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Persistent Current of Interacting Electrons: a Simple Hartree-Fock Picture

G. Montambaux

To cite this version:

G. Montambaux. Persistent Current of Interacting Electrons: a Simple Hartree-Fock Picture. Journal

de Physique I, EDP Sciences, 1996, 6 (1), pp.1-4. �10.1051/jp1:1996128�. �jpa-00247170�

(2)

Short Communication

Persistent Ctlrrent of Interacting Electrons:

a

Simple Hartree- Fock Picttlre

G. Montambaux (*)

Laboratoire de

Physique

des Solides

(**),

Université

Paris-Sud,

91405

Orsay,

France

(Received

20

SeptembeT1995, accepted

23 OctobeT

1995)

Abstract. The average persistent current

(Ii

of diffusive electrons in trie Hartree-Fock ap-

proximation

is derived in

a

simple non-diagrammatic picture.

Trie Fourier

expansion directly

reflects trie

wmding

number

decomposition

of trie diffusive motion around trie

ring.

One recovers trie results of

Ambegaokar

and

Eckern,

and Schmid. Moreover one finds an expression for

(Ii

which is valid

beyond

trie diffusive

regime.

PACS. 05.30Fk Fermion systems and electron gas.

PACS.

72.10Bg

General formulation of transport

theory.

PACS.

71.25Mg

Electron energy states m

amorphous

and

glassy

solids.

The

physics

of

persistent

currents in

mesoscopic

isolated

rings pierced by

an Aharonov-Bohm flux

#

,

bas attracted a lot of interest on tl~e

description

of tl~e

tl~ermodynamic properties

of

mesoscopic metals,

both in tl~e

non-interacting picture

or in trie presence of electron-electron in-

teractions. Trie

description

of trie interactions is a

complicated

task:

although

several attempts bave been made to describe trie rote of the interactions in one-dimensional or few-cl~annel

rings,

with the

help

of

analytical

arguments or numerical calculations

[ii,

trie diffusive nature of trie electronic

motion,

which is

probably

essential in trie

experiments

on metallic

rings

with finite thickness

[2-4],

has been treated

originally

in two series of papers

by Ambegaokar

and Eckern and Scl~mid

là, 6]. They

calculated tl~e average

persistent

current in trie Hartree-Fock approx- imation where tl~e interaction is treated

perturbatively

in a

diagrammatic picture. Althougl~

tl~is calculation

provides

an average current smaller that

experimentally

observed

[2],

one can

believe tl~at it contains tl~e essential

pl~ysical ingredient namely weakly interacting

diffusive electrons. Thus it may be

mteresting

to

simplify

as much as

possible

trie calculation in order to

possibly generalize it,

or to compare it with numerical calculations. In the above papers, the average

persistent

current is calculated with a

diagrammatic technique

where the diffusive motion is described

by

a

Cooperon pote

with a wave vector

quantized by periodic boundary

conditions.

Then, by

Poisson

summation,

this sum over diffusive modes is transformed into a

sum over harmonics with

periodicity #o/2

where

#o

is trie flux quantum.

In this short note, we propose a

simple

denvation where tl~e average current is

directly

related

to trie return

probability

for a diffusive

partiale.

Then tl~is return

probability

is

expanded

according

to tl~e

winding

number of tl~e dilfusive motion around tl~e

ring,

wl~ich gives

directly (*)

e-mail:

[email protected]

(**)

associé au CNRS

©

Les

Éditions

de

Physique

1996

(3)

2 JOURNAL DE

PHYSIQUE

I N°1

access to the harmonics

expansion

of trie current.

Moreover,

we obtain a

general expression

which can be used

beyond

tl~e diffusive

regime.

Consider a

quasi-one

dimensional

ring

of

perimeter

L and of transverse section

S,

in wl~icl~

the motion is

supposed

to be diffusive

along

tl~e

perimeter

and uniform

along

tl~e transverse section.

Tl~e first

step

is to write tl~e total energy

ET

in tl~e Hartree-Fock

approximation:

ET

=

El

+

~j U(r r')

(ifij

(r')(~(ifi~(r)(~drdr' Il)

~~~

Î

£

à«~«~

/ U(r r')ifij (r')ifij jr)

~§]

(r)ifi~(r')drdr'

~>J

where

E[

is tl~e total energy in trie absence of interaction. In trie lowest order in trie interaction

parameter,

the states ifi~ are the states of tl~e

non-interacting system.

Tl~e summation

£~

~ is over filled energy levels. a~ is the

spin

of a state ifi~.

Considering

that the Coulomb interaction

U(r r')

is screened in trie metallic

regime,

it is

replaced by U(r r')

=

Uô(r r')

where U

=

4ire~/q(~

and qTF is trie Thomas-Fermi wave

vector

[5-7]. Replacing

the interaction m

equation (1) by

a à function is

certainly

correct as

long

as trie Thomas-Fermi wave

length

is smaller than tl~e mean free

patl~ le: qTfle

» 1. Tl~e interaction

being

now considered as

à-like,

it is

quite

easy to see tl~at the Fock term has the

same structure as the Hartree term.

Introducing

the local

density n(r)

=

£~ (ifi~(r)(~,

the total energy can be rewritten:

ET

=

El

+ U

/ n~(r)dr ) / n~(r)dr (2)

The Fock term is half the Hartree contribution because of the constraint on the

spin

and its

sign

is

opposite

because of

exchange

of

partiales.

The local

density n(r)

can be

expressed

in

terms of the Green function:

n(r)

=

(-1lin) f)~ ZmGR(r,

r,

uJ)dur

so that trie average current

is given

by

[8]

IIe-e('))

~

(~() (3)

=

$ (

/~~ /~~ /(G~(r,

r,

uJ)G~(r,

r,

uJ'))duJduJ'dr

where

G~ (G~)

is trie retarded

(advanced)

Green function. Trie

product (G~(r,r)G~(r,r)) simply

expresses trie

probability

to go from some

point

r to itself [9]. More

precisely,

for a

partiale

at energy E

[10,11]

P(E,w)

=

£iG~(r,

r, E +

w/2)G~(r,r,E w/2)j (4j

is trie Fourier transform of trie retum

probability P(E,t)

after a time t :

P(E, t)

=

P(E,uJ)e~~~~duJ

(5)

2ir

Because of disorder average, this retum

probability

is

mdependent

of the

position

r. The

current can Dow be

expressed directly

m terms of

P(E,t). Neglecting

the energy

dependence

(P(E,t)

=

P(t)),

one

gets:

~ ô

/°° P(t,~)

~~

(6)

(~~-~

~~~~

~~~~

~

~~

~~

(4)

Q

= LS is the volume. Since the relation

(4)

is exact, the

expression (6)

is

quite general

and is valid

beyond

the diffusive

regime.

In the classical

approximation

for the diffusive

regime (le

<

L),

the diffusion

probability

is the solution of a classical diffusion

equation

D/lP =

ôP/ôt

where D is the diffusion coefficient taken here at the Fermi

level,

D

=

une/3.

It is

given by

~~

~~'~"

~~

4irjÎt)d/2

~ ~~ ~'~~~~~~

~~~

In the

geometry

of a

quasi-one-dimensional ring,

the return

probability

can thus be

expanded according

to the

winding

number of the diffusive motion:

P(t, ~)

=

~j

e~

Ù

[1 +

co8(~~rmp)j (8)

S@$

~

where ç7

=

#/#o.

The second term, of

importance here,

results from the

phase

interference between time-reversed

paths

in the semi-classical

approximation,

each

path accumulating

a

phase ~2irmç7 [10,12].

In zero

flux,

the return

probability

is twice the classical one. This

expansion according

to the

winding

number grues

directly

the Fourier

decomposition

of the current:

ii-e (#))

=

£ Im sin(4irmç7) (9)

m

with

__

i~

=

8mUPo / ~-i

dt

~ioj

#cris

o

t5/2

We have introduced the Thouless energy

E~

=

hD/L~. Defining

a dimensionless

winding

number w

by w2

=

m~/4E~t, Im

can be

simply

rewritten as

~ ~

~~

~P0 ~c /" ~2~-w~

~~

~

fi #o

m2

~

~~~~ ~

~~~~

which is the result of

Ambegaokar

and Eckem [5] and Schmid [6].

We finish with the calculation of the current at finite

temperature

T where two Fermi factors

f(e)

have to be introduced in

equation (3). Dring

the standard substitution

f f(e)g(e)de

=

2iirT£~ g(iuJn)

where mn =

(2n +1)irT,

the average current at finite T is

straightforwardly given by:"

IIe-e)

=

-QUAD

~

l 47r~T~ ~j Pii~J» i~Ji)

~

~~~° Ii Î si~lh

ÎTt)2 ~~~'~~~~

~~~~

By introducing

the same dimensionless

wmding

number w as

above,

the harmonics

Im

are

given by

~

~~ ~~~ ~~

~~~

/Î Î ~~~~~

~~

ÎÎÎ

~~ smh

21fi

~~~

where

Tm

=

E~/m~

is the effective

temperature

associated with the

winding

number m and Ùm =

T/Tm. Although

the

integrand

is

quite different,

this

temperature dependence

is identical

(5)

JOURNAL DE

PHYSIQUE

I N°1

to the one found

by Ambegaokar

and Eckern [5]. It

directly

expresses the current in terms of

a

temperature

square average of a

winding

number.

Equation (ii

shows that the

persistent

current is

proportional

to the interaction parameter.

It is known that this current is smaller than

experimentally

observed [2].

Moreover, Cooper

channel renormalization reduces further trie

amplitude

of the estimated current

[15].

Aise the

importance

of trie

self-consistency

m trie Hartree-Fock

approximation

in still under numerical

investigation [13].

A different

approach,

based on

Density

Functional

Theory,

also

gives

similar

results,

smaller than the

experimental

one

iii.

In

conclusion,

we have calculated the average

persistent

current in the first order of the Hartree-Fock

approximation. By writing

the current

directly

m terms of the

winding

number

decomposition

of the return

probability,

we have avoided the use of the

diagrammatic

calcu- lation and

directly

found the harmonic

expansion

of the current.

Although

this calculation

is reminiscent of trie semidassical

description

of the

spectral

correlations and of the average current of

non-interacting partides

m the canonical ensemble

[14],

it does not use any semidas- sical sum

rule,

since here the correlation function of interest can be

exactly

written in terms of

the retum

probability

without any

approximation. Moreover,

we have written an

expression

for the average current

(Eqs. (6)

and

(12)

which is valid

beyond

trie diffusive regime and may be used for

example

m trie ballistic regime where

interesting magnetic

response have also been

observed

[16].

References

iii Müller-Groeling A.,

Weidenmuller H-A- and

Lewenkopf C.H., Europhys.

Lett. 22

(1993) 193;

Abraham M. and

Berkovits, Phys.

Reu. Lett. 70

(1993) 1509;

Bouzerar

G.,

Poil-

blanc D. and Montambaux

G., Phys.

Reu. B 49

(1994) 8258;

Kato H. and Yoshioka

D., Phys.

Reu. B 50

(1994) 4943;

Giamarchi T. and

Shastry B-S-, Phys.

Reu. B 51

(1995) 10915;

Itamm

M.,

Reulet B. and Bouchiat

H., Phys.

Reu. B 51

(1995) 5582;

Kamal

Ill.,

Musslimani Z-H- and Auerbach

A.,

J.

Phys.

I France 5

(1995)

1487.

[2]

Lévy L.P.,

Dolan

G.,

Dunsmuir J. and Bouchiat

H., Phys.

Reu. Lett. 64

(1990)

2074.

[3] Chandrasekhar

V.,

Webb

Il.A., Brady- M.J.,

Ketchen

M.B., Gallaghern

Vi.J- and Klein-

sasser

A., Phys.

Reu. Lett. 67

(1991)

3578.

[4]

Mailly D., Chapelier

C. and Benoit

A., Phys.

Reu. Lett. 70

(1993)

2020.

[5]

~~mbegaokar

V. and Eckern

U., Phys.

Reu. Lett. 65

(1990) 381;

ibid 67

(1991)

3192.

[6] Schmid

A., Phys.

Reu. Lent. 66

(1991)

80.

[7]

Argaman

N. and

Imry Y., Physica Scripta

49

(1993)

333.

[8] Dther non flux

dependent products

of Green functions have been omitted in this expres-

sion.

[9]

Feynman

Il.P. and Hibbs

A.It., Quantum-Mechanics

and

Path-Integrals (McGraw Hill, 1965); Feynman R-P-,

Reu. Med.

Phys.

20

(1984)

367.

[10]

Chakravarty

S. and Schmid

A., Phys. Rep.

140

(1986)

193.

[iii Prigodin V.N.,

Altshuler

B-L-,

Efetov K-B- and Iida

S., Phys.

Reu. Lett. 72

(1994)

546.

[12] Bergmann G., Phys. Rep.

107

(1984)

1.

[13] Eckern U., Z.

Phys.

B 82

(1991) 393;

Altshuler B-L- and Aronov

A.G.,

Sou.

Phys.

JETP 57

(1983)

889.

[14]

Bouzerar G. and Poilblanc D.

(unpublished)

[15] Argaman N., Imry

Y. and

Smilansky U., Phys.

Reu. B 47

(1993)

4440.

[16]

Lévy L.P.,

Reich

D.H.,

Pfeiffer L. and ~iest

K., Physica

B

(Amsterdam)

189

(1994)

204.

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