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Theory of mott transition : Applications to transition metal oxides
M. Cyrot
To cite this version:
M. Cyrot. Theory of mott transition : Applications to transition metal oxides. Journal de Physique,
1972, 33 (1), pp.125-134. �10.1051/jphys:01972003301012500�. �jpa-00207204�
125
THEORY OF
MOTTTRANSITION :
APPLICATION S
TOTRANSITION
METALOXIDES
M. CYROT
Institut
Laue-Langevin,
Cédex156, 38-Grenoble-Gare,
France(Reçu
le 22 juin 1971, révisé le 26 août1971)
Résumé. 2014 En utilisant le modèle de Hubbard, nous étudions la transition métal-isolant due aux
corrélations entre électrons. Nous ne tenons pas compte des fluctuations de charge mais seulement des fluctuations de spin qui créent sur chaque site un moment magnétique. Cette simplification per- met une analogie avec les alliages binaires. A température nulle, nous obtenons successivement un
métal non magnétique, un métal antiferromagnétique et un isolant antiferromagnétique lorsque le rapport U/W croît (U interaction entre électrons, W largeur de la bande). Ceci est dû, en accord avec
les idées de Slater, à la partie dépendante du spin du potentiel self consistent. De la même manière
qu’il est possible à température nulle d’obtenir une solution antiferromagnétique de plus basse énergie, nous obtenons au-dessus de la température de Néel une solution avec des moments désor- donnés sur chaque site. Pour de grande valeur du rapport U/W le système reste isolant au-dessus de la température de Néel. Pour des valeurs intermédiaires de U/W, la frontière entre métal et isolant
paramagnétique montre que la phase isolante est favorisée à hautes températures a cause de l’entrc-
pie de désordre. Nous donnons un diagramme de phase schématique pour le modèle de Hubbard et nous discutons l’application de la théorie aux oxydes de métaux de transition.
Abstract. 2014 We study the metal-insulator transition due to correlations between electrons using a
Hubbard model. Neglecting fluctuations in charge, we only take into account fluctuations in spin density which build up magnetic moments on each site. A close analogy with binary alloys follows
from this. At zero temperature, with increasing value of the ratio of the interaction between electrons U to the bandwidth W, we obtain successively a non magnetic metal, an antiferromagnetic one and an antiferromagnetic insulator. This is due, as in Slater’s idea, to the exchange part of the self consis- tent potential which cannot have the full periodicity of the lattice. As it is possible to find a solution
with lower energy and with antiferromagnetism to Hubbard hamiltonian, one can construct a self
consistent solution with random but non zero moments on each site. The alloy analog of the metal insulator transition is band splitting. For large values of the ratio U/W, the material remains insulat- ing through the Néel temperature. For intermediate values, the line boundary between a Pauli metal and a paramagnetic insulator shows that the insulating phase is favoured at high temperature because of the entropy disorder. We draw a general schematic phase diagram for the Hubbard model and we
discuss the relevance of the theory to transition metal oxides. The main qualitative features are
consistent with our theory.
LE JOURNAL DE PHYSIQUE TOME 33, JANVIER 1972,
Classification Physics Abstracts :
17.26
Insulator metal transitions are a
phenomenon
which have been known for
quite
a while in a widevariety
of systems : metal vapourliquid
system(mer- cury)
metal ammonia solutions, disordered systems(impurity bands),
transition metalchalcogenides.
Inthe last few years there has been considerable interest in transition metal oxides. These oxides form a very
interesting
class of materials[1].
Their electricalproperties
range from verygood
insulator to verygood
metal. Some of them have an intermediate behaviour and can exhibit a metal-insulator transition with temperature, pressure, ordoping.
Besides
pratical
interest due topossible applica-
tions to switches these oxides are of fundamental interest. This stems from the fact they prove to be a
striking
failure for the elementary Bloch-Wilsontheory.
It is well known that a metal whose band areeither
completely
full orentirely
empty must be aninsulator. While it is
possible
on the basis of the Bloch-Wilsontheory
to account for metallic behaviour in systems with an even number of electrons per unit cellthrough
bandoverlap,
it is notpossible
toexplain
an
insulating
behaviour when the number of electrons per unit cell is odd.Among
theinsulating
oxides arecompounds
which on these basis should be metallic.Mott
[2]
was the first to observe these facts on nickel oxide. For these materials heproposed
to abandonBloch model. The
starting point
would be a localizedground
state wave function or Heitler London onewhich has the immediate
advantage
ofexplaining
theinsulating
behaviour. The reason lies on the fact that if the band is very narrow you do not lose a lot of kinetic energyby localizing
theelectrons,
so an insu-lating ground
state is then favourable. However, asthe atoms are
brought together
the cost in kineticenergy in
confining
electrons to the atomic sitesArticle published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01972003301012500
becomes
larger
until it starts to exceed therepulsion
energy
gained.
At thispoint
the metallic state haslower energy and an insulator metal transition occurs.
A
particularly interesting
feature of theinsulating
materials which are not
explained
in a Bloch-Wilsontheory
is that they appear to bemagnetic. For instance,
this is the case of many mono-oxides of transition metal. The
insulating
behaviour of these materialsseems to be
strongly
connected withmagnetism.
Atthis
point
it seems worth while to define what weshall call a Mott insulator and a Mott transition because a
large
number of materials exhibit a metal insulator transitionalthough
some of them are non-magnetic
in theinsulating phase.
Ingeneral
these non-magnetic
materialsundergo
a latticephase change
which is associated with the
insulating
behaviour.Although
one can argue about the nature of thedriving
force which induces the lattice
phase change,
we willnot label it a Mott transition. We reserve the word Mott insulator for
insulating
materials which arenot
explained by
a usual Bloch-Wilsontheory and,
webelieve,
arealways magnetic.
A Mott transition is atransition from a metallic state to a Mott insulator.
Although
it is now some twenty years since Mott’soriginal proposal,
and there exists a considerable amount of theoretical work, there is, as yet, no satis-factory microscopic theory
of the Mott transition. In hisoriginal
article Mottargued
that the transition is due to correlations between electrons. We shall restrict our-selves to this
point
of viewalthough
other mechanisms[1]
can bethought
of. The occurrence of antiferro-magnetism
in these insulators is asign
that correla- tionsare probably primarily responsible
for the observedfacts. So the
only
articles we willrefer to, will
discussthis
point
of view. In this frame, most of the theoreti- calanalysis
has started with a model hamiltonian introducedby
Hubbard[3].
In this model a localizedor Wannier
representation
is chosen for the electronicwave function. The hamiltonian consists of two terms,
one represents the
tunelling
of electrons from onesite to its
neighbours
and the other therepulsion
energy U when two electrons are on the same site.
Ci:
is the creation operator for an electron ofspin
Qin the atomic state at the ith lattice site.
Tij
is thematrix element of the electron transfer between the states at the ith site and
jth
site and nia =Ci: Ciu.
In the atomic
limit,
i. e. forlarge
value ofUlTij
and for a
single
half filled band, there will be an elec-tron localized on each site and the system will be a Mott insulator. In this limit there is an antiferroma-
gnetic coupling
energy between the local moments due to Anderson kineticexchange.
Thus at low tempera-ture the system is
antiferromagnetic
with a Néel temperaturekTN N zTijlU.
However, the system isinsulating
both above and below TN. AsTijlU
isincreased, the hamiltonian becomes very difficult to
solve and there are no exact results. Considerable
amount of work has been done and we shall not quote all of them
[4].
The main result is due to Hubbard[3]
who used a Green function
decoupling
scheme andcompletely neglected magnetic ordering.
Within hisapproximation
an insulator to metal transition withno
discontinuity
in the number of free carriers, occursas
zTi,IU
goesthrough
a critical value of 1.15. Manyimprovements
of this solution[4]
have been tried andmany discussions appear. Nonetheless it is not clear that this is the correct result for the Hubbard hamil- tonian.
In any case there are some
problems
linked withHubbard’s solution. First it does not take into account
magnetism. Secondly
itcertainly
is incorrect for the metallicphase
since it does notproperly
describe the Fermi surface[5], [6].
Further a temperature induced transition is a rare accident sinceonly change
inlattice parameter can drive a
phase
transition as in Mott’soriginal
idea.Here it is worthwhile to mention Brinkman and Rice’s
approach [7]
to the metal non-metal transition, which used Gutzwiller’s variational method[8]
oftreating
the Hubbard Hamiltonian to obtain a nonmagnetic
solution whichproperly
describes the metallicstate. The results obtained are to be contrasted with those found
by
Hubbard : The effective masse becomeslarge
as the correlation increases when Hubbard’sapproximation
leads to adensity
of states at the Fermilevel
approaching
zero.In
parallel
to this line of workfollowing
Hubbardthere exists another
important
onefollowing
Slater’sidea. Slater
[9]
firstpointed
out that if a metallicmaterial is
antiferromagnetic
the effective self consis- tent Hartree-Fockpotential
which acts on an electroncannot have the full translational symmetry of the lattice. The
exchange
part of thepotential
must havethe double
periodicity
of the sublattice. The first Brillouin zone of the lattice is divided in half and theexchange
energy introduces bandsplitting
at the newfaces of the reduced subzone. If the
exchange
energy islarge
or if theoriginal
nonmagnetic
band is narrowthis
splitting
could introduce a real gap in thedensity
of states and thus
produce
an insulator instead of ametal. We must
emphasize
that we obtain an insulatoronly
in the orderedmagnetic phase.
Above the Néel temperature the material becomes metallic. This transi-tion,
that we shall call a Slatertransition,
lies interme- diate to a usual Bloch-Wilson one and a Mott one.The
insulating
behaviour isexplained
in a Bloch-Wilsontheory
if one takes into account Hartree-Fock poten- tial. Des Cloizeaux[10]
made aparticularly
detailedstudy
of this transition. Let usemphasize
that there isnot one Hartree-Fock solution. There exists an infi- nite number of solutions to the Hartree-Fock equa- tion which are non linear. Des Cloizeaux studied a
particular
set of Hartree-Fock solutions and deter- mined that at T = 0 theantiferromagnetic
state lieslower than the
paramagnetic
state.127
Just in the same way that it was
possible
to find a lower energy solution to the Hartree-Fockequations
for anantiferromagnet
it should bepossible
to have a selfconsistent solution with random but non zero moments on each site above the Néel temperature.
Depending
on the
strength
of these moments the material could be metallic orinsulating.
In thefollowing
we willshow that such a solution is in fact
possible.
In themetallic
phase
such moments can build upgiving
for instance deviation to Pauli
susceptibility.
For acritical value of these moments the band is not stable and electrons localize on each site. The material
undergoes
a metal insulator transition. We willdevelop
the
theory
of this new type of insulator.Essentially
it is a
magnetic
insulator and itsproperties
areconnected with
magnetic
disorder.Our
theory
is based on a Hubbard hamiltonian which we believe to contain all thegeneral physical
features of the
problem.
Interactions between electronscan lead to fluctuations in
charge density
and fluctua-tions in
spin density ;
we willcompletely neglect
theformer and take into account
only
the latter. So inter-actions can build up
only magnetic
moments on eachsite. Our
approach
is a self consistent one anddevelops
a close
analogy
with thetheory
ofalloys.
The resultsare summarized
by
thegeneral phase diagram
of thefigure given
in part VI. Forincreasing
value ofU/W ( W
bandwidth),
we obtain at zero temperature the succession of threephases :
nonmagnetic
métal,antiferromagnetic
metal andantiferromagnetic
insu-lator. At finite temperature, for
large U/W
thephase
remains
insulating
afterbecoming paramagnetic.
Thephase boundary,
in the temperature versusU/ W plane,
between the metallic and theparamagnetic insulating phases
presents anegative slope
and endsat the critical
point
fordecreasing
value of the ratioU/W.
. In part 1 we
develop
thegeneral theory
and ananalogy
withalloys.
Part II is devoted to the very low temperatureregion.
In part III westudy
themetallic state and
particularly
discuss the appearance ofmagnetism.
Part IV is concerned with theinsulating phase.
The results are summed up in part V and we draw thegeneral phase diagram
that one expects for the Hubbard hamiltonian. The relevance of thetheory
to transition metal
compounds
isfinally
discussed in the last part.I. General formulation. - As we
emphasized
aboveit seems
likely
that correlations between electronsplay
the
important
part in the transition. So wecompletely neglect
the former and use a Hubbard hamiltonian which rests on thefollowing
twohypotheses
- intra-correlation effects
only
are effective between electronssitting
at the same time on the same atom - one candefine an average effective correlation energy U which
gives
the average energy difference betweenpairs
ofsuch electrons with
parallel
orantiparallel spins.
Itfavours
parallel spins.
These statements recover ofcourse some difhculties
arising
from thedegeneracy
of the d band but as a start we will use the
simple
Hubbard hamiltonian.
Here we will restrict the
analyses
tothermodynamic properties
and calculate the free energy. We want to show that within this band hamiltonian the free energycan have the behaviour of bound electrons : i. e.
gives
a Heitler-London behaviour. So our main pro- blem is to calculate thepartition
function definedby
Let us now set up our
approximation.
Correlations between electrons can lead to fluctuations incharge
and fluctuations in
spin.
Aparticularly interesting
way
[11]
to separate both effects is to rewrite the last term of the hamiltonianIn our model we will
completely neglect
fluctuations ofcharges.
In the metallic case, this seems reasonableas Coulomb
repulsion
inhibits fluctuations. In theinsulating phase
the number of electrons on a site isessentially
constant. So we will assume that the lastterm of equation (3) equals U/4
and we will takeinto account
only
fluctuations inspin.
In
appendix
A we recall how thepartition
functioncan be written in a functional
integral
form as firstpointed
outby
Hubbard[12].
The main interest of this formulation is to eliminate thetwo-body potential
and to
replace
itby
a timedependent
localized fieldacting
on any site i. The drawback of thissimplifica-
tion which
permit
us to treat asimple
hamiltonian is that we have to average over all these fieldsweighted by
agaussian
factor.Where T, is the
ordering
operator for the time « s ».2
mi, is a kind of effectivemagnetic
moment on site i.(Cf. appendix B.)
At this
point
we introduce the secondimportant approximation
of this paper. Weneglect
the « timedependence
of these effective moments, i. e. we aredealing only
with Schrieffer’s staticapproximation [13].
This
approximation gives
the exact result in the twolimiting
cases, U = 0 and7
= 0 andgives
a smoothinterpolation
between them. We think that thephysical
results are contained within this
approximation
whichis valid any time fluctuations are
unimportant.
Webelieve this is the case in the
following
exceptperhaps
when we discuss the
properties
of the metallicphase.
Now we have to solve
essentially
the same hamil-tonian as Anderson
proposed
in hisstudy
of localiza-tion in a random system
[14].
The hamiltonian is for one
spin
direction(with
aslight change
of zeroenergy).
Ili is a random
potential.
Theonly
difference is that electrons ofspin
up and down do not see the samepotential
but anopposite
one.To calculate the
partition
function we introduce inthe usual manner a
coupling
constantni,, > is
given by
the one electron thermal green function atequal
time in the presence of the wholeIn the absence of the random moments Mi we have
Introducting
theexplicit
notation :Gij(e),, ;
p i , M2, - - -,lln)
it is
straight
forward to show thatThe
partition
function in presence of the set{ /li }
canbe written.
We transform the sum to an
integral
in the usual wayand obtain the
partition
function in the formn (a) ;
fl1, ..., Mi = 0, ...,y.)
is the localdensity of states
at
point
i when Mi = 0. It isinteresting
for thefollowing
to introduce the
phase
shift[15] tl’,(co)
due to thelocalized
potential - 2 U,u
i in presence of the other momentsyj j
0 iAmi
is thechange
in energy due to theperturbation - 2
U,ui. Ingeneral
it isimpossible
to calculate thefunctional
integral.
IfF({ jui ))
isstrongly peaked
forsome value of the
set f J.li }
we canapproximate
thefree energy of the system
by
the free energy for thisparticular
set. Thisapproximation
isequivalent
to theusual self consistent
approximation.
Thisparticular
set is determined
by
minimization ofF({ J.li ))
withrespect to the effective moment
Where we used the fact
i. e.
These
equations
16 are the self consistentequations
ofour
problem.
Of course ni, > is a function of thewhole
set {J1i }
but inprinciple
this set ofequations
determines J1i i = 1, 2, ... The
procedure
we used is theusual one which
gives
a self consistentapproximation.
Equation
16 could have been deduced at once fromequations
1 and 3using
a Hartree-Fock factorization.We
preferred
to use arelatively
morecomplicated
formalism which has the
advantage
ofleading directly
to the
thermodynamical quantities
that astudy
ofphase
transitionsrequire.
Inparticular
the entropyterm comes out of the
theory
contrary to asimple
Hartree-Fock’s one.
From
equation
12 we see that F is an even functionof all J1i. So if we have a
particular
set which mini- mizes F all sets where wechange
thesign
of onemoment minimize F. When all the sites can be considered as
equivalent J1i
isindependent
of site iand we have J1i = ± J1. As a result our
problem
reduces to an
alloy
one. Theonly
difference is that J1 must be determined selfconsistently
but we canrest very
heavily
on known results foralloys [16].
Many
general
conclusions can be drawn at thispoint.
At low temperature when J1 is different fromzero there is
magnetic
order. Thishappens
as we willshow for not too small value of
U/W (W band width).
For one electron per atom the
phase
is antiferroma-gnetic
and ourproblem
reduced to an orderedalloy
129
one. Our results are
essentially
similar to Slater’sones
[9]. When Up
islarge enough
the bandsplits
and we obtain an insulator. This will be discussed in Part III.
The most
interesting possibility
of this model lieson the fact that we can also describe a
magnetically
disordered insulator. In our
analogy
asplit
bandlimit can occur in a disordered
alloy.
This rests onthe well known localization theorem
[16]
foralloys.
For a
binary alloy
of the typeconsidered,
the energy levels lie within the energy bands of the pure metals.For the disordered
alloy
thedensity
of states is zeroin no interval within these bands. In our case the
split
band limit is
equivalent
to an insulator. We will show that forlarge
ratioU/W
the entropy disorder favourslarge
Up which leads to bandsplitting.
Sowhatever the temperature, i. e. in the ordered or disor- dered state we obtain an insulator for
large U/W.
If we associate band
splitting
and appearance of aninsulating phase
our criterion for the transition to adisordered
insulating phase
is MU = W. However if for the orderedphase
this assimilation iscertainly
true, for the disorderedphase
thepossible
existence oflocalized states within the band makes this criterium
an upper limit. We will discuss this
possibility
in thetheory
of theinsulating phase (part V).
II. Very low température région. - At zero tempe-
rature many
simplifications
occur. One canalways
assume
perfect ordering
ifmagnetism
exists and the hamiltonian becomesperiodic.
Thus the interest of a detailedstudy
of this case stems from the exact calcu-lations that one can
perform.
Some studies have beendone
[10]-[17]
underassumptions
which areequivalent
to ours at zero temperature. So our results are
formally
similar to those of these authors. However we
give
there another range of
validity.
The hamiltonian forone
spin
direction is :Il must be determined
by
the self consistentequation
16.In
equation
17 we have assumed anantiferromagnetic
order
and p
is half areciprocal lattice
vector.Except
in
special
case we obtain two critical values for the ratioU/W.
Below the first one nomagnetism
occurs, i. e. the self consistent solution ofequation
16 isIl = 0. For intermediate value of this
ratio,
one obtainsan
antiferromagnetic
metal and forlarge
value anantiferromagnetic
insulator because a gap opens up in thedensity
of states[16].
Hamiltonian
[17]
iseasily diagonalized using
apairing
of states k and k + pand we obtain the
eigen
energythe self consistent
equation
whichdetermines y
becomes
n is the Fermi function at zero temperature.
The sum is
performed
on themagnetic
Brillouinzone i. e. a reduced zone.
Equations
18 and 19 aresimilar to those of reference
[17].
In reference[17]
and
[8]
the energy associated with this solution has been calculated in one dimension to compare it with the exact solution of Lieb and Wu[19]
on the Hubbard hamiltonian in this case. One finds a reasonable agreement and this resultjustifies
somewhat ourassumption
ofneglecting density
fluctuations.Let us remark that one has to be careful when
using
a
simple tight binding approximation
for ek. For a band in asimple
cubic orbody
centered cubic onehas :
Equation
19 shows that theinsulating
behaviourappears with
magnetism.
As theright
hand si de ofequation
20diverges for J1
= 0, we find that theground
state is
antiferromagnetic
andinsulating
even for Uinfinitesimally
small. Ingeneral
a finite value of Uis
required
to obtainantiferromagnetism.
U must beequal
to 2J1jxp
where X, is thesusceptibility
for wave vector p. When the ratioUj
W islarger
than a secondcritical value a gap opens up in the
density
of states.For F. C. C.
crystal
withferromagnetic
IIIplane
stacked
antiferromagnetically
thishappens
forWe also notice that this
description permits
in a bandmodel localized
magnetic
moments with nonintegral spin
even in theinsulating phase.
Fromequation
20one can
verify that y
isequal
to the atomicmagnetic
moment
only
in the limitFormula 20 can be
easily generalized
at finitetemperature. For a
simple
cubic we have :But we must
emphasize
that we have assumed atthe
beginning
anantiferromagnetic
order. So thisequation
isonly
valid at low temperature when thelong
range order is notdestroyed
i. e. for temperature smaller than the Néel temperature. Even in this caseequation
21 isapproximate
because some electrons areexcited and we obtain disorder. It is not
possible,
within this
simple
calculation, to deduce from equa- tion 21 a Néel temperature or a temperature for a metal insulator transition. Thecoupling
betweenmoments must be calculated in order to obtain the
Néel temperature. We will do
this,
both in the metallic andinsulating phase,
and will compare the free energy of the differentphase.
It is our main difference with thequoted
reference. Inparticular
we will not findany metal insulator transition for
large
value ofU/W ;
the system is
always insulating
in anantiferromagnetic
or
paramagnetic phase.
III. Theory of metallic
phase.
- In this part wewant to
investigate
themagnetic properties
of themetallic
phase.
This isparticularly important
fordrawing
thegeneral phase diagram
andcalculating
the Néel temperature. We have
just
shown that the metallicphase
can bemagnetic
or nonmagnetic
atlow temperature. For low value of
U/ W
thephase
isnon
magnetic.
This remains true at all temperature and thephase
has the usual Paulisusceptibility.
Whenthe low temperature
phase
ismagnetic
and metallic there are twopossibilities
for the apperarance ofmagnetism
withdecreasing
temperature. In the firstone the non
magnetic phase
becomesantiferromagne-
tic below a temperature
TN.
In the second one loca-lized moments appear in the non
magnetic phase.
These moments interact
through
a Ruderman-Kittel interaction which make them ordered at a critical temperature TN. We calculate that these localized moments are stableonly
below a temperatureTL (TL> TN).
We get
successively
these two different behaviours forincreasing
value ofU/ W. They correspond
to afirst and to a second order transition. We have
already applied
thistheory [21]
to discuss transition metal and toemphasize
that aHeisenberg
behaviour canstem from a band model much of the discussion is still valid.
To illustrate these different behaviours let us go back to
equation
12 and assume for the moment thatwe can
neglect
all term which connect the local fieldon different sites that is :
M(û))
is thedensity
of state of hamiltonian(6)
whenthe whole
set { Mi 1
isequal
to zero. We evaluate the functionalintegral (11) by
means of the saddlepoint
method if there is a
deep
minimum for the functionFl.
This function is even and forlarge
value of T,Fl(p,)
has asingle
minimum at theorigin
so that state/li = 0 is most
heavily weighted.
For T smaller thanTL
there rise twosymmetrical
minimum ± po corres-ponding
tospin
up andspin
down. Thesusceptibility corresponding
to these tworegimes gives
from a Paulilaw to a Curie law with a temperature
dependant
moment
[13].
The temperatureTL
isgiven by
One can see that
TL
is zero forU/
W smaller than acritical value which
depends
on theshape
of the band.We recall that this formula is
only
valid in the metallicstate i. e. for not too
large
value of the ratioU/W.
Within the static
approximation
thevalidity
ofthis one site
approximation
can be discussedby
consi-dering coupling
between localized moments. The nextapproximation
toequation
10 is[13] :
In fact it is easy to show that one can write :
where the ratio of two successive terms is small.
When
Fl(p,)
hast wosymmetric
minimum ± po wecan
approximate Mi
and pj, in the smallerquantity
F2by
po ui and lio uj with u, = ± 1, uj = ± 1 andneglect
all interactions of order greater than two.One can write
The Fourier transform of
J,j
isgiven by
We obtain a Ruderman-Kittel like interaction between localized moments. Thank to it we will get a transition
to a
magnetic
ordered state indecreasing
temperature.When the ratio
Ul
W is notlarge enough
it is unfa-vorable to create localized moments in a
magnetically
disordered state. However it can be worthwhile to create ordered localized moments because of the energy
gained by magnetic ordering.
That is T,equal
the transition temperature to the ordered
magnetic phase TN.
To show this
possibility
wealways neglect
interac-tion of order greater than two and we restrict, in the calculation of the
partition function,
tovalue Pk
= YUk, uk = ± 1. Then we look at minimum ofF,
+ F, asa function of y. The sum over Uk leads to the free energy of an
Ising
modelY(p)
with interactiongiven by equation
27.This
integral
can be doneby
a saddlepoint
method.One obtain a non zero value
of J1
if the energy needed to create a localized moment is less than the energy131
gained by magnetic ordering.
Increating directly
ordered moments we obtain
magnetism
for a lowervalue of
U/ W
than thatgiven by equation (23).
For the
special
case of aparabolic density
of stateswe can
apply
our results.Equation
23gives
for theexistence of localized moments in a disordered state
a minimum ratio of
U/ W
of 3nl 16
= 0.59.Taking
into account the energy
gained by magnetic ordering
this ratio becomes of the order of 0.24. So we obtain the
qualitative diagram
offigure
1.FIG. 1. - Schematic phase diagram for the metallic phase. The dashed curve does not represent a phase transition but the
temperature below which localized moments are stable.
IV. The
insulating phase.
- In the usualtheory
an insulator is a material whose band are either com-
pletely
full orentirely
empty. Mott was the first topoint
out that another type of insulator can exist.It is
typified by
an array ofhydrogen
atoms in theatomic limit. Electrons are localized on each site
although
in a Blochtheory
one obtains a half filled band. So this type of insulator isonly
due to correla- tion and ismagnetic.
In the ordered
phase
agreement between these twotypes occurs because the
superimposed exchange
fielddue to
antiferromagnetism splits
the first Brillouinzone. Slater’s
description
with Bloch wave functions isequivalent
to Mott’s with a Heitler-Londonground
state. Our results of part II illustrate this
point.
Slater’sidea seems
simpler
to deal with and toexplain
nonintegral spin
in theinsulating phase
but ismisleading
in the sense that it suggest
incorrectly
that thecrystal
will show metallic
conductivity
above the Néel tempe-rature.
Mott
description
has theadvantage
ofpermitting
aparamagnetic
insulator but is very difficult to set upmathematically.
We will show that ourformalism,
which
developed
ananalogy
with analloy
and whichgave
physically
the same result as Slater’s idea in theordered
phase,
can be extended to deal with theparamagnetic
case. The formulation is different from Mott’s but it lies on the samephysic
andpermits
effective calculation.
In part 1 we
developed
ananalogy
withalloys
because the
magnetic
moment on each site acts as alocal
potential.
So we canapplied
known results onthis
problem.
As wequoted
above the localization theorem forbinary alloy gives
an exact criterium fora
split
band which isequivalent
toinsulating
behaviour.We obtain the
split
band ifThis
important inequality
means that we get insu-lating
behaviour for agiven
moment when U islarge enough. As y
has a maximum value which isgiven by
Hund’s
rule,
there is a minimum value of U below which noinsulating phase
can appear. This remark will be used in thefollowing.
Up
to now we have associated bandsplitting
andappearance of an
insulating phase.
This iscertainly
true for the ordered
phase
butprobably
wrong in the disordered one. This stems from the fact that it isnow
generally
believed that a continuousdensity
oflocalized states can exist in a disordered system. If the Fermi level lies within these states it does not define
a metal but rather an insulator. In our case the loca- lization theorem does not say
anything
about thenature of the states localized or extended
throughout
the lattice. Before band
splitting,
the states at theminimum of the
density
of states which occurs in themiddle of the band may be localized. So we would get an
insulating
behaviour with a Fermi level located in the middle of the band. Anderson[22]
was the firstto
give
strong arguments in favour of a continuousdensity
of localized states. Later Mott[23]
introducedthe concept of a critical energy
separation
in a bandlocalized from non localized states. So in our
magneti- cally
disordered case, bandsplitting
is not the exactcriterion for the metal insulator transition. One must rather know the nature of the states at the Fermi level.
Anderson
[14]
gave a definition of the concept of localization : if one put an electron on aparticular
site at time zero, it has a finite
probability
to be onthe same site at infinite time. To
study
thisproblem
he
emphazised [22]
that it is wrong tostudy
averages but instead allquantities
must be characterisedby
their
probability
distribution functions. We haveseen in part II that a natural
quantity
one has tointroduce is the local
density
of states on site i withoutthe
perturbation
on this site. This iseasily
seen fromequation
12.If the self consistent
magnetic
moment yi islarge enough
to create a bound state of energyEB
out ofthe local
density
of statesn(w ;
pi , ..., Mi = 0, ...,Iln)
the free energy has an extra contribution