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Theory of random multiplicative transfer matrices and its implications for quantum transport

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HAL Id: jpa-00212392

https://hal.archives-ouvertes.fr/jpa-00212392

Submitted on 1 Jan 1990

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its implications for quantum transport

J.-L. Pichard, N. Zanon, Y. Imry, A. Douglas Stone

To cite this version:

(2)

Theory

of

random

multiplicative

transfer matrices

and

its

impli-cations for

quantum transport

J.-L.

Pichard(1),

N.

Zanon(1),

Y.

Imry(2,3 )

and A.

Douglas

Stone(4)

(1)Service

de

Physique

du Solide et de Résonance

Magnétique,

CEA

Saclay,

91191 Gif-sur-Yvette

Cedex,

France

(2)Department

of Nuclear

Physics,

Weizmann Institute of

Science,

Rehovot

76100,

Israel

(3)I.B.M.

Thomas J. Watson Research Center Yorktown

Heigths,

NY

10598,

U.S.A.

(4)Applied

Physics,

Yale

University,

New

Haven,

CT

06520,

U.S.A.

(Requ

le

27 septembre

1989,

accepté

le 8 décembre

1989)

Résumé. 2014 En

régime quantique

cohérent,

la conductance g d’un

système

désordonné

possèdant

N canaux de diffusion est déterminée par N

paramètres

réels

("niveaux") {03BBi}

qui

caractérisent sa

ma-trice de transfert M. La mesure

adéquate

pour

M,

combinée avec une

hypothèse d’entropie

maximum

"globale",

conduit à une loi de distribution de ces niveaux

identique à

celle des ensembles de matrices aléatoires

classiques,

si l’on excepte la

présence

d’un comportement nouveau de la densité de niveaux

03C1(03BB),

qui

est loin d’être

uniforme,

et

dépend

de

façon

significative

des

paramètres

du

système.

Nous étudions en détail cette densité et ses

implications

pour les fluctuations de conductance, montrant

que le comportement

spécifique

de cet ensemble résulte de la loi de

composition

multiplicative

de M.

Pour N donné et

quand

la

longueur

Lz du

système

augmente, ce sont les 03B1i ~

(1/2Lz)~n(03BBi)

(qui

convergent vers les

exposants

de

Lyapunov

de

M)

qui

ont une densité essentiellement uniforme.

Uti-lisant cette

densité,

nous

développons

une

analogie

coulombienne pour

expliquer

le

changement

des

statistiques

des niveaux et de la conductance

qui

accompagne la transition du

régime métallique

au

régime

isolant. Le

régime

métallique correspond à

une

"phase"

de haute densité du gaz de

coulomb,

avec une

statistique identique

à celle des ensembles

classiques

avec interactions

logarithmiques,

si l’on excepte la

présence

d’une "interaction" avec des

charges

images près

de

l’origine;

ceci

implique

une loi normale pour

p(g)

avec une variance universelle. Des mécanismes

possibles

d’apparition

de

queues

lognormales

dans le

régime métallique

sont discutés. Le

régime

localisé

correspond à

une

"phase"

de faible densité où les niveaux fluctuent de

façon

quasi-indépendante

et où la conductance

est distribuée de

façon

lognormale

avec

~(03B4~n g)2~ ~

2/g0,

go =

N~/Lz

étant la conductance

ohmique

classique

et ~ le libre parcours moyen

élastique.

Les

conséquences

de cette

analogie

coulombienne

pour la distribution des fluctuations de niveaux et de conductance sont confirmées par des calculs

numériques indépendants.

La distribution

p(g)

n’étant fonction que de

03C1(03BB)

dans notre théorie, nous

étudions dans la seconde

partie

de ce travail les

propriétés

d’échelle de

03C1(03BB)

afin d’examiner la

vali-dité d’une théorie d’échelle à un

paramètre.

D’abord, nous

généralisons

pour chacun des niveaux 03B1i

les lois d’échelle

déjà

obtenues pour la chaine désordonnée. Puis nous montrons que la convergence

de chacun des 03B1i vers sa limite

quasi-unidimensionnelle (N

donné,

Lz ~

oo)

ne

dépend

que de

la conductance moyenne

~g~.

Nous en concluons que

(g)

satisfait à une loi d’échelle à un

paramètre

dans le domaine de

paramètres

examiné.

Cependant,

nous ne pouvons exclure que la

dépendance

en

fonction de i des lois d’échelle obtenues n’introduise des

paramètres

d’échelle

supplémentaires

pour

03C1(g).

Classification

Physics

Abstracts

71.30 - 71.55J - 72.10 - 72.15R

(3)

Abstract. 2014 The

two-probe

conductance, g,

of a disordered quantum system with N tranverse

scat-tering

channels is determined

by

N real

parameters

("levels") {03BBi}

characterizing

the transfer matrix M. The

appropriate

measure for M combined with a

"global"

maximum entropy

hypothesis,

leads to a

joint

distribution for these levels of the same form as the standard random matrix ensembles, except for the occurence of a novel behavior of the level

density

03C1(03BB),

which is far from

uniform,

and

depends

importantly

on the system parameters. We

study

this

density

and its

implications

for conductance fluctuations in

detail,

showing

that the novel behavior of this ensemble stems from the

multiplicative

composition

law for M. For fixed

N,

as the system

length

Lz ~ oo it is the 03B1i ~

(1/2Lz) ~n

03BBi

(which

converge to the

Lyapunov

exponents of

M)

that have an

approximately

uniform

density.

Us-ing

this

density

we

develop

a Coulomb gas

analogy

to understand

analytically

the

change

in the level

and conductance statistics which

accompanies

the transition from metallic to localized behavior. The metallic

regime corresponds

to the

high-density "phase"

of the gas, with statistics similar to

stan-dard,

logarithmically-correlated

ensembles except for the appearance of an "interaction" with

image

charges

near the

origin;

this leads to a normal distribution

p(g)

with a universal variance. Possible mechanisms for the occurrence of

lognormal

tails in the metallic

regime

are discussed. The local-ized

regime

corresponds

to a

low-density

"phase"

in which the levels fluctuate

independently

and the conductance is

lognormally

distributed with

~(03B4~n g)2~ ~

2/g0

where g0 =

N ~/Lz

is the classical

con-ductance and ~ is the elastic man free

path.

The consequences of the Coulomb gas

analogy

for both the conductance and level statistics are confirmed

by

independent

numerical calculations. In our

the-ory, the distribution

p(g)

depending

only

on

p(A),

we

study

in a second

part

of this work the finite-size

scaling

properties

of

03C1(03BB)

to address the

question

of

one-parameter

scaling.

First we

generalize

for each level 03B1i the

scaling

law obtained for the disordered chain. Then we show that the convergence of each 03B1i towards their

quasi-one

dimensional limit

(N

fixed, Lz ~

oo)

depends only

on the average

conductance

(g)

in the range of

investigated

parameters.

However,

we cannot rule out a

dependence

on the index i of the

scaling

functions which would introduce additional

scaling

parameters for

p(g).

Introduction

It has been known

for

some time that a

study

of the

eigenvalues

of the matrix

Mt M

(where

M is the transfer

matrix),

as the

system

length

Lz

--; oo,

gives

useful information

concerning

the

localization

length

and

scaling properties

of the conductance

g(Lz )

in disordered

systems

[1- S].

More

recently,

it has been understood that since the

two-probe

conductance and the transfer

ma-trix are

simply-related

for

systems

of any size

[6],

such an

approach

is also very natural and useful

in

studying

the statistical fluctuations

of g

in the metallic

regime

[7],

where the behavior

of g

can

be very different from the

Lz

--· oo

(localized)

limit. Such statistical fluctuations have now been

widely

observed and studied in

experimental

systems,

typically

small

("mesoscopic")

disordered microstructures

[8].

A

striking

result of these

experiments

is that the variance of the conductance

is

always

of order

unity (in

units of

e2/h),

independent

of the average

conductance,

when the

conductor is

phase-coherent,

i.e. measured on a scale smaller or

equal

to the inelastic

scattering

length.

The transfer matrix

approach,

when combined with a maximum

entropy

hypothesis (as

discussed

below)

and certain

concepts

from the

theory

of the standard random matrix ensembles

[7, 9,11],

provides

what is

probably

the

simplest general explanation

for these "universal

conduc-tance fluctuations"

[12].

At the same

time,

the

discovery

of observable conductance fluctuations has

reopened

the

question

of the

validity

of the

scaling theory

of

quantum

conductance

[13],

as

applied

to the whole

probability

distribution of g,

p(g) [14 - 16].

In this work we extend the

"global

maximum

entropy

approach"

introduced earlier

[9 - 10]

to address the

origin

of universal conductance fluctuations. In

particular

we

exploit

a Coulomb gas

analogy

which arises

naturally

in this

approach

to understand the

large change

in the statistical behavior of the conductance which

accompanies

the transition between the metallic and localized

(4)

fact that it is determined

by

the

eigenvalues

of an ensemble of

multiplicative

random matrices whose combination law determines a definite evolution of the

eigenvalue density

with the

length

of the

system

(number

of factors in the

product).

In contrast to our earlier work

[9 - 10],

which

emphasized

that this ensemble exhibits statistical behavior in the metallic

regime

characteristic of the standard random matrix ensembles

(e.g.

the Gaussian

orthogonal ensemble),

here we also

emphasize

that these ensembles have novel and different

properties

because its members are

ran-dom matrix

products,

and must be characterized

by

a certain

density

of

self-averaging

lyapunov

exponents

as

Lz

- oo, In the Coulomb gas

analogy

we show that the metallic and localized

regimes

correspond respectively

to

high density (strongly-correlated),

and low

density

(weakly-correlated) phases

of the gas; and the former

phase

leads to normal fluctuations

in g,

whereas the

latter leads to

lognormal

fluctuations. We thus arrive at a unified

picture

of the statistical behavior of

quantum

conductors of fixed width as the

length

is varied. We test many of the

implications

of this

picture

by

numerical simulations. In addition we

study

in detail the

scaling

properties

of the

eigenvalues

of

M~M

both as a function of width and

length

in order to address the

question

of

one-parameter

scaling.

We consider here electronic

quantum transport

through

disordered

systems,

invariant under time reversal

symmetry

(no applied magnetic field),

with

spin-independent hopping (no spin-orbit

coupling).

We consider the

simplest measuring

geometry

in which the current is

supplied

to a

finite disordered

region

of

length

kz

and width

Lt

by

two semi-infinite ordered leads and the

driving

voltage

is measured between two electron reservoirs

feeding

the

sample

via the leads. This

corresponds

to a

two-probe

measurement in which the

voltage

difference is measured between the

current source and sink

[17].

It now seems

likely

that a

complete

theory

of

mesoscopic

conduction

will have to take into account the nature of the actual

measuring

geometry,

which often involves distinct current and

voltage probes

[18 -19].

For the

general

statistical

questions

addressed here

however,

it should be sufficient to consider

only

the

two-probe

case. In this case, the

system

is characterized

by

N

propagating

momentum channels in the leads and

M(Lz)

denotes the 2N x

2N

multiplicative

transfer matrix

giving

the flux

amplitudes

to the

right

of the disordered

region

(henceforth

referred to as the

sample)

in terms of the

incoming

and

outgoing

amplitudes

on the

left of the

sample.

For

example,

linear

response

theory

[20]

for this

system,

with the

assumption

of a uniform electric

field,

yields

a

many-channel

Landauer formula

[21]

which states that the conductance

g(Lx ),

measured in unit of

2e2/h

(where

the factor 2 comes from

including

spin

degeneracy),

is

equal

to the total

probability

for electrons at the Fermi surface to be transmitted

through

the

sample.

Thus g

for a

given

realization of the disordered

potential

can be

expressed

exactly

as the sum of all the interchannel transmission coefficents

Tij;

or

equivalently, simply

using

the definitions of the

scattering

matrix S and of

M,

and

taking

into account the

symmetry

of M

(current

conservation and

time-reversal),

in terms of the N

eigenvalues

mi (L z)

of the hermitean matrix

Mt (Lz ).M(Lz ).

One finds for

g(Lz )

A derivation of the fundamental relation

(1)

can be found in references

[6,7].

The

advantage

of

studying

the formulation in terms of the transfer matrix is that in

general

one can divide the full

sample

into a series of shorter disordered slices such that M is

given

as the

product

of random transfer matrices which describes each

slice,

whereas a much more

complex

composition

rule holds for the transmission matrix or for the

scattering

matrix.

For the usual Anderson

tight-binding

model with

diagonal

disorder that we have

employed

(5)

different

slices,

which can be obtained

simply

by rearranging

the

time-independent Schradinger

equation

for the

sample.

The

degree

of disorder is measured

by

the

parameter W

which is the width of the

rectangular

distribution taken for the

diagonal

elements of the Hamiltonian. For

simplicity

we

study

two-dimensional

samples (each

slice is

just

a

row)

for an energy E = 0

(band

center)

where

(with rigid

transverse

boundary

conditions)

the number of

propagating

channels N in the leads is

just equal

to the transverse width

Lt.

Taking

Lt

fixed and

Lz

varying (quasi

one-dimensional

geometry),

Oseledec’s theorem

[1]

for random

multiplicative

matrices tells us that the N

a; ( Lz )

self-average

in the

large

Lx -limit

to N "inverse localization

lengths"

0152i(oo).

Thus,

the inverse localization

lengths

characterizing

the

Lt

parallel

channels of the disordered

sample

in the

large

Lz -limit

do not

depend

on the

particular

realization of the random

potential.

If one could

simply

substitute into

(1)

the

self-averaged

ai (oo)

for the random

sample-dependent quantities

o;,(L~),

one would find that

g(Lx )

just

measures the number

Neff

of active transmission channels

[7]

of the disordered

sample

for which

a¡( 00 ).Lz

1.

The

approximate validity

of such a substitution is not obvious : one

might

think that there would be substantial

sample

to

sample

fluctuations in the

ai(L,)

in the metallic

regime

(l

Lz

~,

where is the elastic mean free

path

and ~

the localization

length

of the disordered

sam-ple,

defined as the inverse of the smallest

positive

0152i ( 00 ))

and that this substitution would make

sense

only

for

Lz

> ~ .

Fortunately,

numerical studies show that this substitution is

approximately

correct, and the

approaches

based on random matrix

theory

justify

in more

depth

the observed smallness of the fluctuations of the

a¡(Lz)

in the metallic

regime

by

introducing

the fundamental

concept

of

spectral rigidity

[7, 9 -11],

which is

intimately

related to the

universality

of the

con-ductance fluctuations.

Figure

1 shows the ai

(Lz )

of a

randomly-chosen sample, arranged

in order of

increasing

mag-nitude,

and the

ensemble-averaged

spectrum.

The difference is

small,

as is the difference between

this

averaged

spectrum

of

a¡(Lz)

and the

self-averaged

limiting

spectrum

of inverse localization

lengths

as

(cxJ) .

We shall

study

in detail these small differences

below;

however we wish to make

the

preliminary

observation that the data shown in

figure

1

justify

the

concept

introduced in reference

[7]

of an effective number

Ne$

of channels which control the metallic conductance

(as

long

as it is understood that these "channels" are associated to the

eigenvalues

of

MtM,

and not to the initial momentum channels of the leads whose the correlations have been

recently

studied in Refs.

[22, 23] ).

Since the

0152i(Lz)

are

sample-dependent,

we

analyze

in

section

1 their

statistics,

for the first

Neff

open transmission channels

(metallic regime,

ai (Lz). Lz

«

1),

for the N -

Neff

closed

trans-mission channels

(a¡(Lz).Lz

»

1),

and for those at the interface between those two sets

(which

are crucial for the conductance

fluctuations).

The

analysis

is based on the

global

maximum

entropy

ansatz

proposed

in reference

[9],

which has been

recently proved

[24]

to be consistent with the lo-cal maximum

entropy

approach developed

in reference

[11],

and which

yields

a certain

prob4bility

distribution for the

0152i ( L z ).

This distribution leads us to introduce different formal

analogies

with ensembles of classical

negative

charges,

free to move on a

line,

and

interacting

between themselves and with a

positive "jellium",

at a

given

temperature.

Comparisons

with the results of numerical studies of the Anderson model are

presented.

In section

2,

the

implications

of the level statistics for the conductance fluctuations are consi-dered. For metallic

quantum

conductors

( N~,

»

1),

the bulk of

p(g)

is found Gaussian with a uni-versal variance

(universal

conductance

fluctuations),

while

possible

mechanisms for

having

non-universal and

non-gaussian

tails are

suggested

[14].

For

quantum

insulators

(ai(Lz ).Lz

»

1,

V

i),

a

lognormal

distribution is obtained. The

importance

of the

averaged

spectral density

for this maximum

entropy

approach

is underlined : a one

parameter

spectral density

of

Mt (Lz ).M(Lz )

yields

a one

parameter

distribution for

g(Lz).

(6)

Fig.

1. -

az (Lz, Lt)

as a function of the index

i, arranged

in order of

increasing

magnitude

for Lt = 25

and W = 2. The crosses

give

ai(Lz =

25, Lt =

25)

for a

given

25x25 disordered square, while the diamonds

(o)

are obtained after ensemble

averaging.

The squares

(D)

are the inverse localization

lengths

(aa (Lz

= oo, Lt =

25)).

increases for a fixed value of

Lt

(quasi-one-dimensional

geometry)

is

analyzed.

We

generalize

the

scaling theory

of the Id-chain

[4, 24]

to the many channel case. In

addition,

our numerical data agree

reasonably

with the

assumption

that,

for each

channel,

this convergence is

only

controlled

by

the average conductance

(g) .

This

yields

the existence of

one-parameter

scaling

for

(g),

in the

range of

investigated

parameters.

In section

4,

we

numerically

study

the convergence of the

ai (L)

towards their limits for

squares of

increasing

size L

(L

=

Lz

=

Lt,

two dimensional

geometry).

We sketch

briefly

how the

scaling

works,

without

having

a limit

given by

Oseledec’s theorem on

large

random matrix

prod-ucts. Sections 3 and 4 show how

large insulating samples

and their small metallic elements are

simply

related,

using

scaling

relations which are

obeyed by

the cei. For a

given

channel i,

the

scaling

relation involves

only

a

single

parameter,

but we do not know for the moment if the visible i-

de-pendence

of the

scaling

functions does not introduce new

physical

parameters.

The

compatibility

between our

approach

and a one

parameter

scaling

for

p(g) depends

on this issue.

1. Random transfer matrix

theory

and level statistics.

As illustrated

by

figure

1,

the fluctuations of a~

(Lz)

from one member of an ensemble of metal

samples

with the same

macroscopic

characteristics to another are

surprisingly

small,

typically

of

the order of one average

spacing

between

neighbouring

ai . As discussed in references

[9 - 10],

this

"spectral rigidity" gives

rise to the universal fluctuations

[25 - 26]

of g

in the metallic

regime.

The second

important

property

of the as shown

by

numerical

studies,

which have been observed

for random matrix

products

in different contexts

[27 -

29],

is a

tendency

to have a more or less

uniform density.

(7)

distribution

[30,31],

two "maximum

entropy" approaches

were

proposed

for the

joint probability

distribution of the variable

Ai

(Lz ),

related to the ai

(Lz )

by :

We denote the two

approaches

as

"global"

versus "local". In the

global approach

[9 - 10],

the distribution of the real

positive

variables

Ai

corresponds

to a statistical ensemble of matrices

M t (Lz ).M(Lz ),

which is as random as

possible (maximum

entropy

ensemble), given

a

density

P L z

(A)

which is assumed to contain all the

dependence

on

physically-relevant sample

parameters

such as the size or the elastic mean free

path.

In the local

approach [11],

it is assumed that the statistical ensemble of transfer matrices which characterize slices of small

length

6 L z

is as random

as

possible, given

a mean free

path

~.

6 L z

is taken small

compared

to

Lz,

but

large enough

so that the chosen statistical ensemble could be

ultimately justified

by

a central limit theorem.

Then,

the evolution with

Lz

of the distribution of

Ai

is shown to

satisfy

a diffusion

equation.

This

approach,

which is necessary a

single

parameter

theory, gives

[32]

for the variance of

P(g)

in the metallic

regime

the same value as the one

previously

obtained

by

microscopic

perturbative

calculations

[25 - 26],

in the

quasi-1d-limit (Lz

»

Lt).

The

global

and local

approaches

are identical

[33] (in

the

large

N-limit)

if the

input

density

PL.

(A)

in the first coincides with the

one-parameter

density

implied by

the second. This later result adds

something

very new in

comparison

with the classic

ran-dom matrix ensembles: the ansatz chosen in the

global

approach

is not

arbitrary,

but can be

justified

by

the

underlying multiplicative composition

law

generating

the ensemble.

The distribution of the

aa,

resulting

from those two maximum

entropy

approaches,

can be

formally

written as :

where

Ca

is a normalization constant and :

The

probability

distribution

(3)

is

formally

identical to the

thermodynamic equilibrium

distribu-tion of N identical

point charges

at

positions

Ai

and

temperature

kT =

11,3, interacting

via a

logarithmic repulsion (as

in a 2d electron

gas),

but free to move

only

on the real

positive

axis in

one-dimension,

with a

neutralizing "jellium"

background

described

by

the term

involving

the

density

p~& {a).

The

logarithmic

"interaction" of the

Ai

and the effective

temperature

were de-rived

using only

symmetry

considerations

[9 -11] ;

,Q

= 1 for our case

(real

Hamiltonian which

hence can be

diagonalized

by

an

orthogonal

transformation).

This Coulomb gas

analogy

is

fa-miliar in random matrix

theory;

the crucial difference between the distribution

(3)

and the well-known Gaussian

Orthogonal

Ensemble

(G.O.E)

introduced

by

Wigner

is that the

density

p~

(A)

in our case is

apparently

far from the "semi-circle law"

characterizing

the

eigenvalue

density

in the G.O.E. This can be seen

simply

by noting

that for a G.O.E. distribution the

density

near the

origin

is

approximately

uniform whereas in our case, it is the variable a=, related to

as

by

(2),

which has an

approximately

uniform

density,

as shown in

figure

1. Let us

point

out also that the

one-parameter

density

PL.

(A) implied

by

the local

approach

has been shown

[33]

to

correspond,

in the limit N - oo, then

Lz

- oo, to a uniform

density

of inverse localization

lengths

(Xi ( (0)

between 0 and

£-1 .

In order to use our

physical

intuition to guess the statistical

properties

of

(3)

and related

(8)

approximately

uniform.

Thus,

let us consider the

distribution

hL= (111, ..., vN )

of the variables

v;(Lz)

=

2a¡( Lz ).Lz.

corresponding

to a "Hamiltonian" :

The external

potential VL~ (vi)

contains the

physical

information on the considered

sample

through

the

density

(J’L"

(v)

which is now

essentially

uniform near the

origin.

The interaction term

u(vi, vi),

which is

just

yielded by

flux conservation and time reversal

symmetry

in absence of

spin-orbit

scattering,

is no

longer

logarithmic:

To

analyze

the

consequences

of the random transfer matrix

theory

for the statistics of the

v-variables,

we need now an

analytical

expression

for the external

potential

VL.

(v)

yielded by

the

positive jellium.

We shall use for

simplicity

the

one-parameter

density

obtained

(in

the

large

~z-limit)

in reference

[33] :

This substitution

neglects,

in addition to the variation of the

averaged

spacing

(a)

between consecutive vi

(only

noticeable far from the

origin, Fig.

1 and Ref.

[5])

an additional

Lz

depen-dence of this

density,

which will be studied later

(Sects.

3 and

4).

From

(7)

and

(9),

we obtain a

simple quadratic

external

potential,

as shown in

appendix

7V~

go =

Nt

being

the classical ohmic conductance.

L,

Let us first consider a metallic

sample (.~

Lz

~).

We remind ourselves that the first

0(Ne$~ N

go

"levels" vj

such

thai vj

Vet! ,..., 1 are the ones

contributing

to the conductance g

(open

transmission

channels)

since the contribution of "levels" with vj » Vetl is

exponentially

small

(closed

transmission

channels),

as

implied

by

formula

(1).

(9)

The two-level interaction

(8)

can be

simplified

as follows :

- for the

open

channels

( vi ,

Vj « Veff ~

1 ),

expanding

cosh vs - cosh v~ , one

gets :

i.e.

again

the usual

logarithmic

repulsion,

except

that now there are

"image" charges

located at

-vj

(for Vj

>

0).

The second term of the R.H.S. of formula

(8) gives

the interaction of vi with - vj ;

- for the closed chantlels

(v; ,

v3 »

veff),

the two-level interaction reduces to a

non-interac-ting

potential

term,

plus

a

remaining

logarithmic

interaction if two

consecutive vi

are very close.

This leads us to

distinguish

between the closed channels of a metallic

sample

and the closed

chan-nels of a localized

system.

In the first case, the

spacing

(a)

between consecutive

equilibrium

po-sitions of the levels is small

(a) - 2 1

and the

logarithmic remaining

interaction term still

B

go

/

g g

involves

0 ( Ne ff )

levels. In the localized case,

(a)

»

1,

so that the two-level interaction

disappears

and

just

leaves the

non-interacting

potential

term :

When 2 >>

1,

the

logarithmic

interaction

can

only

be

probed

by

a

large

fluctuation of the levels

90

around their

equilibrium positions,

so that two consecutive levels become very close.

1.1 THE SYMMETRIC COULOMB GAS FOR THE OPEN TRANSMISSION CHANNELS - As we have obtained a

symmetric

set of

negative charges

from the two-level

interaction,

we have after the

same

expansion

from

(7)

a

symmetric

jellium

of

positive charges

near the

origin

(va

«

1)

,-which is

essentially

uniform.

Thus,

the

only

difference between the statistics of the

levels vi

« 1

and the usual random matrix G.O.E. statistics is due to the exact

symmetry

around the

origin

sa-tisfied

by

the locations of the

charges.

However since the force exerted on one of these

charges

by

the others is screened

by

the

positive jellium (the Debye screening

length

[34]

is of the order

of

~a~),

one

expects

that this exact

symmetry

does not matter very much.

Thus,

the fluctuations

of the

spacing

a, between the consecutive vi, measured in

averaged

spacing

units,

must be

des-cribed

by

the same distribution as those characteristic of the

G.O.E.,

which is

given

in a very

good

approximation

by

the so-called

Wigner

surmise :

The

spectral rigidity (statistics

A3

in

Dyson-Mehta

[35])

must also be the one of the G.O.E.

But,

the

symmetric

Coulomb gas that we have obtained for the vi

implies

in addition

something

very

specific,

which does not appear in the classical Gaussian ensemble : because of the

repulsion

(10)

essentially

different from the other

spacings.

Therefore we

expect

that vl

itself,

which is related to the transmission coefficient

T1

of the best

transmitting

channel

by :

also follows the

Wigner-Surmise,

as

supposed

in reference

[7].

This

specific

result has been chec-ked

by

a numerical calculation of 10 x 10 metallic

squares,

defined as

explained

in the introduction

(W

=

2),

which very

clearly

confirms this

prediction (Fig. 2).

Numerical studies of

larger

metallic

squares

(50x50) give

the same result. The

spacing

distribution between the other nearest

neigh-bor v;

corresponds

also to the

Wigner-Surmise

for a metallic

sample.

Such a result was found for the

Ai

in references

[9 - 10],

but

only by

"unfolding

the

spectrum"

i.e.

by numerically

scaling

to a

variable with uniform

density (which

was

approximately equivalent

to

considering

the

v;).

The

spectral rigidity

of the unfolded

spectrum,

as

measured

by

the

A3

statistic

[35]

was also found

to

correspond exactly

to that of the G.O.E. in the metallic

regime.

Now,

we are no

longer

obliged

to advocate the

independence

of the local statistics to the detailed form of the

confining potential,

we have recover for

the vi

the classical G.O.E.

quadratic potential.

Distributions of v2, v3 and v4

around their

averaged

values are

given

in

figure

3. If one

compares

the actual results to Gaussian distributions of same mean and

variance,

differences in the tails are

noticeable,

as well as an

asymmetry

around the

top

(mainly

for

v2)

which are reminiscent of the

asymmetry

of p(vl)

(Fig.

2 -

Wigner

Surmise).

Fig. 2

Fig. 3

Fig.

2. - Small

metallic squares

Lz = Lt =10, W = 2.

Probability given by

an ensemble of 6000

samples

for the first level vl, measured in units of

(vi)

= 0.39

(circles),

compared

to the

Wigner

Surmise

(continuous

line).

Fig.

3. -

Probability

of v2, v3 and v4,

compared

with Gaussian distributions of same mean and variance.

((v2)

= 0.86,

(6v2)

= 0.07, circles;

(v3)

= 1.35,

~w3 ~

= 0.09, squares;

(v4)

= 1.85,

(11)

At the other

extremity

of the

spectrum

(closed

channel of a metallic

sample),

each level viz

(v~

»

1)

experiences

a force of

unity

to the

right

from each level viz « v~,

plus

an additional

logarithmic repulsion

from

0(7Veg)

levels vi

so that

IVi - Vj

«

1

(Eq.(12)).

When

Neff.

»

1,

we

expect

that the local level statistics are

governed by

the

remaining logarithmic

repulsion, yielding

a

level

spacing

statistics in

agreement

with the

Wigner

Surmise. This is confirmed

by

our numerical results

(Fig. 4).

Fig.

4. - Closed channels of a metallic

system : distribution of the last

spacing

vlo - v9, measured in

aver-aged

spacing

units and

compared

to the

Wigner

Surmise

(continuous curve).

Lz = Lt = 10. W = 2.

1.2 THE LATTICE WITH QUASI-INDEPENDENT FLUCTUATIONS IN THE LOCALIZED REGIME - In this

regime,1

« vl « v2 ~ ... and the

spacing

betwen successive

equilibrium

positions

of the levels is

large.

The

logarithmic repulsion disappears,

and we see from

(6), (10)

and

(13)

that the

potential

U felt

by

level vj

is :

-This means that the vj » 1 have

equilibrium

lattice

positions

v?

given by :

(12)

Fig.

5. -

Probability

of

v9 and vlo,

compared

to Gaussian distributions

(v9)

=

5.4,

(5v) )

= 0.4, diamonds

-

(~10)

= 6.9,

(b V2

= 0.7,

octogons).

Lz = Lt = 10. W = 2.

Note that the last closed channels of the 10 x 10 studied metallic

squares

are characterized

by

Gaussian distributions of their

levels,

with variances of the order of

2/go (Fig. 5).

They

are in

a cross-over

regime

where the

logarithmic repulsion

remains

important,

since

(vlo - v9~ N

1.5,

but we have obtained

(6V2) -

0.4 and

(8vla) -.J

0.7,

to compare with

2/go N

0.55. Note also that substantial deviations from the G.O.E. behavior were

reported

in reference

[9]

for the

As

statistics of the unfolded

spectrum,

for

(g) -

1 where the

system

approaches

localization. The

analysis developped

in this section shows that these deviations are real and that even the unfolded

spectrum

does not exhibit the standard G.O.E.

behavior,

in contrast to the

conventional

view that after

correcting

for variations in

spectral density,

all random matrix ensembles are

expected

to show such behavior. The reason that conventional wisdom fails here is the decrease in the

level

density

with

length, again

emphasizing

the novel features of

multiplicative

random matrix ensembles. Let us mention that the

tendency

of the

joint

probability

distribution of

the vi

to

approach

a distribution of

independent

random variables in the

large

Lx

-limit has

previously

been obtained in the

study

of multimode

waveguides

by

Thtubalin

[37] (see

also

Ref. [38]).

We summarize in

figure

6 the different Coulomb

systems

yielded by

the

theory

of random

multiplicative

transfer matrices. For a metallic

sample,

the level

spacing

is small and the set of levels can be divided in series of

0(Ne~)

levels which behave as a Coulomb gas with

long

range

regularity.

The

part

which is closed to the

origin

of the levels of the open transmission channels differs

only

from the classical

Dyson’s "wobbly crystal"

[34]

by

an

image

effect. For an

insulating

sample,

the gas is so rarified that the

logarithmic

repulsion

is almost

completely

lost

(except

when

two levels

attempt

to

cross),

and instead the

charges

near the

origin

create a linear

potential

for

the j th

charge

which fix its average

position

to be at a lattice

position

V9

=

2 j /go = j ~a},

with

(13)

Fig.

6. -

(a)

Schematic

picture

of the v-levels for a metallic disordered

sample

with

Neff

open transmission channels.

((g)

~

1). (b)

Schematic

picture

of the v-levels for an

insulating

localized

sample

((g)

«

1).

2. Random transfer matrix

theory

and conductance fluctuations.

We startwith the

strongly

localized

quasi-ld

case

(L ~>~).Here~i

=

21go

=

2L/~

where ~

=

Ni,

as first obtained

by

Thouless

[39].

In this case, the

typical

conductance is determined

by:

while the conductance fluctuations are

given

by

the fact that

-it 9

= v, and that the first level v,

has

quasi-independent

Gaussian fluctuation

(vl

»

1).

So

that,

by

(18)

and

(19),

the fluctuations

of in 9

are distributed

normally,

with a variance:

This is as if each

piece

of the wire of

length - I

fluctuates

independently,

having

a conductance

~91y N

1 and

(bg2) _

1.

(21)

is the

many-channel generalization

of the

scaling

idea of Anderson et aL

[24]

for the

purely ld-system.

The latter result was also obtained for various models and

cases in one dimension

(see

Refs.[15,

40,

41]

and references cited

therein).

The

generalization

to

quasi-ld

is in agreement with the

general

idea that

In g

is additive in

strong

localization,

and was

(14)

Fig.

7

Fig.

8

Fig.

7. -

Probability

of -~n

g(circles),

compared

with a Gaussian law of same mean

((In g) =

-6.5)

and

variance

«6in2g)

=

7).

Lz = Lt =10. W = 12.

Fig.

8. - Conductance distribution

compared

with a Gaussian law of same mean

(g) -

1 and variance

(62g) -

0.17. Lz = Lt = 25, W = 4.2.

We believe that this demonstration is

simple

and

systematic,

and illustrates the power of the

ran-dom transfer matrix idea in

quantum transport.

Statistics of 2000 10 x 10

strongly

disordered

squares

have been

numerically

calculated. When localization is

strong

(W

=

12,

(.~n g) - -6.5,

Fig. 7),

in g has the

expected gaussian

distribution with a variance

(~

7)

in

agreement

with

(21).

For weaker

localization,

a

lognormal

distribution

for g

does not agree

accurately,

but we have noted that relation

(21)

is still valid for W = 8

(Lt

=

Lz = 10,

(.~n g) = - 2.55,

~b.~n2g~ ~

2.6).

If

we continue to decrease the

potential

fluctuations,

we find for W =

4.2,

(g) N

1 and

61n g -

bg.

Therefore,

if we continue to look at

p(g)

from the localized channel view

point,

the

lognor-mal distribution would reduce to a

simple

normal one. This

prediction

turns out to be

cor-rect, as illustrated

by figure

8,

however the variance

(6g2) f’J

0.17 does not agree with

(21),

but rather with the

2d-perturbative

result for the

amplitude

of the universal conductance fluctuations

(~bg2~u.c.F. ’~

0.1857

for g

measured in units of 2

e2/h).

This shows us that the

logarithmic

inter-actions

(formula (11))

are now efficient and reduce the

amplitude

of the conductance fluctuations.

Then,

it is more correct to look now at

p(g)

from the

open

channel view

point.

In the metallic

regime,

~bg2~

does not

depend

on

(g)

and takes a universal value. This can

be obtained

by

assuming

the

logarithmic

interactions for the 0

(Neff)

levels and

using

the

Dyson-Mehta G.O.E. results

[7] :

any linear statistic Z

roe 1 f

(v1)

has a variance which does not

depend

on the average number

Neff

of relevant

levels,

when

f

is a smooth function. The deriva-tion of the whole distribuderiva-tion of conductance fluctuaderiva-tions

requires

a more subtle

analysis.

The

genericity

of G.O.E.

predictions

for the level correlations has

recently

been studied in references

(15)

matrices does not

change

the level correlations.

Then,

going

back to the

ai

and

assuming

that the level

density

p(A)

is smooth

enough,

it was

argued

[44]

that

p(g),

as any linear statistic

de-fined on a random matrix

ensemble,

is

gaussian. Figure

9,

where a statistic

including

6000 small metallic

squares

is

reported,

supports

such a

conclusion,

and the variance of this numerical si-mulation

(8g2) ’-

0.1923)

does not

significantly

differ from the

2d-perturbative

result.

But,

the

universality

of G.O.E.

predictions

for level statistics and conductance

fluctuations

breaks down in the localized

regime,

as

previously

shown.’,

and even in the metallic

regime

where non Gaussian corrections to

p(g )

were first found

by

Altshuler et al.

[14]

from a calculation of

higher

cumulants

of g. We note that our numerical simulations do not show any visible deviations from

gaussian

tails for the

large

fluctuations when

(g) >

1. It is

possible

that the

non-gaussian

tails arise from

extremely improbable samples

which

practically

do not occur in the finite ensemble used. The

difficulty

to see tails

corresponding

to an

exceedingly

small fraction of the statistical ensemble is known in others

physical

contexts, e.g. : the Griffiths

singularity

in dilute

Ising

models

[45].

Fig.

9. - Conductance distribution in the

metallic

regime,

compared

with a

gaussian

law of same mean

((g) - 3.62)

and variance

~S2g~

= 0.19. Lz = Lt = 10, W = 2.

’Ib

push

further our

investigations

of the conductance fluctuations in the metallic

regime,

let

us return to the v-variables.

We can obtain the Gaussian distribution within the

Neff

approximation, using

a method intro-duced in reference

[46]

for

calculating

the fluctuation

~N(E)

in the number of levels in an energy

interval E. The idea is to estimate the

energy A

needed to take

6NetI

uniformly spaced

v-levels from the

segment

[1,1

+

E]

into the

segment

[1- ~,1],

and to use:

were 3

= 1 for the

samples

with

spin-independent hopping

matrix elements and site

energies,

(16)

note that the total force

acting

on each level is

equal

to zero at

equilibrium,

so we have

just

to

take into account the two-level interaction between the translated levels

("negative charges")

and

the "holes" which are created after the fluctuation at the

non-occupied

equilibrium positions.

Then the

energy A

required

to form additional

charges

of ~

6 Ney

in the two

segments

is:

Considering

In

Bch x -

ch

yB

instead of

In )z -

g~

will

just

change

the value of the constant, and

will

give

also a Gaussian distribution with a variance

independent

of

parameters.

In order to continue this discussion very

qualitatively,

we note that the fluctuation of

~6Neff

uniformly spaced

v-levels around 1 could be

energetically

favourable for small

&g,

but another

kind of excitations could have a lower energy

price

for

larger

conductance fluctuations. Numerical studies of

highly unprobable v-configurations

lead us to

envisage

on a uniform fluctuation of the level

spacings.

Let us take the

spacing

a of the "effective levels" to

slightly

differ from the average

(a)

=

2~90 ~

In this

hypothesis, g

is

given by:

which

yields

that

tn(g)

will be distributed in an identical fashion to veff :

since

~s ’ ~ ~

~eS

and

Neff’

a - 1.

The fluctuations of

6 vetr

being approximately

Gaussian,

we find that in g has an

approximately

gaussian

distribution both in the metallic and localized

regimes.

However,

note as

long

as

8g

«

~g~,

the

gaussian approximation

fits the

lognormal

one.

One may include non-uniform fluctuations for

having

a fuller

picture

of

p(g),

for

example

by

expanding

the

spacing

aj =

v3 +1- v~ in Fourier series. There are

grounds

to

believe,

following

reference

[46],

that fluctuations which are uniform on different scales are

independent.

Thus one

may express the conductance fluctuations as a sum over a

large

number

(of

order

N~$)

indepen-dent contributions. Such a sum is known

[46]

to

produce

a normal distribution on the main

part,

with correction in the

higher

moments or in the tails. We

hope

to return to a fuller treatment of

this issue in a future work.

In conclusion of this

section,

let us recall that the conductance distribution

yielded by

our

maximum

entropy

approach

could be written as:

This

expression

is not very useful for

calculations,

but makes clear that the number of

inde-pendent

parameters

necessary to characterize the

spectral

density

of the

Ai

will also

specify

the

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