HAL Id: jpa-00246359
https://hal.archives-ouvertes.fr/jpa-00246359
Submitted on 1 Jan 1991
HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
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�
Classification
Physics
Abstracis75.10Jm
Extended proof of long-range order in the two-dimensional
quantum spin-1/2 XX2kmodel at T
=
0
Hans-Aloys
WischJnann and Ervin Mfiller-HartmannInstitut ffir Theoretische
Physik,
Universitit m K61n,Zfilpicher
StraBe 77, D-W 5000 K61n 41,Germany
(Received25
January J99J,accepted
JFebruary
J99J)Abs«act. We prove the existence of
long-range
order(LRO)
in theground
state of the 2D quantumspin-1/2
XXZ-model for allanisotropies
0 WA « 0.22 and Am1.47. We achieve this extension ofprevious proofs by developing
animproved
variant of theDyson-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,
whichconsiderably
increased with thediscovery
ofhigh-temperature superconductors ii
]. Due to thelayered
structure of thesematerials,
most of theearly attempts
to describe thenovel
physics
were based on electronic andmagnetic
correlation effects in two-dimensional models. Thesimplest
ofthese,
the Hubbard and theHeisenberg
models have since been theobject
of innumerablestudies,
and theinvestigation
of theground
stateproperties
of thesemodels has outlasted the somewhat naive
hopes
of asimple
electronic mechanism forsuperconductivity.
The most
interesting
and mostextensively
studiedproperty
of theground
state of theantiferromagnetic Heisenberg
model is thedecay
of thespin
correlation functions with distance.Although
much numerical evidence for the existence of aNkel-type antiferromagne-
tic
long-range
order(LRO)
has beenaccumulated,
arigorous proof
for the square lattice is stillmissing.
On the otherhand,
there has beensignificant
progress inhigher
dimensions and for theanisotropic generalization,
the XXZ-model :H
=
£ (S) )+
+St )Y
+AS) )f)
with A m 0,
(1)
(<Jl
where the
exchange
interaction J has been set tounity.
A number of authors[3-6]
extendedthe scope of the
original proof by Dyson,
Lieb and Simon[2]
for theHeisenberg
antiferromagnet
andgeneralized
it to the XXZ-model. In this manner, Kubo and Kishi[8]
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 allAm
0,
as well as for S=
1/2
in the KY-likeregion
0 WA~ 0.13 and the
Ising-like region
A m 1.78.
Ozeki,
Nishimori and Tomita [9] extended thisproof
to Am 1.72. Their
proof
for 0 « A <0.20, however,
is notrigorous
: it uses «variational »energies
which Suzuki andMiyashita [13]
calculated in a verygood
but uncontrolledapproximation
as upper bounds for the energy. The sameenergies
are also used in theproof
for 0 « A « 0.59by
Nishimori andOzeki
[10].
Inaddition,
this last result as well as theproof
for Am 1.10 also contained in
[10],
is based upon the
assumption
that thenearest-neighbour
correlation functions are monotonic functions of thesystem
size. Thisassumption
was verifiednumerically
in[10]
for the10, 16,
18 and 20spin
systems with Oitmaa-Betts[12] boundary conditions,
but we have found that thex-component
of these correlations does not show anymonotonicity
for A=0.8 and A=
0.9 when one includes the 26
spin
system('). Although
this range of A is outside theregion
of interest for theproof,
a doubt is cast on thevalidity
of theassumption,
sincelarger
systems may exhibit this kind of behaviour at smaller values of A. On the otherhand,
theproof
for theIsing-like region
Am 1.67
given
in[10]
isrigorous,
so that the existence of LRO in theground
state of the XXZ-model has been shown for alldimension,
allspins
and allanisotropies
with theexception
ofS=1/2
on the square lattice for theanisotropies
0.13 w A w 1.67.
In this work we present an extension of the above
proofs
to the KY-likeregion
0 w A w 0.22 and to the
Ising-like region
A m1.47,
thusclosing
as much of theremaining
gapas is
possible
with this method. Theimprovement
is achievedby optimizations
on threeaspects
of theexisting proofs
in section2,
wepresent
animproved
variant of theDyson-
Lieb-Simon[2] (DLS) proof,
in section 3 we deriveimproved
lower bounds for the x-component
of thenearest-neighbour spin
correlationfunctions,
while section 4 is devoted toimproved
variationalenergies. 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-thcomponent
of thespins 6j
on a D-dimensionalhypercubic
lattice A(with
itsreciprocal
latticeA*)
and the
positive
semidefinitequantity gl'~
=(S[ S[~)
that satisfies thefollowing
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
thefollowing
values for the 18, 20 and 26spin
systems:(6~S~)~~=-0.13044,
-0,13040, -0,13044 and$~ S~j
~ ~ =
0,12477, 0.12474, 0.12501
In the
thermodynamic limit,
the correlation functions becomeindependent
of the lattice sites R and the bond directions e~, and we obtain(S( S()
=
i~~~
~ g)~~ + lim
( g(~
and(5)
Bz
(2
gr)
A- m
($ S(
=
~~~
~ gj~~
j (
cos p~ + lim
( g(~
,
(6)
Bz
(2 ")
m=i Al -m
provided
thegl'~
are bounded from above for all p #Q. Here, Q
=(gr,
gr,..)
is the wave vectorcorresponding
toantiferromagnetic LRO,
and the second term on theright-hand
sides of(5)
and(6) is, just
the related orderparameter
lim
g(~
= lim~
£ exp(-iQR) Sk I= (ml'~)~ (7)
A
- m
~
A
- m
A
ReA
~
A
rigorous proof
of LRO can thus be obtainedby deriving
a lower bound for the left-hand side and a smaller upper bound for theintegral
on theright-hand
side of either of theseequations.
At thispoint
we remark that we do not have to choose between(5)
and(6),
but can insteadinvestigate
the linear combinationIS Sii
+ «<Si Sol ~z
~/)~ ~i~ la i ~l C°S
Pm +
+
(a
+I)
limg(~, (8)
(Al -m
A(
which reduces to
(6)
for a= 0 and to
(5)
for infinite a. Intiis variant, rigorous proofs
can be obtained for all values a mI,
butnegative
values do notyield improved results,
so that we shallonly
be concemed with a m0 in thefollowing.
The introduction of theparameter
a thus leads to a
family
ofproofs containing
the bestproof
conceivableusing only
site-diagonal
andnearest-neighbour
correlation functions.The
required
upper bound forgl')
wasoriginally
derivedby Dyson,
Lieb and Simon[2]
for theHeisenberg
and the KY-model in three and more dimensions at finitetemperatures.
Neves and Perez _[3] then showed that the two-dimensional
problem
can be treated in thesame manner, as
long
as thezero-temperature
limit is taken before thethermodynamic limit,
whileKennedy,
Lieb andShastry [4] directly
derived the same bounds in the 2Dground
state.These results were
subsequently generalized
to theanisotropic
caseby
Nishimori et al.[7],
who obtained thefollowing
formulas for zerotemperature
in thethermodynamic
limitg(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 cosp~) lxx)
~
2
£ (A
cosp~) (zz)
~ ,
C)~)
= 4lxx)
~
E~
,
m i m =1
(lo)
D D
Ej
=
£ (I+cosp~), E~
=£ (I-cosp~), (11)
m=i m=1
where the
following
abbreviations for thenearest-neighbour spin
correlation functions havebeen introduced :
(xx)~
=(S(Stj(A)
and(zz)~
=
($S()(A). (12)
Inserting
the aboveexpressions
forj)~)
for the two-dimensional case into(8),
we obtain thefollowing
sufficient condition for LRO in thez-component
in theIsing-like region
A m :
~
j- lxx) ~
~~~~4
~4 " 2 A
'~~~"~
~~~~with
where the
«
+» indicates
thatthe
integration is estricted to that part ofwhich the ntegrand
is
positive. imilarly, the ollowing ufficient conditionfor
RO in thejxxj~+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 toreplace h~(a,rj) by h~(a,
I)
=
r~(a )
because theargument jzz )
~ + A
lxx)
4
(1?)
ri "
j xxi
~ + A
jzzj
4
is bounded
by (rj
w I. This caneasily
be verifiedusing
theequations (14a)
and(14b)
of Nishimori et al.[7].
Theseequations
also prove theinequality (zz)~«- lxx)
~
for
0 WA w I which has been used to
simplify
theright-hand
side of(15).
Following
Nishimori and Ozeki[10],
we now transform the above conditions(13)
and(15) using
themonotonicity(2)
of the correlation functions(xx)~m lxx)
for Am I andlxx)
~ m
(xx)
~
for A m 0 as well as variational values for the
ground
stateenergies
per bond : e~(A)
We0(A)
#
2
jXX)
4 ~ A
l~~)
4'
(18)
We
finally
obtain thefollowing
sufficient conditions for LRO in the z-component in theIsing-
like
region
A m I :~y
j- (XX)j.A
~v(4)"4~+2~~~)l~
~
°~2("), (l~)
~2)
Thiscan
rigorously
be shownusing simple
variational arguments.and for LRO in the x-component in the KY-like
region
0 « A «1:~
+ " »
fi r~(
« for « » o
(20)
fi
4-(xx)~
23. Lower bounds on the
spin
correlation functions.In order to be able to make use of these
formulas,
we needgood
lower bounds on thecorrelation functions
lxx) (at
theHeisenberg point)
as well aslxx)
~
(at
theKY-point),
thatcan
evidently
be deduced from lower bounds on theground
stateenergies. Slightly generalizing
anelegant application
of the variationalprinciple
that wasdeveloped by
Nishimori and
dzeki [10],
thesecan in turn be derived
by numerically calculating
theground
state
energies E#( ((y)
of theinhomogeneous
HamiltonianHI
=
£ (y($~ f+
+St fY
+AS) )f) (21)
(;y)
on a finite
plaquette
with openboundary conditions,
where the(j
m0 represent bond-dependant
interactionstrengths. Using
theground
state of thehomogeneous
model on the infinite lattice as a variational test state andtaking advantage
of its translational androtational
symmetry,
we then obtain(H/)
=
£ (~ (2 (xx)
~ + A
(zz ) ~)
mE#( ( (y ) ) (22)
( ,j)
This leads to the desired lower bounds on the
ground
stateenergies
per bond for the infinitehomogeneous
modelEt( jzj1 )
(23)
~°~~~
~z ij
~and
finally
to therequired
bounds on the correlation functions :E(( (/y ) El ( (y) )
( xxi
~ m
and
( xxi
m(24)
2
£ (y
3£ (j
The
remaining
task is tojudiciously
choose the set of interactionstrengths ((j)
so as to maximize these bounds. Since asystematic study
of allpossible
sets is not feasible forlarge plaquettes,
we have used thefollowing
heuristic rule that hasalways
proven toyield
verygood
bounds: for the case of a
plaquette
ofNx by N~ spins,
the interactionstrength
(~
for the bond(ij)
is determined as the functionS(x, Y)
=
Ii
+ C°S1~ i~" Ii
+ C°S1~ i~" 1, (25)
evaluated at the centre of the
bond,
where theorigin
of the coordinate system has beenplaced
at the centre of the
plaquette
and the bondlength
has been set tounity.
We have been able to determine the
ground
stateenergies
ofHI
andH/
with theseinteraction
strengths
on the 5 x4,
6 x 4 and 6 x 5plaquettes using
a modified Lanczosmethod (3). The
resulting
lower bounds on the correlation functions are :(xx)
m 0. II764, 0.11681,
0. II 524 and(26)
(xx)~
m0.14094, 0.14034,
0.13942(27)
respectively.
Thecomparison
of the best obtained bounds with thenumerically
determinedlxx)
correlation functions for the16, 18,
20 and 26spins
systems(using
Oitmaa-Betts[12]
boundary conditions)
infigure
Iclearly
shows that our bound onlxx)
~
is excellent in the KY-
region
andquite satisfactory
in theIsing-like region.
4.
Upper
bounds on theground
stateenergies.
To
complete
theproof,
we now have to derivegood
upper bounds on theground
stateenergies.
For this purpose, we start from the Nkel-stateN)
that haspositive z-components
for thespins
on the A-sublattice and divide the infinite 2D lattice intoequal rectangular plaquettes P,.
We theninvestigate
thefollowing
variational state~P~)
that wasoriginally proposed by
Bartkowskiill]
andsubsequently
studied on 2x2plaquettes by Ozeki,
Nishimori and Tomita
[9]
(~P~)
=fl fl' (I
+ASP S()(N), (28)
P, (<,b)eP,
where
fl'
is restricted to nearestneighbour pairs jab)
with as A and beB,
andA is a real variational
parameter. Furthermore,
the conventions S+ =S~+iSY andS~
=
S~- iSY will be used for the ladder
operators.
Due to the fact that theseoperators
commute
provided they
are on different latticesites,
the calculation of the energy is04
20 18
°6 18
08
~ li
,,
~°
V ,>,e.3,4.5
iz
14
18
o 5 1-o 1.5
A
Fig,
I. Correlation functionslxx)
~
for the 16, 18, 20 and 26 spin systems with Oitmaa-Betts [12]
boundary
conditions(curves) compared
to therigorous
lower bounds(xx)
~
and
(xxi (straight lines).
The inset shows the XY-like
region
on anexpanded
scale.(3) For the 6 x 5
plaquette,
one Lanczos step consumedapproximately
10 minutes CPU time on one processor of anIBM-3090-6005/VF,
and 35 steps were necessary to achieve convergence.straightforward
and leads toev
(A)
=
£ £ (If-
+
AIl$)/Io
+£ £
'(AII I])/Ii (29)
ab)e P (<,b
Here M is the number of
spins
perplaquette
and£'
is restricted to nearestneighbour pairs jab
with a ePi
and b e(P~
UP~),
whereP~
is theright
and P~ is the upperneighbour
ofplaquette Pi.
The introducedexpectation
values I can beexpressed
asIo(A
=(~P([ ~P() (30)
1](A )
=
(~P([S[[ ~P() (31)
1(~_ (A
= ~P
([ St Sp
+Sp St
~P() /2 (32)
I~(A
=
(~P([ S( S([ ~P() (33)
with the
help
of~P()
=fl' (I
+ASP St ) [fir)
,
(34)
jab)eP
where
fir) represents
theconfiguration
of thespins
onplaquette
P when the infinite lattice is in the Nkel-state)N).
As we shallshow,
an evaluation of these formulas leads to verysatisfactory
variationalenergies
for theIsing-like anisotropies
AmI,
even if the lattice is divided into very smallplaquettes.
It thus appearsamazing
that this test state isseldomly
used for the KY-likeanisotropies.
For 0 WA w I it is of courseadvantageous
to renumber thecoordinates in the Hamiltonian
(I)
andstudy
theequivalent
formji
=
£ (AS/ f~
+Sf fY
+S) f~) (35)
(;j)
=
£
~(St )+
+S/ ()
+£
~ ~($+ §
+Sj )+ )
+S) )~ (36)
j,~~ 4
;~j 4
We have calculated the energy
i~ (A )
of the test state ~P~ withrespect
toji. Noticing
thatthe first sum in
(36)
does not contribute because it does not preserve the zcomponent
of the totalspin,
we obtain :iv (A)
=
~j £ ((A
+ II~t_ /2
+Ijf)/Io
+£ £' (Ii If)/Ii (37)
jabje P jab>
Denoting
the sums of theexpectation
values Iby
j~_
£, ~a~b
j~£
~ab j~£
~ab(3~)
z z z, zz zz, + + ,
(<,b) (ab)E P jab )EP
the variational
energies
canfinally
beexpressed
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 tosymbolically
evaluateIo
and the sums T for the caseof 2 x
2,
3 x3,
4 x 4 and 5 x 5plaquettes.
The details can be found in[14],
and the results for the 5 x 5plaquette
aregiven
in theappendix.
Thesubsequent
numerical minimization of theenergies
withrespect
to A for 201equally spaced anisotropies
in the range 0 WA w 2 thenprovided
us with therequired
upper bounds on theground
state energy.We were able to further
improve
these valuesmainly
in thevicinity
of theHeisenberg point by investigating
thefollowing generalization
of the test state*i)
"
fl C~P(~
'l(Nil Nil))' n' (I
+ASP St ) l~>
,
(41)
P, (ab)eP,
where
Nl'/
andNl'i~ represent
the number ofparallellantiparallel neighbouring spins
on theplaquette P;.
Theoriginal
test statecorresponds
toY~ =
0,
andY~ = 0.03 leads to
slightly
better variational
energies
for allanisotropies
whereasY~ =
0.06 leads to
slightly
worsevalues. Since the
improvement
is so small that the scope of theproof
is notextended,
we refrain fromwriting
down thecorresponding
sums T. Theenergies
forY~ = 0.03
have, however,
been used indetermining
the bounds of table I and have been included infigures
2 and 3 which present the variationalenergies
for the KY-like and theIsing-like regions.
It is evident from thesefigures,
that we have been able toconsiderably improve
the variationalenergies
over the whole range ofanisotropies.
Table I.
Limiting
valuesA~,~(a) for rigorous proofs of
LRO in the z-component andA~~~(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
theimprovements
that werepresented
in thepreceding
threesections,
we arenow able to extend the scope of the
proof
of LRO. In section 3 we derived a lower bound oflxx)
m 0.11524 on thex-component
of thenearest-neighbour spin
correlationfunction,
which should becompared
to the boundlxx)
m 0.11895 derivedby
Nishimori and Ozeki[10]
and to thenumerically
obtained value oflxx)
m 0. I1167.
Inserting
our bound into theoriginal proof already
extends itsvalidity
from Am 1.67 to A m 1.61.
Adding
thesignificantly improved
variationalenergies
we calculated in section4,
theoriginal proof
becomes valid for allanisotropies
A m 1.52 and 0 w A w 0.19.Numerically evaluating
theintegrals r~(a)
andinserting
the lower boundlxx)
~ m 0.13942 we derived in section
3,
the variant of the DLS method which we derivedin section 2 then leads to
proofs
of LRO in thex-component
for allanisotropies
0 w A «
A~~~(a )
and in thez-component
for allanisotropies
AmA~~(a
with thelimiting
24
z6
11
2830
32
0 Z 4 6 8 1-O
1i
Fig.
2. Variationalenergies
for the XY-likeanisotropies.
The centre lines show theenergies
obtained for the test state 4~~) by dividing
the infinite lattice intoplaquettes
of different sizes. The uppermost linecorresponds
to the N6el-state(in x-direction)
and the lowermost linecorresponds
to exact lower bounds calculatedusing equation (23).
The interactionstrengths
were chosenaccording
to(25)
and a 5 x 4plaquette
was used.z5
30
35
11
4045
50
55
1-O I-Z 1-4 1-B 1.8 Z-O
A
Fig.
3. Variationalenergies
for theIsing-like anisotropies.
The centre lines show theenergies
obtained for the test state
4~~) by dividing
the infinite lattice intoplaquettes
of different sizes. The uppermost linecorresponds
to the N6el-state (inz-direction)
and the lowermost linecorresponds
to exact lower bounds calculatedusing equation (23).
The interactionstrengths
were chosenaccording
to(25)
and a 5 x 4plaquette
was used.values listed in table I.
Finally optimizing
the value of a, we find the widest range ofvalidity
for smallpositive values,
as was to beexpected
since(6)
haspreviously
led to better limitsthan
(5).
We have thus achieved our
goal
ofextending
theproof
of LRO from Am1.67 toA m 1.47 and from 0 WA < 0.13 to 0 WA w
0.22, closing
30 9b of theremaining
gap on theIsing-like
side andextending
the scope of theproof by
70 9b on the KY-like side. Furthersignificant improvements using
this method seemquite unlikely,
andalthough
we have been able toslightly improve
the methoditself,
results for theisotropic Heisenberg
model can still not beobtained,
even if we insert the numerical estimates for thenearest-neighbour
correlation functions. As
Kennedy
et al.[4]
and Nishimori and Ozeki[10]
havepreviously pointed
out, a new method isrequired
to treat theisotropic
case.Acknowledgements.
We wish to thank the Rechenzentrum der Rheinisch-Westiilischen Technischen Hochschule Aachen for its kind
hospitality during
the numerical calculations. This research wasperformed
within the program of theSonderforschungsbereich
341supported by
the DeutscheForschungsgemeinschaft.
Appendix.
Dividing
the square lattice into 5 x 5plaquettes,
we obtain thefollowing
valuesIo
andT,
which arerequired
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)
References
ii]
BEDNORz J. G., MULLER K. A., Z.Phys.
EM(1986)
188.[2] DYSON F., LIES E. H., SIMON B., J. Stat.
Phys.
18(1978)
335.[3] JORDXO NEVES E., FERNANDO PEREz J.,
Phys.
Lett. l14A(1986)
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.[7] NISHIMORI H., KuBo K., OzEKI Y., TOMITA Y., KISHI T., J. Stat.
Phys.
SS(1989)
259.[8] KuBo K., KISHI T.,
Phys.
Rev. Lett. 61(1989)
2585.[9] OzEKI Y., NISHIMORI H., TOMITA Y., J. Phys. Soc.
Jpn
58(1989)
82.[10] NISHiMORi H., OzEKi Y., J.
Phys.
Soc. Jpn 58(1989)
1027.[I ii BARTKOWSKi R. R., Phys. Rev. B S
(1972)
4536.[12]
OiTMAA J., BETTS D. D., Can. J.Phys.
56(1978)
897.[13] SuzuKi M., MiYASHiTA S., Can. J.
Phys.
56(1978)
902.[14] WiSCHMANN H.-A., Thesis,