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Random Matrices, Integrals and Space- time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information Theory, Dec 15-18, 2003

Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

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Page 1: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Random Matrices, Integrals and Space-

time Systems

Babak HassibiCalifornia Institute of TechnologyDIMACS Workshop on Algebraic Coding and Information

Theory, Dec 15-18, 2003

Page 2: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Outline

• Overview of multi-antenna systems• Random matrices• Rotational-invariance• Eigendistributions• Orthogonal polynomials• Some important integrals• Applications• Open problems

Page 3: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Introduction

We will be interested in multi-antenna systems of the form:

,VSHM

X

where NTNMMTNT VHSX CCCC ,,, are the receive, transmit, channel, and noise matrices, respectively.Moreover, are the number of transmit/receive antennasrespectively, is the coherence interval and is the SNR.

The entries of are iid and the entries of are also , but they may be correlated.

NM ,T

V )1,0(CN H)1,0(CN

Page 4: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Some Questions

• What is the capacity?• What are the capacity-achieving input distributions?• For specific input distributions, what is the mutual

information and/or cut-off rates?• What are the (pairwise) probability of errors?

We will be interested in two cases. The coherent case, where is known to the receiver and the non-coherent case, where is unknown to the receiver.

The following questions are natural to ask.

HH

Page 5: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Random Matrices

A random matrix is simply described by the joint pdf of its entries,

An example is the family of Gaussian random matrices, where the entries are jointly Gaussian.

nm A

),...,1;,...,1;()( njmiapAp ij

Page 6: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Rotational-InvarianceAn important class of random matrices are (left- and right-) rotationally-invariant ones, with the property that their pdf is invariant to (pre- and post-) multiplication by any and unitary matrices and .

mmnn

),()( ApAp and

mI **

),()( ApAp nI **

If a random matrix is both right- and left- rotationally-invariantwe will simply call it isotropically-random (i.r.).If is a random matrix with iid Gaussian entries, then it is i.r.,as are all of the matrices:G

*11

*1

12

*21

12121

1** ,)(,,,,,, AGGGGGGGGGGGGGGGG p

Page 7: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Isotropically-Random Unitary Matrices

A random unitary matrix is one for which the pdf is given by

).()()( *mIfp

When the unitary matrix is i.r., then it is not hard to show that

).()1()...(

)( *2/)1( mmm

Im

p

Therefore an i.r. unitary matrix has a uniform distribution overthe Stiefel manifold (space of unitary matrices). It is also calledthe Haar measure.

Page 8: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

A Fourier Representation

If we denote the columns of by then ,,..,1, mkk

))(Im())(Re()( ***kllkkllk

lkmI

Using the Fourier representation of the delta function

xjedx

2

1)(

It follows that we can write

*

* )(

2/)13(*

2

)1()...()( mIjtr

mmmm edm

I

Page 9: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

A Few TheoremsI.r. unitary matrices come up in many applications.

Theorem 1 Let be an i.r. random matrix and consider the svd Then the following two equivalent statements hold:1. are independent random matrices and and are i.r. unitary.2. The pdf of only depends on

Idea of Proof: and have the same distribution forany unitary and

A nm.*VUA

VU ,, U V

A :).()( fAp

*A A ......

Page 10: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Theorem 2 Let A be an i.r. Hermitian matrix and consider theeigendecomposition . Then the following two equivalent statements are true.1. are independent random matrices and is i.r. unitary.2. The pdf of A is independent of U:

Theorem 3 Let A be a left rotationally-invariant random matrixand consider the QR decomposition, A=QR. Then the matricesQ and R are independent and Q is i.r. unitary.

*UUA

,U U

).()( fAp

Page 11: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Some JacobiansThe decompositions and can be consideredas coordinate transformations. Their corresponding Jacobianscan be computed to be:

and

for some constant c.

Note that both Jacobians are independent of U and Q.

*UUA QRA

)()(!

1 *2mlk

lk

IUUm

dUddA

)( *

1m

kmkk

m

k

IQQrdQdRcdA

Page 12: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

EigendistributionsThus for an i.r. Hermitian A with pdf we have),(Ap

).()(!

1)(),( *2

mlk

lkA IUUm

pUp

Integrating out the eigenvectors yields:

Theorem 4 Let A be an i.r. Hermitian matrix with pdf Then

Note that , a Vandermonde determinant.

).(Ap

lk

lkA

mm

pm

p 2)1(

)()()1()...1(

)(

lk

lk V )(det)( 22

Page 13: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Some Examples

• Wishart matrices, , where G is

• Ratio of Wishart matrices,

• I.r. unitary matrix. Eigenvalues are on the unit circle and the distribution of the phases are:

GGA * ., nmnm

).(det)( 22

1

1

Vecpk

n

k

nmk

:121 AAA

).(det)1

1()( 22

1

Vcp n

k

n

k

.)(sin),...,( 21

lk

lkm cp

Page 14: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

The Marginal Distribution

Note that all the previous eigendistributions were of the form:

For such pdf’s the marginal can be computed using an eleganttrick due to Wigner.

Define the Hankel matrix

Note that Assume that Then we can perform theCholesky decomposition F=LL*, with L lower triangular.

m

kk Vfcp

1

2 ).(det)()(

.1

1

)( 1

1

m

m

fdF

.0F .0F

Page 15: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Note that implies that the polynomials

are orthonormal wrt to the weighting function f(.):

Now the marginal distribution of one eigenvalue is given by

But

mIFLL *1

1

1

1

0 1

)(

)(

mm

L

g

g

.)()()( kllk ggfd

)(det)()( 2

121

Vfddcpm

kkm

21

1212

))((det)(det

VLfdd

L

c m

kkm

)(

)()(

)()(11

)(

111

010

111

11

G

mmm

m

mm

m

V

gg

gg

LVL

Page 16: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Now upon expanding out and integrating over the variables the only terms that do not vanish are those for which the indices of the orthonormal polynomials coincide.

Thus, after the smoke clears

In fact, we have the following result.

Theorem 5 Let A be an i.r. Hermitian matrix with Then the marginal distribution of the eigenvalues of A is

)(det 2 GV

m 2

1

0

2 ).()()(m

kkgfcp

).()( kA fAp

1

0

2 ).()(1

)(m

kkgf

mp

Page 17: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Orthogonal Polynomials

• What was just described was the connection between random matrices and orthogonal polynomials.

• For Wishart matrices, Laguerre polynomials arise. For ratios of Wishart matrices it is Jacobi polynomials, and for i.r. unitary matrices it is the complex exponential functions (orthogonal on the unit circle).

• Theorem 5 gives a Christoffel-Darboux sum and so

• The above sum gives a uniform way to obtain the asymptotic distribution of the marginal pdf and to obtain results such as Wigner’s semi-circle law.

))()()()(()(

)( '11

'1 mmmmm

m gggga

a

m

fp

Page 18: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Remark

The attentive audience will have discerned that my choice ofthe Cholesky factorization of F and the resulting orthogonal polynomials was rather arbitrary.

It is possible to find the marginal distribution without resortingto orthogonal polynomials. The result is given below.

1

11

1

1)(1

)(m

m Ffm

p

Page 19: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Coherent ChannelsLet us now return to the multi-antenna model

where we will assume that the channel H is known. We will assume that where are the correlation matrices at the transmitter and receiver and G has iid CN(0,1)entries. Note that can be assumed diagonal wlog.

According to Foschini&Telatar:

1. When

,VSHM

X

rtGDDH rt DD ,

rt DD ,

:, NrMt IDID

))(1log()det(log*

*

M

GGEGG

MIEC N

Page 20: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

2. When

3. When

4. In the general case:

Cases 1-3 are readily dealt with using the techniques developed so far, since the matrices are rotationally-invariant.

Therefore we will do something more interesting and compute the characteristic function (not just the mean). This requires more machinery, as does Case 4, which we now develop.

:Mt ID

))(1log()det(log*2

*2

M

GGDEGGD

MIEC r

rM

:Nr ID

))(1log(max)det(logmax*

)(

*

)( M

GPDDGGPDDG

MIEC tt

MPtrttN

MPtr

))(1log(max*

)( M

GDPDDGDEC rttr

MPtr

Page 21: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

A Useful Integral FormulaUsing a generalization of the technique used to prove Theorem

5, we can show the following result.

Theorem 6 Let functions begiven and define the matrices

Then

where

1,,0),(),(),( mkhgf kk

)()(

)()(

)(,

)()(

)()(

)(

111

010

111

010

mmm

m

H

mmm

m

G

hh

hh

V

gg

gg

V

FmVVfd H

m

kGk det!)(det)(det)(

1

.)()(

)(

)(

)( 10

1

0

m

m

hh

g

g

fdF

Page 22: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Theorem 6 was apparently first shown by Andreief in 1883.

A useful generalization has been noted in Chiani, Win and Zanella (2003).

Theorem 7 Let functionsbe given. Then

where for the tensor we have defined

and the sums are over all possible permutations of the integers 1 to m.

1,,0),(),(),( mkhgf kkk

))()()(()(det)(det)(1

kjiH

m

kGkk hgfTensorVVfd

ijkA

m

kkkk

AATensor1

)sgn()sgn()(

,

Page 23: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

An Exponential IntegralTheorem 8 (Itzyskon and Zuber, 1990) Let A and B be m-dimensional diagonal matrices. Then

where

Idea of Proof: Use induction. Start by partitioning

)(det)(det

),(det)1()1()( **

BVAV

BAEmIed m

BAtr

mmm

m

baba

baba

ee

ee

BAE

1

111

),(

ma

AA 1

1 ,

Page 24: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Then rewrite so that thedesired integral becomes

trBaBIaAtrBAtr mmm ))(()( *1111

*

)()( 11

*11

* *1

'1

*

mBAtrtrBa

mBAtr IedeIed m

)(1

11*1

*1

'1 mm IjtrBAtrtrBa eddce

m

kk

jtrtrBa

jAb

edce m

1

' )det(

m

kmk

WjtrAtrBa

jWIb

edWce m

11 )det(

'

)()(det)(

1*2

1

1

1

*'

mm

klk

m

l

UUjtrAtrBa IUUV

jb

edUdce m

Page 25: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

The last integral is over an (m-1)-dimensional i.r. matrix.And so if use the integral formula (at the lower dimension)to do the integral over U, we get

An application of Theorem 6 now gives the result.

)(det),(det)(

1

)(det'

1

1

1'

VAEjb

dAV

ec

m

klk

m

l

trBam

Page 26: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Characteristic FunctionConsider

The characteristic function is (assuming M=N)

Successive use of Theorems 6 and 8 give the result.

)det(log)det(log ** DGGM

IEGDGM

IEC NM

j

N

DGGM

IjDGG

MIEEe

N

)det( *)det(log *

trWjN eDW

MIdWc

)det(

1

)det()(det

trWDjNm

eWM

IdWD

c

)()(det)1()(det

*2

1

1*

MDUtrU

M

kkm

IUUVeM

dUdD

c

Page 27: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Non-coherent Channels

Let us now consider the non-coherent channel.

where H is unknown and has iid CN(0,1) entries.

Theorem 9 (Hochwald and Marzetta, 1998) The capacity-achieving distribution is given by S = UD, where U is T-by-Mi.r. unitary and D is an independent diagonal.

Idea of Proof: Write S=UDV*. V* can be absorbed in H and so Is not needed. Optimal S is left rotationally-invariant.

,VSHM

X

Page 28: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Mutual InformationDetermining the optimal distribution on D is an open problem.However, given D, one can compute all quantities of interest.The starting point is

The expectation over U is now readily do-able to give p(X|D). (A little tricky since U is not square, but doable using FourierRepresentation of delta functions and Theorems 6 and 8.)

)(det),|(

*2

)( 1*2*

UUDM

I

eDUXp

TNTN

XUUDM

ItrX T

)(det 2

)( *12**

DM

I

e

MNTN

XUDM

IUtrXXtrX M

Page 29: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Other Problems

• Mutual information for almost any input distribution on D can be computed.

• Cut-off rates for coherent and non-coherent channels for many input distributions (Gaussian, i.r. unitary, etc.) can be computed.

• Characteristic function for coherent channel capacity in general case can be computed.

• Sum rate capacity of MIMO broadcast channel in some special cases can be computed.

• Diversity of distributed space-time coding in wireless networks can be determined.

Page 30: Random Matrices, Integrals and Space-time Systems Babak Hassibi California Institute of Technology DIMACS Workshop on Algebraic Coding and Information

Other Work and Open Problems

• I did not touch at all upon asymptotic analysis using the Stieltjes transform.

• Open problem include determining the optimal input distribution for the non-coherent channel and finding the optimal power allocation for coherent channels when there is correlation among the transmit antennas.