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Extended proof of long-range order in the two-dimensional quantum spin-1/2 XXZ-model at T=0

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Submitted on 1 Jan 1991

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Extended proof of long-range order in the

two-dimensional quantum spin-1/2 XXZ-model at T=0

Hans-Aloys Wischmann, Erwin Müller-Hartmann

To cite this version:

Hans-Aloys Wischmann, Erwin Müller-Hartmann. Extended proof of long-range order in the two-

dimensional quantum spin-1/2 XXZ-model at T=0. Journal de Physique I, EDP Sciences, 1991, 1

(5), pp.647-657. �10.1051/jp1:1991109�. �jpa-00246359�

(2)

Classification

Physics

Abstracis

75.10Jm

Extended proof of long-range order in the two-dimensional

quantum spin-1/2 XX2kmodel at T

=

0

Hans-Aloys

WischJnann and Ervin Mfiller-Hartmann

Institut ffir Theoretische

Physik,

Universitit m K61n,

Zfilpicher

StraBe 77, D-W 5000 K61n 41,

Germany

(Received25

January J99J,

accepted

J

February

J99J)

Abs«act. We prove the existence of

long-range

order

(LRO)

in the

ground

state of the 2D quantum

spin-1/2

XXZ-model for all

anisotropies

0 WA « 0.22 and Am1.47. We achieve this extension of

previous proofs by developing

an

improved

variant of the

Dyson-Lieb-Simon proof

of LRO in quantum spin systems and by deriving improved upper and lower bounds for the

ground

state energy of the XXZ-model.

1. Introduction.

In recent years, there has been a resurgence of interest in low-dimensional

quantum spin models,

which

considerably

increased with the

discovery

of

high-temperature superconductors ii

]. Due to the

layered

structure of these

materials,

most of the

early attempts

to describe the

novel

physics

were based on electronic and

magnetic

correlation effects in two-dimensional models. The

simplest

of

these,

the Hubbard and the

Heisenberg

models have since been the

object

of innumerable

studies,

and the

investigation

of the

ground

state

properties

of these

models has outlasted the somewhat naive

hopes

of a

simple

electronic mechanism for

superconductivity.

The most

interesting

and most

extensively

studied

property

of the

ground

state of the

antiferromagnetic Heisenberg

model is the

decay

of the

spin

correlation functions with distance.

Although

much numerical evidence for the existence of a

Nkel-type antiferromagne-

tic

long-range

order

(LRO)

has been

accumulated,

a

rigorous proof

for the square lattice is still

missing.

On the other

hand,

there has been

significant

progress in

higher

dimensions and for the

anisotropic generalization,

the XXZ-model :

H

=

£ (S) )+

+

St )Y

+

AS) )f)

with A m 0

,

(1)

(<Jl

where the

exchange

interaction J has been set to

unity.

A number of authors

[3-6]

extended

the scope of the

original proof by Dyson,

Lieb and Simon

[2]

for the

Heisenberg

antiferromagnet

and

generalized

it to the XXZ-model. In this manner, Kubo and Kishi

[8]

(3)

were able to show the existence of LRO in three and more dimensions for all

spins

S in the whole

antiferromagnetic region,

in two dimensions for SW I also for all

Am

0,

as well as for S

=

1/2

in the KY-like

region

0 WA

~ 0.13 and the

Ising-like region

A m 1.78.

Ozeki,

Nishimori and Tomita [9] extended this

proof

to A

m 1.72. Their

proof

for 0 « A <

0.20, however,

is not

rigorous

: it uses «variational »

energies

which Suzuki and

Miyashita [13]

calculated in a very

good

but uncontrolled

approximation

as upper bounds for the energy. The same

energies

are also used in the

proof

for 0 « A « 0.59

by

Nishimori and

Ozeki

[10].

In

addition,

this last result as well as the

proof

for A

m 1.10 also contained in

[10],

is based upon the

assumption

that the

nearest-neighbour

correlation functions are monotonic functions of the

system

size. This

assumption

was verified

numerically

in

[10]

for the

10, 16,

18 and 20

spin

systems with Oitmaa-Betts

[12] boundary conditions,

but we have found that the

x-component

of these correlations does not show any

monotonicity

for A=0.8 and A

=

0.9 when one includes the 26

spin

system

('). Although

this range of A is outside the

region

of interest for the

proof,

a doubt is cast on the

validity

of the

assumption,

since

larger

systems may exhibit this kind of behaviour at smaller values of A. On the other

hand,

the

proof

for the

Ising-like region

A

m 1.67

given

in

[10]

is

rigorous,

so that the existence of LRO in the

ground

state of the XXZ-model has been shown for all

dimension,

all

spins

and all

anisotropies

with the

exception

of

S=1/2

on the square lattice for the

anisotropies

0.13 w A w 1.67.

In this work we present an extension of the above

proofs

to the KY-like

region

0 w A w 0.22 and to the

Ising-like region

A m

1.47,

thus

closing

as much of the

remaining

gap

as is

possible

with this method. The

improvement

is achieved

by optimizations

on three

aspects

of the

existing proofs

in section

2,

we

present

an

improved

variant of the

Dyson-

Lieb-Simon

[2] (DLS) proof,

in section 3 we derive

improved

lower bounds for the x-

component

of the

nearest-neighbour spin

correlation

functions,

while section 4 is devoted to

improved

variational

energies. Finally,

these parts are assembled and the results are summarized in section 5.

2. The method.

Following

Kubo and Kishi

[8],

we define the Fourier transform of the I-th

component

of the

spins 6j

on a D-dimensional

hypercubic

lattice A

(with

its

reciprocal

lattice

A*)

and the

positive

semidefinite

quantity gl'~

=

(S[ S[~)

that satisfies the

following

sum rules :

( z (Sk Sk) =( z gl'~

and

(3)

ReA peA.

( £ (6lt Sk

+

e~)

"

j £ (gl'~

C°S

pm) (4)

Re A pe A"

(1) Our numerical deternfination of the ground state correlation functions

produced

the

following

values for the 18, 20 and 26

spin

systems:

(6~S~)~~=-0.13044,

-0,13040, -0,13044 and

$~ S~j

~ ~ =

0,12477, 0.12474, 0.12501

(4)

In the

thermodynamic limit,

the correlation functions become

independent

of the lattice sites R and the bond directions e~, and we obtain

(S( S()

=

i~~~

~ g)~~ + lim

( g(~

and

(5)

Bz

(2

gr

)

A

- m

($ S(

=

~~~

~ gj~~

j (

cos p~ + lim

( g(~

,

(6)

Bz

(2 ")

m=i Al -m

provided

the

gl'~

are bounded from above for all p #

Q. Here, Q

=

(gr,

gr,..

)

is the wave vector

corresponding

to

antiferromagnetic LRO,

and the second term on the

right-hand

sides of

(5)

and

(6) is, just

the related order

parameter

lim

g(~

= lim

~

£ exp(-iQR) Sk I= (ml'~)~ (7)

A

- m

~

A

- m

A

ReA

~

A

rigorous proof

of LRO can thus be obtained

by deriving

a lower bound for the left-hand side and a smaller upper bound for the

integral

on the

right-hand

side of either of these

equations.

At this

point

we remark that we do not have to choose between

(5)

and

(6),

but can instead

investigate

the linear combination

IS Sii

+ «

<Si Sol ~z

~/)~ ~i~ la i ~l C°S

Pm +

+

(a

+

I)

lim

g(~, (8)

(Al -m

A(

which reduces to

(6)

for a

= 0 and to

(5)

for infinite a. In

tiis variant, rigorous proofs

can be obtained for all values a m

I,

but

negative

values do not

yield improved results,

so that we shall

only

be concemed with a m0 in the

following.

The introduction of the

parameter

a thus leads to a

family

of

proofs containing

the best

proof

conceivable

using only

site-

diagonal

and

nearest-neighbour

correlation functions.

The

required

upper bound for

gl')

was

originally

derived

by Dyson,

Lieb and Simon

[2]

for the

Heisenberg

and the KY-model in three and more dimensions at finite

temperatures.

Neves and Perez _[3] then showed that the two-dimensional

problem

can be treated in the

same manner, as

long

as the

zero-temperature

limit is taken before the

thermodynamic limit,

while

Kennedy,

Lieb and

Shastry [4] directly

derived the same bounds in the 2D

ground

state.

These results were

subsequently generalized

to the

anisotropic

case

by

Nishimori et al.

[7],

who obtained the

following

formulas for zero

temperature

in the

thermodynamic

limit

g(I)

~

j(I)

I

( B(I)

c (I))1<2 j~ (x), ~) ~~

~,~-

i j~ (z) ~~ ~ ~,

~-

i ~~~

P P

~2

P P ' P P ' P P '

D D

Cj~)~ ~~ =

2

£ (1

A cos

p~) lxx)

~

2

£ (A

cos

p~) (zz)

~ ,

C)~)

= 4

lxx)

~

E~

,

m i m =1

(lo)

D D

Ej

=

£ (I+cosp~), E~

=

£ (I-cosp~), (11)

m=i m=1

where the

following

abbreviations for the

nearest-neighbour spin

correlation functions have

(5)

been introduced :

(xx)~

=

(S(Stj(A)

and

(zz)~

=

($S()(A). (12)

Inserting

the above

expressions

for

j)~)

for the two-dimensional case into

(8),

we obtain the

following

sufficient condition for LRO in the

z-component

in the

Ising-like region

A m :

~

j- lxx)

~

~~~~4

~

4 " 2 A

'~~~"~

~~~~

with

where the

«

+

» indicates

that

the

integration is estricted to that part of

which the ntegrand

is

positive. imilarly, the ollowing ufficient condition

for

RO in the

jxxj~+f> jxx)~.fi.r~(«). (15)

Here we have used the fact that

~

j2-cospi -~°~P2. (2 a)

+

~~~"'~~

"

i[z 2('1)~

~

~ ~°~~~

~l~~[lospi

xC°~P~.

(-

cospi

°SP2~)

~~~~

+ ~ ~ cos pi + COS p2

il

is an

increasing

function of x, so that we were allowed to

replace h~(a,rj) by h~(a,

I

)

=

r~(a )

because the

argument jzz )

~ + A

lxx)

4

(1?)

ri "

j xxi

~ + A

jzzj

4

is bounded

by (rj

w I. This can

easily

be verified

using

the

equations (14a)

and

(14b)

of Nishimori et al.

[7].

These

equations

also prove the

inequality (zz)~«- lxx)

~

for

0 WA w I which has been used to

simplify

the

right-hand

side of

(15).

Following

Nishimori and Ozeki

[10],

we now transform the above conditions

(13)

and

(15) using

the

monotonicity(2)

of the correlation functions

(xx)~m lxx)

for Am I and

lxx)

~ m

(xx)

~

for A m 0 as well as variational values for the

ground

state

energies

per bond : e~

(A)

W

e0(A)

#

2

jXX)

4 ~ A

l~~)

4'

(18)

We

finally

obtain the

following

sufficient conditions for LRO in the z-component in the

Ising-

like

region

A m I :

~y

j- (XX)j.A

~v(4)"4~+2~~~)l~

~

°~2("), (l~)

~2)

This

can

rigorously

be shown

using simple

variational arguments.

(6)

and for LRO in the x-component in the KY-like

region

0 « A «1:

~

+ " »

fi r~(

« for « » o

(20)

fi

4

-(xx)~

2

3. Lower bounds on the

spin

correlation functions.

In order to be able to make use of these

formulas,

we need

good

lower bounds on the

correlation functions

lxx) (at

the

Heisenberg point)

as well as

lxx)

~

(at

the

KY-point),

that

can

evidently

be deduced from lower bounds on the

ground

state

energies. Slightly generalizing

an

elegant application

of the variational

principle

that was

developed by

Nishimori and

dzeki [10],

these

can in turn be derived

by numerically calculating

the

ground

state

energies E#( ((y)

of the

inhomogeneous

Hamiltonian

HI

=

£ (y($~ f+

+

St fY

+

AS) )f) (21)

(;y)

on a finite

plaquette

with open

boundary conditions,

where the

(j

m0 represent bond-

dependant

interaction

strengths. Using

the

ground

state of the

homogeneous

model on the infinite lattice as a variational test state and

taking advantage

of its translational and

rotational

symmetry,

we then obtain

(H/)

=

£ (~ (2 (xx)

~ + A

(zz ) ~)

m

E#( ( (y ) ) (22)

( ,j)

This leads to the desired lower bounds on the

ground

state

energies

per bond for the infinite

homogeneous

model

Et( jzj1 )

(23)

~°~~~

~

z ij

~

and

finally

to the

required

bounds on the correlation functions :

E(( (/y ) El ( (y) )

( xxi

~ m

and

( xxi

m

(24)

2

£ (y

3

£ (j

The

remaining

task is to

judiciously

choose the set of interaction

strengths ((j)

so as to maximize these bounds. Since a

systematic study

of all

possible

sets is not feasible for

large plaquettes,

we have used the

following

heuristic rule that has

always

proven to

yield

very

good

bounds: for the case of a

plaquette

of

Nx by N~ spins,

the interaction

strength

(~

for the bond

(ij)

is determined as the function

S(x, Y)

=

Ii

+ C°S

1~ i~" Ii

+ C°S

1~ i~" 1, (25)

evaluated at the centre of the

bond,

where the

origin

of the coordinate system has been

placed

at the centre of the

plaquette

and the bond

length

has been set to

unity.

We have been able to determine the

ground

state

energies

of

HI

and

H/

with these

interaction

strengths

on the 5 x

4,

6 x 4 and 6 x 5

plaquettes using

a modified Lanczos

(7)

method (3). The

resulting

lower bounds on the correlation functions are :

(xx)

m 0. II

764, 0.11681,

0. II 524 and

(26)

(xx)~

m

0.14094, 0.14034,

0.13942

(27)

respectively.

The

comparison

of the best obtained bounds with the

numerically

determined

lxx)

correlation functions for the

16, 18,

20 and 26

spins

systems

(using

Oitmaa-Betts

[12]

boundary conditions)

in

figure

I

clearly

shows that our bound on

lxx)

~

is excellent in the KY-

region

and

quite satisfactory

in the

Ising-like region.

4.

Upper

bounds on the

ground

state

energies.

To

complete

the

proof,

we now have to derive

good

upper bounds on the

ground

state

energies.

For this purpose, we start from the Nkel-state

N)

that has

positive z-components

for the

spins

on the A-sublattice and divide the infinite 2D lattice into

equal rectangular plaquettes P,.

We then

investigate

the

following

variational state

~P~)

that was

originally proposed by

Bartkowski

ill]

and

subsequently

studied on 2x2

plaquettes by Ozeki,

Nishimori and Tomita

[9]

(~P~)

=

fl fl' (I

+

ASP S()(N), (28)

P, (<,b)eP,

where

fl'

is restricted to nearest

neighbour pairs jab)

with as A and be

B,

and

A is a real variational

parameter. Furthermore,

the conventions S+ =S~+iSY and

S~

=

S~- iSY will be used for the ladder

operators.

Due to the fact that these

operators

commute

provided they

are on different lattice

sites,

the calculation of the energy is

04

20 18

°6 18

08

~ li

,,

V ,>,e.3,4.5

iz

14

18

o 5 1-o 1.5

A

Fig,

I. Correlation functions

lxx)

~

for the 16, 18, 20 and 26 spin systems with Oitmaa-Betts [12]

boundary

conditions

(curves) compared

to the

rigorous

lower bounds

(xx)

~

and

(xxi (straight lines).

The inset shows the XY-like

region

on an

expanded

scale.

(3) For the 6 x 5

plaquette,

one Lanczos step consumed

approximately

10 minutes CPU time on one processor of an

IBM-3090-6005/VF,

and 35 steps were necessary to achieve convergence.

(8)

straightforward

and leads to

ev

(A)

=

£ £ (If-

+

AIl$)/Io

+

£ £

'

(AII I])/Ii (29)

ab)e P (<,b

Here M is the number of

spins

per

plaquette

and

£'

is restricted to nearest

neighbour pairs jab

with a e

Pi

and b e

(P~

U

P~),

where

P~

is the

right

and P~ is the upper

neighbour

of

plaquette Pi.

The introduced

expectation

values I can be

expressed

as

Io(A

=

(~P([ ~P() (30)

1](A )

=

(~P([S[[ ~P() (31)

1(~_ (A

= ~P

([ St Sp

+

Sp St

~P

() /2 (32)

I~(A

=

(~P([ S( S([ ~P() (33)

with the

help

of

~P()

=

fl' (I

+

ASP St ) [fir)

,

(34)

jab)eP

where

fir) represents

the

configuration

of the

spins

on

plaquette

P when the infinite lattice is in the Nkel-state

)N).

As we shall

show,

an evaluation of these formulas leads to very

satisfactory

variational

energies

for the

Ising-like anisotropies

Am

I,

even if the lattice is divided into very small

plaquettes.

It thus appears

amazing

that this test state is

seldomly

used for the KY-like

anisotropies.

For 0 WA w I it is of course

advantageous

to renumber the

coordinates in the Hamiltonian

(I)

and

study

the

equivalent

form

ji

=

£ (AS/ f~

+

Sf fY

+

S) f~) (35)

(;j)

=

£

~

(St )+

+

S/ ()

+

£

~ ~

($+ §

+

Sj )+ )

+

S) )~ (36)

j,~~ 4

;~j 4

We have calculated the energy

i~ (A )

of the test state ~P~ with

respect

to

ji. Noticing

that

the first sum in

(36)

does not contribute because it does not preserve the z

component

of the total

spin,

we obtain :

iv (A)

=

~j £ ((A

+ I

I~t_ /2

+

Ijf)/Io

+

£ £' (Ii If)/Ii (37)

jabje P jab>

Denoting

the sums of the

expectation

values I

by

j~_

£, ~a~b

j~

£

~ab j~

£

~ab

(3~)

z z z, zz zz, + + ,

(<,b) (ab)E P jab )EP

the variational

energies

can

finally

be

expressed

as :

e~ =

£ ((T~_

+

AT~~)/Io

+

(AT~)/I/)

and

(39)

i~

=

(A

+ I

) T~ /2

+

T~~)/Io

+

T~/1() (40)

we have written a

computer

program to

symbolically

evaluate

Io

and the sums T for the case

(9)

of 2 x

2,

3 x

3,

4 x 4 and 5 x 5

plaquettes.

The details can be found in

[14],

and the results for the 5 x 5

plaquette

are

given

in the

appendix.

The

subsequent

numerical minimization of the

energies

with

respect

to A for 201

equally spaced anisotropies

in the range 0 WA w 2 then

provided

us with the

required

upper bounds on the

ground

state energy.

We were able to further

improve

these values

mainly

in the

vicinity

of the

Heisenberg point by investigating

the

following generalization

of the test state

*i)

"

fl C~P(~

'l

(Nil Nil))' n' (I

+

ASP St ) l~>

,

(41)

P, (ab)eP,

where

Nl'/

and

Nl'i~ represent

the number of

parallellantiparallel neighbouring spins

on the

plaquette P;.

The

original

test state

corresponds

to

Y~ =

0,

and

Y~ = 0.03 leads to

slightly

better variational

energies

for all

anisotropies

whereas

Y~ =

0.06 leads to

slightly

worse

values. Since the

improvement

is so small that the scope of the

proof

is not

extended,

we refrain from

writing

down the

corresponding

sums T. The

energies

for

Y~ = 0.03

have, however,

been used in

determining

the bounds of table I and have been included in

figures

2 and 3 which present the variational

energies

for the KY-like and the

Ising-like regions.

It is evident from these

figures,

that we have been able to

considerably improve

the variational

energies

over the whole range of

anisotropies.

Table I.

Limiting

values

A~,~(a) for rigorous proofs of

LRO in the z-component and

A~~~(a) for rigorous proofs of

LRO in the x- as well as the y-component.

«

r~(«) A~~(«) A~~~(«)

0.0 0.646803 1.52 0.19

0.1 0.758695 1.49 0.21

0.2 0.877613 1.48 0.22

0.3 1.001576 1.47 0.21

0.4 1.129471 1.47 0.20

0.5 1.260509 1.48 0.19

0.6 1.394080 1.49 0.17

S. Conclusion and summary.

Assembling

the

improvements

that were

presented

in the

preceding

three

sections,

we are

now able to extend the scope of the

proof

of LRO. In section 3 we derived a lower bound of

lxx)

m 0.11524 on the

x-component

of the

nearest-neighbour spin

correlation

function,

which should be

compared

to the bound

lxx)

m 0.11895 derived

by

Nishimori and Ozeki

[10]

and to the

numerically

obtained value of

lxx)

m 0. I1167.

Inserting

our bound into the

original proof already

extends its

validity

from A

m 1.67 to A m 1.61.

Adding

the

significantly improved

variational

energies

we calculated in section

4,

the

original proof

becomes valid for all

anisotropies

A m 1.52 and 0 w A w 0.19.

Numerically evaluating

the

integrals r~(a)

and

inserting

the lower bound

lxx)

~ m 0.13942 we derived in section

3,

the variant of the DLS method which we derived

in section 2 then leads to

proofs

of LRO in the

x-component

for all

anisotropies

0 w A «

A~~~(a )

and in the

z-component

for all

anisotropies

Am

A~~(a

with the

limiting

(10)

24

z6

11

28

30

32

0 Z 4 6 8 1-O

1i

Fig.

2. Variational

energies

for the XY-like

anisotropies.

The centre lines show the

energies

obtained for the test state 4~~

) by dividing

the infinite lattice into

plaquettes

of different sizes. The uppermost line

corresponds

to the N6el-state

(in x-direction)

and the lowermost line

corresponds

to exact lower bounds calculated

using equation (23).

The interaction

strengths

were chosen

according

to

(25)

and a 5 x 4

plaquette

was used.

z5

30

35

11

40

45

50

55

1-O I-Z 1-4 1-B 1.8 Z-O

A

Fig.

3. Variational

energies

for the

Ising-like anisotropies.

The centre lines show the

energies

obtained for the test state

4~~) by dividing

the infinite lattice into

plaquettes

of different sizes. The uppermost line

corresponds

to the N6el-state (in

z-direction)

and the lowermost line

corresponds

to exact lower bounds calculated

using equation (23).

The interaction

strengths

were chosen

according

to

(25)

and a 5 x 4

plaquette

was used.

values listed in table I.

Finally optimizing

the value of a, we find the widest range of

validity

for small

positive values,

as was to be

expected

since

(6)

has

previously

led to better limits

than

(5).

We have thus achieved our

goal

of

extending

the

proof

of LRO from Am1.67 to

A m 1.47 and from 0 WA < 0.13 to 0 WA w

0.22, closing

30 9b of the

remaining

gap on the

(11)

Ising-like

side and

extending

the scope of the

proof by

70 9b on the KY-like side. Further

significant improvements using

this method seem

quite unlikely,

and

although

we have been able to

slightly improve

the method

itself,

results for the

isotropic Heisenberg

model can still not be

obtained,

even if we insert the numerical estimates for the

nearest-neighbour

correlation functions. As

Kennedy

et al.

[4]

and Nishimori and Ozeki

[10]

have

previously pointed

out, a new method is

required

to treat the

isotropic

case.

Acknowledgements.

We wish to thank the Rechenzentrum der Rheinisch-Westiilischen Technischen Hochschule Aachen for its kind

hospitality during

the numerical calculations. This research was

performed

within the program of the

Sonderforschungsbereich

341

supported by

the Deutsche

Forschungsgemeinschaft.

Appendix.

Dividing

the square lattice into 5 x 5

plaquettes,

we obtain the

following

values

Io

and

T,

which are

required

for the calculation of the energy of the variational test state

~P~ in section 4 :

Io(A)

=

= 383504 A~~ + 1931008 A~~ + 4120288 A + 5074336 A ~~ + 4085352 A ~~ + 2284144 A ~~

+ 911872 A ~~ + 261872 + 53645 A~+ 7640 A~ + 718 A~ + 40 A ~ + l

(42)

7~(A)

=

=

(-

1164068293120 A~~ 9225631229952 A " 32850592375808 " 69738691879936 A~~

98317887695360 A 96181079215104 A~~ 65011188580096 A3~ 27611636833792 A 3~

3621561153088 A ~~ + 4137375844608 A + 3339275955712 A ~~ + 1086767643200 A~~

49682207392 A~~ 247925155392 A~~ 148968844112 A 56118842240 A~~

15451961466 A '~ 3256218376 A '~- 532373904 A '~ 67330632 A

6480956 ~ 459768 A~ 22688 ~ 696 A ~

10)/4

(43) T--(A )

=

= 13156864 A ~~ 50016000 A~~ 79563392 A 72818624 A ~~ 44628544 A~~

20555744 A ~~ 7838816 A ~~ 2554560 A 671096 A~

129016 A~ 16448 ~ 1224 ~

40)/4 (44)

T~_ (A

=

= 4602048 A~~ + 21241088 A ~' + 41202880 A '~ + 45669024 A '? + 32682816 A '~

+ 15989008 A~~ + 5471232 A + 1309360 A~ + 214580 A ? + 22920 A~ + 1436 A + 40 A

(45)

(12)

References

ii]

BEDNORz J. G., MULLER K. A., Z.

Phys.

EM

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188.

[2] DYSON F., LIES E. H., SIMON B., J. Stat.

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18

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335.

[3] JORDXO NEVES E., FERNANDO PEREz J.,

Phys.

Lett. l14A

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331.

[4] KENNEDY T., LIES E. H., SHASTRY B. S., J. Stat. Phys. 53

(1988)

1019.

[5] KuBo K., Phys. Rev. Lett. 61

(1988)

l10.

[6] KENNEDY T., LIES E. H., SHASTRY B. S.,

Phys.

Rev. Lett. 61 (1988) 2582.

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58

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[10] NISHiMORi H., OzEKi Y., J.

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[I ii BARTKOWSKi R. R., Phys. Rev. B S

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OiTMAA J., BETTS D. D., Can. J.

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