}^{N}). Thus, the coefficient SkijS^{ij}_{k} can be written as

Our aim now is to prove that λm\lambda_{m} is proportional to am‾\overline{a_{m}}. To this end, we shall use the symmetry properties of SS. From the simultaneous reduction (23), we get

where tU{}^{t}U is the transpose matrix of UU. Thus, we have

In particular we have, for all p∈{0,…,N}p\in\{0,\ldots,N\}

But applying the symmetry (15) this is also equal to

We have obtained the orthonormal diagonalization of SS. The proof is complete. □\square

2 Back to Obtuse Random Variables

The theorem above is a general diagonalization theorem for 3-tensors. For the moment it does not take into account the relation (12). When we make it enter into the game, we see the obtuse systems appearing.

for all i,k=0,…,Ni,k=0,\ldots,N. Then the orthogonal system V\mathcal{V} such that

Proof: First assume that V={v1,…,vK}\mathcal{V}=\{v_{1},\ldots,v_{K}\}. By hypothesis, we have

for all i,j,k=0,…,Ni,j,k=0,\ldots,N. With hypothesis (12) we have in particular

This proves the first part of the theorem. The last part concerning obtuse systems is now obvious and was already noticed when we have introduced obtuse systems. □\square

In particular we have proved the following theorem.

– The random variable XX is the only random variable satisfying

3 Recovering the Real Case

In have been introduced the notions of real obtuse random variables and their associated real doubly-symmetric 3-tensors. In the same way they obtained certain symmetries on the tensor which corresponded exactly to the condition for being diagonalizable in some real orthonormal basis. Note that in the situation for the diagonalization theorem was much easier, for the symmetries associated to the 3-tensor came down to simultaneous diagonalization of commuting symmetric real matrices.

The question we want to answer here is: How do we recover the real case from the complex case? By this we mean: On what condition a complex doubly-symmetric 3-tensor correspond to a real one, that is, corresponds to real-valued random variables? Surprisingly enough, the answer is not: When the coefficients SkijS^{ij}_{k} are all real! Let us see that with a counter-example.

Let us consider the one dimensional random variable XX which takes values ii, −i-i with probability 1/21/2. As usual denote by X0X^{0} the constant random variable equal to 1 and by X1X^{1} the random variable XX. We have the relations

which give us the following matrices for the associated 3-tensor SS:

They are real-valued matrices, but they are associated to a complex (non real) random variable.

In fact, the major difference between a complex (non real) doubly-symmetric 3-tensor and a real doubly-symmetric 3-tensor is the commutation property of indices ii and kk in the coefficients SkijS^{ij}_{k}. Let us make this more precise.

Proof: The commutation relation implies that

for all i,ki,k. Then Xk‾ Xi\overline{X^{k}}\,X^{i} is almost surely real for all i,ki,k. Considering the case k=0k=0 implies that XiX^{i} is almost surely real and the result follows. □\square

In the counter-example above, one can check that S101=1S^{01}_{1}=1 and S011=−1S^{11}_{0}=-1. The commutation condition is not satisfied.

4 From Complex to Real Obtuse Random Variables

Proof: This is essentially the same argument as in Theorem 2.4, at least for the second property. For the first property one has to write that, if YY is real-valued and Y=UXY=UX then

Now recall the following classical result.

We repeat the procedure until all the coordinates are exhausted. □\square

Now, here is an independence property specific shared by the obtuse systems.

Every strict sub-family of an obtuse family is linearly free.

then, taking the scalar product with vNv_{N} we would get

whereas, taking the scalar product with vN+1v_{N+1} would give

This would imply ∥vN∥2=−1{\left\|v_{N}\right\|}^{2}=-1, which is impossible. □\square

Finally, using Proposition 3.8 we make an important step towards the main result.

Then there exist ϕ1,…,ϕN\phi_{1},\ldots,\phi_{N}, modulus 1 complex numbers, such that for every i=1,…N+1i=1,\ldots N+1 we have

Proof: First note that the ziiz^{i}_{i}’s, i=1,…,Ni=1,\ldots,N, cannot vanish, for otherwise, the family {w1,…,wN}\{w_{1},\ldots,w_{N}\} would not be linearly free, contradicting Proposition 3.9.

Secondly, the scalar product conditions ⟨w1 , wj⟩=−1\left\langle w_{1}\,,\,w_{j}\right\rangle=-1, for j=2,…,N+1j=2,\ldots,N+1, imply

In particular, all the zi1z^{1}_{i}’s, i=1,…,N+1i=1,\ldots,N+1, have the same argument.

With the conditions ⟨w2 , wj⟩=−1\left\langle w_{2}\,,\,w_{j}\right\rangle=-1, for j=3,…,N+1j=3,\ldots,N+1, we get

Hence all the zi2z^{2}_{i}’s are equal for i=3,…,n+1i=3,\ldots,n+1 and all zi2z^{2}_{i}’s have same argument (i=2,…,N+1i=2,\ldots,N+1).

One easily obtains the result in the same way, line by line. □\square

Altogether we have proved the following theorem.

5 Unitary Transforms of Obtuse Random Variables

As every complex obtuse random variable XX can be obtained as UYUY for some unitary operator UU and some real obtuse random variable YY, we shall concentrate for a while on the unitary transformations of obtuse random variables and their consequences on the associated 3-tensors, on the multiplication operators, etc.

As a first step, let us see how is transformed the associated 3-tensor under a unitary map of the random variable.

If SS and TT are the 3-tensors of XX and YY respectively, we then have

Conversely, the tensor TT can be deduced from the tensor SS by

The converse formula is obvious, replacing UU by U∗U^{*}. □\square

In the following if two 3-tensors SS and TT are connected by a formula of the form (26) we shall denote it by

Under the conditions and notations above, we have

An explicit formula for the operator US UT∗ apn UT US∗U_{S}\,U_{T^{*}}\,a^{n}_{p}\,U_{T}\,U_{S^{*}} is obtained easily by acting on the basis:

Injecting this in the previous identity, we get

That is, we get (27) and (28) immediately. □\square

The point is that this unitary operator has not been yet obtained very constructively. The following theorem gives it a little more explicitly, from the associated 3-tensor.

By Takagi Theorem 3.2, this matrix S0S_{0} can be decomposed as U D UtU\,D\,U^{t} for some unitary UU and some diagonal matrix DD. But as S0S_{0} is unitary we have

and the matrix DD is unitary too. In particular its entries are complex numbers of modulus 1. Let LL be the diagonal matrix whose entries are the square root of the entries of DD, they are also of modulus 1, so that L L‾=IL\,\overline{L}=I

We have proved the announced decomposition of S0S_{0}.

We now check the last assertion. Let vijv_{ij} be the coefficients of VV. Define the 3-tensor R=V∗∘SR=V^{*}\circ S, that is,

Injecting this relation in the expression of RkijR^{ij}_{k} above, we get

But the above expression is clearly symmetric in (i,j)(i,j), for SnpαS^{p\alpha}_{n} is symmetric in (p,α)(p,\alpha). By Proposition 3.6 this means that the 3-tensor RR is real. The theorem is proved. □\square

Complex Normal Martingales

In the next section of this article we wish to obtain two types of time-continuous results:

– a limit in distribution for the processes, for which we would like to rely on the results of where is proved that the convergence of the 3-tensors associated to the discrete time obtuse random walks implies the convergence in law of the processes;

– a limit theorem for the multiplication operators, for which we would like to rely on the approximation procedure developed in , where is constructed an approximation of the Fock space by means of spin chains and where is proved the convergence of the basic operators aji(n)a^{i}_{j}(n) to the increments of quantum noises.

When considering the complex case we had two choices: either develop a complex theory of normal martingales and structure equations, extend all the results of , of and of to the complex case and prove the limit theorems we wished to obtain; or find a way to connect the complex obtuse random walks to the real ones and rely on the results of the real case, in order to derive the corresponding one for the complex case. We have chosen the second scenario, for we have indeed the same connection between the complex obtuse random variables and the complex ones as we have obtained in the discrete time case. In this section we shall present, complex normal martingales and their structure equations, the connection between the complex and the real case, together with their consequences. Only in next section we shall apply these results in order to derive the continuous-time limit theorems.

The following theorem is proved in . It establishes the fundamental link between the 3-tensors Φ(s)\Phi(s) associated to the martingale XX and the behavior of XX.

If one denotes by Vs(ω)\mathcal{V}_{s}(\omega) the orthogonal family associated to the non-vanishing eigenvalues of Φ(s,ω)\Phi(s,\omega) and by Πs(ω)\Pi_{s}(\omega) the orthogonal projector onto Vs(ω)⊥\mathcal{V}_{s}(\omega)^{\perp}, that is, on the null-egeinvalue subspace of Φ(s,ω)\Phi(s,\omega), then the continuous part of XX is

the jumps of XX only happen at totally inaccessible times and they satisfy

The case we are concerned with is a simple case where the process Φ\Phi is actually constant. In that case, things can be made much more explicit, as is proved in again.

Conversely, any solution of (32) has the same law as XX.

The martingale XX solution of (32) possesses the chaotic representation property.

– the angle bracket ⟨Xi‾ , Xj⟩t\langle\overline{X^{i}}\,,\,X^{j}\rangle_{t} is equal to δij t\delta_{ij}\,t,

– the martingale XX has the Predictable Representation Property.

To these conditions we add the following simplifying condition:

If YY is the null process then Bsk=0B^{k}_{s}=0 almost surely, for a.a. ss and for all kk. This means that

for all tt and thus AA vanishes too. □\square

We now detail the symmetry properties of SS, TT and Λ\Lambda, together with some intertwining relations between SS and Λ\Lambda.

Proof: The proof is a rather simple adaptation of the arguments used in Proposition 2.7 and Proposition 2.8. First of all, the symmetry [Xi , Xj]t=[Xj , Xi]t[X^{i}\,,\,X^{j}]_{t}=[X^{j}\,,\,X^{i}]_{t} gives

for all tt. By the uniqueness Lemma 4.3 this gives the symmetry of the matrices Λs\Lambda_{s} and the first symmetry relation (13) for the 3-tensors S(s)S(s).

Computing [[Xi , Xj] , Xk‾]t[[X^{i}\,,\,X^{j}]\,,\,\overline{X^{k}}]_{t} we get

Again, by the uniqueness lemma, and the symmetry (13), we get the relation (36).

Now, in the same way as in the proof of Proposition 2.8, we compute [[Xi , Xj‾] , [Xk , Xl]]t[[X^{i}\,,\,\overline{X^{j}}]\,,\,[X^{k}\,,\,X^{l}]]_{t} in two ways, using the symmetry in (i,k)(i,k) of that quadruple bracket:

By uniqueness again, the time integral part gives the relation

The relation (15) is obtained exactly in the same way, from the symmetry of [[Xi , Xj‾] , [Xl‾ , Xk]]t[[X^{i}\,,\,\overline{X^{j}}]\,,\,[\overline{X^{l}}\,,\,X^{k}]]_{t} in (i,k)(i,k). We have proved that the 3-tensors S(s)S(s) are doubly-symmetric.

Computing [Xi , [Xj , Xk]]t[X^{i}\,,\,[X^{j}\,,\,X^{k}]]_{t} in two different ways we get

on the other hand. Identifying the time integrals, we get the relation (37).

Finally, computing [Xi , [Xj , Xk‾]]t[X^{i}\,,\,[X^{j}\,,\,\overline{X^{k}}]]_{t} in two different ways we get

on the other hand. Identifying the time integrals, we get the relation (38).

for some predictable processes HikH^{ik}. We write

The unicity lemma gives the relation Hsij=Λsij‾H^{ij}_{s}=\overline{\Lambda^{ij}_{s}}, almost surely, for a.a. ss.

This proves the announced unitarity. □\square

Then the matrix Λ\Lambda admits a decomposition of the form

Proof: This is exactly the same proof as for Theorem 3.14 : the decomposition of Λ\Lambda comes from Takagi’s Theorem, the expression of RkijR^{ij}_{k} in terms of the coefficients of VV and of the SkijS^{ij}_{k}’s is transformed with the help of the relation XX. One then see that RR satisfies the symmetry property which makes it real. □\square

3 Complex Unitary Transforms of Real Normal Martingales

From the result above concerning real normal martingales, we shall deduce easily the corresponding behavior of complex normal martingales, as they are obtained by unitary transforms of real normal martingales.

With the notations above, the complex martingale XX satisfies the following two “structure equations”

The process XX possesses the chaotic representation property.

Proof: The martingale YY satisfies the structure equation

But as RR is a real-valued 3-tensor, symmetric in i,j,ki,j,k, the last expression gives

Decomposing each AtjA^{j}_{t} as Btj+iCtjB^{j}_{t}+iC^{j}_{t} (real and imaginary parts), the last two relations ought to

The part (41) of the theorem is obvious, again by application of the map UU.

for some deterministic functions fi1,…,inf_{i_{1},\ldots,i_{n}}’s. But decomposing each YtjY^{j}_{t} as ∑m=1Numj‾ Xtm\sum_{m=1}^{N}\overline{u_{mj}}\,X^{m}_{t} shows clearly that FF can also be decomposed as

where the gi1,…,ing_{i_{1},\ldots,i_{n}}’s are linear combinations of the fi1,…,inf_{i_{1},\ldots,i_{n}}’s. This proves the chaotic representation property for XX and the theorem is completely proved. □\square

Continuous-Time Limit of Complex Obtuse Random Walks

We are now ready to consider the convergence theorem for complexe obtuse random walks.

We are now given a time parameter h>0h>0 which is meant to tend to 0 later on. This time parameter is the time step of the obtuse random walk we want to study, but note that hh may also appear in the internal parameters of the walk, that is, in the probabilities pip_{i} and the values viv_{i} of XX.

for all j=1,…,nj=1,\ldots,n. Putting ε0=1\varepsilon_{0}=1 and εi=1/2\varepsilon_{i}=1/2 for all i=1,…,ni=1,\ldots,n, we then have, for all i,j=0,…,Ni,j=0,\ldots,N

Proof: These are direct applications of the definitions and the symmetries verified by the Skij(h)S^{ij}_{k}(h)’s. For example:

This gives immediately that Mk0j=0M^{0j}_{k}=0. And so on for all the other cases. □\square

Proof: Let us check that (Mkij)i,j,k=1,…,N(M^{ij}_{k})_{i,j,k=1,\ldots,N} satifies the three conditions for being a doubly-symmetric 3-tensor. Recall that for these indices, we have

The first condition Mkij=MikjM^{ij}_{k}=M^{kj}_{i} is obvious from the same property of Skij(h)S^{ij}_{k}(h) and passing to the limit.

We wish now to prove that ∑m=1NMjim Mmkl\sum_{m=1}^{N}M^{im}_{j}\,{M^{kl}_{m}} is symmetric in (i,k)(i,k). The corresponding property for S(h)S(h) gives

In particular, multiplying by hh, we get

By hypothesis lim⁡h→0S0kl(h)\lim_{h\rightarrow 0}S^{kl}_{0}(h) and lim⁡h→0S0il(h)\lim_{h\rightarrow 0}S^{il}_{0}(h) exist hence, passing to the limit, we get

which is the second symmetry asked to MM for being doubly-symmetric.

The third symmetry is obtained in a similar way. Indeed, we have

Now, passing to the limit as hh tends to 0, we get

This gives the last required symmetry. □\square

2 Convergence in Distribution

We can now give our convergence in distribution theorem.

Applying the unitary operators UhnkiU_{h_{n_{k_{i}}}}, which converge to VV, we have the convergence in law of the process ZhnkiZ^{h_{n_{k_{i}}}} to the process Z=VYZ=VY. By Theorem 4.6 the process ZZ is solution of the complex structure equations associated to the tensor SS.

3 Convergence of the Multiplication Operators

Let us first recall very shortly the main elements of the construction and approximation developed in , which will now serve us in order to prove the convergence of the multiplication operators. This convergence of multiplication operators is not so usual in a probabilistic framework, but it is the one interesting in the framework of applications in Quantum Statistical Mechanics, for it shows the convergence of the quantum dynamics of repeated interactions towards a classical Langevin equation, when the unitary interaction is unitary (cf ).

When dealing with the associated random walk with time step hh

the canonical space is naturally isomorphic to

via a unitary isomorphism denoted by UAU_{A}. This space is the natural space for the quantum noises aji(t)a^{i}_{j}(t), made of the time operator a00(t)=tIa^{0}_{0}(t)=tI, the creation noises ai0(t)a^{0}_{i}(t), the annihilation noises a0i(t)a^{i}_{0}(t) and the exchange processes aji(t)a^{i}_{j}(t), with i,j=1,…Ni,j=1,\ldots N (cf ).

The main constructions and results developed in are the following:

– each of the spaces TΦ(h)T\Phi(h) can be naturally seen as concrete subspace of Φ\Phi;

– when hh tends to 0 the subspace TΦ(h)T\Phi(h) fills in the whole space Φ\Phi, that is, concretely, the orthogonal projector PhP_{h} onto TΦ(h)T\Phi(h) converges strongly to the identity II;

– the basic operators aji(nh)a^{i}_{j}(nh), now concretely acting on Φ\Phi, converge to the quantum noises, that is, more concretely the operator

converges strongly to aji(t)a^{i}_{j}(t) on a certain domain D\mathcal{D} (which we shall not make explicit here, please cf ), where

if one extends the coefficients NkijN^{ij}_{k} to the 0 index, by putting N0ij=δijN^{ij}_{0}=\delta_{ij}.

Once this is recalled, the rest is now rather easy. We can prove the convergence theorem for the multiplication operators.

The operators of multiplication MZth\mathcal{M}_{Z^{h}_{t}}, acting of Φ\Phi, converge strongly on D\mathcal{D} to the operators

These operators are the operators of multiplication by ZZ the complex martingale satisfying

Proof: The convergence toward the operator Zt\mathcal{Z}_{t} given by (44) is a simple application of the convergence theorems of , let us detail the different cases.

If j,k≠0j,k\not=0, we know that h Skij\sqrt{h}\,S^{ij}_{k} converges to MkijM^{ij}_{k} and by we have that ∑m=1[t/h]akj(m)\sum_{m=1}^{\left[t/h\right]}a^{j}_{k}(m) converges to akj(t)a^{j}_{k}(t).

If j=0j=0 and k≠0k\not=0, we know that S0ijS^{ij}_{0} converges to M0ijM^{ij}_{0} and that ∑m=1[t/h]h a0j(m)\sum_{m=1}^{\left[t/h\right]}\sqrt{h}\,a^{j}_{0}(m) converges to a0j(t)a^{j}_{0}(t).

If k=0k=0 and j≠0j\not=0, we know that Ski0S^{i0}_{k} converges to Mki0M^{i0}_{k} (actually their are all equal to δik\delta_{ik}) and that ∑m=1[t/h]h ak0(m)\sum_{m=1}^{\left[t/h\right]}\sqrt{h}\,a^{0}_{k}(m) converges to ak0(t)a^{0}_{k}(t).

The fact that Zt\mathcal{Z}_{t} is indeed the multiplication operator by the announced normal martingale comes as follows. The martingale ZZ is the image UAUA, under a unitary operator UU of some real normal martingale AA. The 3-tensor MM is the image U∘NU\circ N, under the unitary operator UU, of some real tensor NN. The real normal martingale AA associated to the real 3-tensor NN has its multiplication operator equal to

by Theorem 5.4. As ZtZ_{t} is equal to UAtUA_{t} its canonical space is the same as the one of AA, only the canonical isomorphism is modified by a change of basis. The rest of the proof is then exactly similar to the one of Proposition 3.13. □\square

Examples

We shall detail 2 examples in dimension 2, showing up typical different behaviors.

with probabilities p1=1/3p_{1}=1/3, p2=1/4p_{2}=1/4 and p3=5/12p_{3}=5/{12} respectively. Then the 3-tensor SS associated to XX is given by

It is then rather easy to find a unitary matrix VV such that V Vt=M0V\,V^{t}=M_{0}, we find

for example. Following our results on complex normal martingales, this means that the process ZZ has the following distribution: given a 2-dimensional real Brownian motion W=(W1 , W2)W=(W^{1}\,,\,W^{2}) then

with probabilities p1=1/2p_{1}=1/2, p2=h/(1+2h)p_{2}=h/(1+2h) and p3=1/(2+4h)p_{3}=1/(2+4h) respectively. Then the 3-tensor SS associated to XX is given by the following, where we have only detailed the leading orders in hh

The renormalized 3-tensor converges to the 3-tensor

In order to diagonalize the 3-tensor, we solve

This means that the continuous-time limit process ZZ is a compensated Poisson process in the direction vv.

This is all for the information which is given by the 3-tensor. If we want to know the direction where the process is Brownian, we need to look at the decomposition of M0M^{0} as V VtV\,V^{t} for a unitary VV. We easily find

The process ZZ is finally described as follows, let NN and WW be a standard Poisson process and a Brownian motion, respectively, independant of each other. Then

References