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Stability of the atomic magnetic moments in

La2-xSrxCuO4 and effect of their fluctuations on the electronic density of states

T. Hocquet, J.-P. Jardin, P. Germain, J. Labbé

To cite this version:

T. Hocquet, J.-P. Jardin, P. Germain, J. Labbé. Stability of the atomic magnetic moments in La2-

xSrxCuO4 and effect of their fluctuations on the electronic density of states. Journal de Physique I,

EDP Sciences, 1994, 4 (3), pp.423-439. �10.1051/jp1:1994149�. �jpa-00246918�

(2)

J. Phys. I Fianc.e 4 (1994) 423-439 MARCH 1994, PAGE 42~

Classification Physics Abstracts

75.10L 74.70v 74.20

Stability of the atomic magnetic moments in La~ ~Sr~Cu04 and

effect of their fluctuations

on

the electronic density of states

T.

Hocquet (1),

J.-P. Jardin

(2),

P. Germain

(1)

and J. Labbé

(1)

il)

Laboratoire de

Physique

de la Matière Condensée de l'Ecole Normale

Supérieure,

24 rue Lhomond. 75231 Paris Cedex 05, France

(2) Laboratoire PMTM (CNRS), Université Paris Nord, 93430 villetaneuse, France

(Received Jo September 1993,

accepted

29 November

1993)

Abstract. We calculate the band structure of the

antiferromagnetic phase

of La~ ~Sr~CUO~ m a

bidimensional itinerant electron model. Then, we discuss the

stability

of the

antiferromagnetic

phase and we calculate the size of the atomic magnetic moments with respect to the temperature and the

doping

ratio x. We show that the

antiferromagnetic

solution is m any case much more stable than the

ferromagnetic

one.

Finally,

we grue a

description

of the

antiferromagnetic

fluctuations from which merges an

exphcit physical meaning

of the pseudo-gap found in the electronic density of states. Implications for superconductivity are proposed.

l. Introduction.

It is a common idea that the

superconductivity

of the copper oxides cannot be understood

mdependently

of their

magnetic properties.

Indeed, spm fluctuations are observed even in the

superconducting phase,

and it is an

extremely

controverted

question

tu know whether

superconductivity

in these materais finds its

physical origm

in these

fluctuations,

or

simply

coexists with them.

In this paper, in view tu

clanfy

a little this

question,

we come back tu a detailed theoretical

study

of the

antiferromagnetic phase by

using a bidimensional itmerant electron model in the

CUO~ planes.

We concentrate our attention on the

La~ ~Sr~CUO~ compounds,

which have a

single-layered

structure of

CUO~ planes.

A simùar

study certainly

would be valid in other

oxides with

CUO~ planes,

but with

complications

due tu their

mufti-layered

structure

and,

in

YBa2Cu30~,

tu trie CUO linear chains.

We calculate trie

antiferromagnetic

gap and trie size of trie atomic

magnetic

moments as

functions of trie temperature and trie

doping

ratio x, and we discuss their stabilities. Then we calculate the electromc

density

of states of trie

paramagnetic phase by taking

mto account trie fluctuations of the size of the atomic

magnetic

moments. As a result, we obtam a

deep pseudo-

gap which is very similar tu that found

by Charfi-Kaddour,

Tarento and Hénlier

Ii by

a

(3)

424 JOURNAL DE PHYSIQUE I N° 3

different method. From Dur

analysis,

the main feature of this

pseudo-gap

is

entirely

due tu trie fluctuations of the size of trie magnetic moments. Furthermore, our

explicit description

of the fluctuations indicates that the overall

density

of states is

nothing

else than the addition of contributions

coming

from different parts of the

crystal

at a

given time,

and thus it cannot be used tu calculate local

properties.

As a matter of

fact,

in the

paramagnetic phase,

near the transition fine,

only

the most

probable

value of the atomic magnetic moments vanishes and, at a given time, areas of the

crystal

with non

vanishing

moments coexist with other areas without

moment, where a

superconducting

state can

locally

exist. From this

point

of

view,

une can

understand trie observed coexistence of

antiferromagnetism

and

superconductivity

without

having

tu assume this coexistence at trie same

place

in trie

crystal.

In section

2,

we

give

a detailed

analytical

calculation of trie band structure of trie

antiferromagnetic phase.

In section

3,

trie

equihbrium properties

of the

antiferromagnetic phase

are deduced from trie

grand potential.

In section 4, we compare trie stabilities of trie

ferromagnetic

and

antiferromagnetic

solutions,

showing

that

ferromagnetic

fluctuations would be

entirely negligible.

In section

5,

we

explicitly analyse

the effect of trie fluctuations of trie size of trie atomic

magnetic

moments on trie overall

density

of states, and we discuss its

physical

meamng.

2. Band structure of the

antiferromagnetic phase.

In trie

La~ ~Sr~CUO~

type of

compounds,

the Fermi level is

customarily

assumed tu lie in trie

antibonding

part of a band ansmg from

hybridization

between copper d~2_~,2 and oxygen p~ and p~, orbitals inside

CUO~ planes [2-4].

A two-dimensional

tight-binding

model leads tu trie

following simplified dispersion

relation in trie

paramagnetic phase

E(k)=E~~-2t(cosk~a+cosk,a),

il)

where E~~ is the effective energy of an electron

occupying

trie d~2

_~,2 orbital on a copper site,

t is the effective transfer

integral

between two nearest

neighbounng

copper sites

through

the p~ or p~, orbital of the intercalated oxygen atom, a is the square lattice parameter, and k~ and k~ are the Cartesian components of the wave vector k

along

the axes of trie square lattice.

Within this scheme,

only

the two-dimensional array of copper atoms m

CUO~ planes

is

considered.

The

simplest

way to take into account the

repulsion

between the electrons in this

tight- binding

model is to introduce the

single

band Hubbard Hamiltoman which, m the mean-field

approximation,

reduces to

H~t

1 CΫCjoe+11(Eat+U(fin))fin

+

(Eat+U(fin))fin ~U(fin)(fin)1> (2)

1jw i

where

c)~ (resp.c~~)

is the creation

(annihilation)

operator for an electron with

spin

w on a copper site i,

(n~~)

is the expectation value of the number operator n~~ = c.)~ c~~, U is the Coulomb

repulsion

parameter between two electrons with opposite spms on the same

copper site, and, m the first term, the summation must be extended

only

on the nearest

neighbounng

sites i and

j.

Different types of

magnetic

solutions can be discussed from trie model Hamùtoman

(2).

In trie present section, we are interested in trie

antiferromagnetic

solution. It will be

compared

to trie

ferromagnetic

solution m section 4.

In trie case of

antiferromagnetic order,

trie copper lattice is

split

mto two sublattices referred to as and

2,

and trie unit cell size is doubled as shown m

figure

I. Trie new unit cell contains

two

unequivalent

copper atoms

having

the same number of electrons but opposite magnetiza-

(4)

N° 3 ANTIFERROMAGNETIC STABILITY IN

La2-~Sr~CUO~

425

~

i ,"""' """",

x

",,, à

,,"

",, ,,."

a

Fig. l.

Antiferromagnetic

unit cell (dashed fine), with the

magnetic

moments localised on the copper sites.

tions m and m, with

n =

(n

ji +

(ni

j

)

=

(n~

t

)

+

(n~

j

)

,

(3a)

~ ~

~~l1 ) ~~l

Î

)

~

~~21 ~~21) (~~)

As a result, the initial band

sphts

into two subbands. In the

tight-binding approximation,

the Bloch wave function becomes

9'(«(r)

=

jj e'~'~"' jjAj~(q) 4 (r Rm

r~ ),

(4)

,,1 a

where q is trie wave vector,

R~

is the

ongin

of trie mth

antiferromagnetic

unit cell, where r~ Iocates trie copper atom « =

I or 2, v

= ± will be trie subband

index,

and trie coefficients

A[~(q)

are

determined,

as well as trie

eigenvalues E(

of trie Hamiltoman

H, by solvmg

trie

Schrüdinger equation.

One finds trie

following

two

dispersion

relations :

E(

=

Eo

±

/A2

+ 64 t~

cos~ (qj

~

cos~ (q~

~ ,

(5)

2 2 2

which are

independent

of the spm w, as

expected

for an

antiferromagnetic

solution, and where A

=

U

mi, Eo

= E~~ + nU, b = a

/

is trie

antiferromagnetic

lattice parameter, and 2

qj =

(k~

+

k~)/ À

and

q~ = (k~ k~,)/

/

are the Cartesian components of the wave vector q

along

the axes of the

antiferromagnetic reciprocal

lattice.

When m

=

0,

equation

(5)

comes down to

equation (1),

with

Eo

in

place

of E~~, due to the introduction of the on-site electron interaction. But when m #

0,

a gap is

opened along

the constant energy hne the

equation

of which is

cos k~ a + cos k~, a = 0

(6)

The

density

of states per copper atom,

including

trie two spm states, is

5l« (E j

=

£ jj s~j~ (E j

,

(7j

with

b 2

jj

~ ~

s~lu(E)

=

~

d

q[Aj~(qj[ à(E-Ej). 18)

(5)

426 JOURNAL DE PHYSIQUE I N° 3

When

solving

trie

Schrüdinger equation,

one finds

(Ali (q)(~

+

(Ait (q)[~

= i

independently

of « and v indices. Thus trie

density

of states per atom is trie same for trie two

copper atoms a = or 2 within a same unit

ceII,

and reduces to

b 2

jj

5~(E)=ij(E)=d~~(E)= (-j jj d~qô(E-E(). (9)

2 w

~__

This Ieads to

i

[E-Eo[

~~~~"/ ~~~~~> (~°)

(E-Eo)~-~

Î

4 with

F

(E)

=

&i<(E)i &((E Eo)~ Ki<(E)i

,

(i i)

where

&[u]

= I for u

m 0 and 0 for u

<

0,

f(E)

=

~

(E Eo

+

~j

(Eo

+

~ Ej

,

(12)

16t 2

and

~~~~~~~ 0

,

<(E)sin~u

~~~~

m which we recognise trie

complete elhptic integral

of trie first kind as

only

(

(E

m 0 bas to be retamed in

expression II).

Trie total

density

of states per copper atom is shown in

figure

2, m trie

following

two cases :

(il

trie

paramagnetic

case

(Fig. 2a),

when m

=

0,

and thus A

= 0,

Ieading

to

%~~~~(E)

= 2

d~1°~(E)

=

F1°~(E), (14)

w t

where

d~~°~(E)

is trie

density

of states per atom and per spm, with

Fi°~(Ei

=

&1<~°~(E)i Ki<~°~(Eii

and

(~°~(E)= ~~(E-Eo+4t)(Eo+4t-E).

16t

It is easy to show that d~~~~~(E) exhibits a

loganthmic

Van Hove

smgulanty

in trie middle

Eo

of the band, this kind of

singularity being expected

for a two-dimensional lattice :

(ii)

the

antiferromagnetic

case

(Fig. 2b),

when m #

0,

m which the band is

split

into two

subbands

separated by

a

non-vanishing

gap A, trie previous

smgularity

at

Eo

in the

paramagnetic case

being split

mto two new

singulanties

at trie

edges

of trie band gap. Close to

(6)

N° 3 ANTIFERROMAGNETIC STABILITY IN

La~_~Sr~CUO~

427

E

flfpa~a(ll~

~a

E~ 4t E~ E~+ 4t

E

b

A m imiu

flf(é~

E~+E~

E

E~-e~

E~ E~ ° E~

Fig.

2. Electronic density of states m the

paramagnetic

state (ai, and in the antiferromagnetic state (b)

with a gap A =

[m

U, Eo E + nU, F~

=

,fi

~~~

~, ~

l

~

~ 2 2 2

these

singulanties, d~(E)

can be

approximated by

trie

following analytic expression

~

~~

~

/

~2

~~

~2

~~~~

~~ Î~ -

~ (E

~ÎÎ)2

~

Î Î

which in trie

previous paramagnetic

case would reduce to

d~~~~(E)=2fl~~°~(E)>

Ln ~~~

(16)

" t

ÎE~EOÎ

Since the band is

nearly

half-filled in these

compounds,

the Fermi level

E~

lies close to one of trie gap

edges.

Thus we will use in trie

following,

as a

good approximation

of

d~(E),

the

simplified

version

(15) adequately

normahsed tu unity

simply by changing

gr2 into 4

(1

+ 2 Ln 2

).

3.

Stability

of the

antiferromagnetic phase.

The

equilibrium

value of A

= m

U,

as a function of trie

temperature

T and trie occupancy of trie

band,

which itself

depends

on trie

doping

ratio x m

La~ _,Sr~CUO~,

is that which minimises trie

grand potential D(T,

p,

A),

for fixed values of T and of the chemical

potential

p. In the meanfield

approximation,

the

expression

of D

(T,

p, A j, counted per copper atom, is

D(T,

p,

A)

= kB T

Îd~(E)Ln [1+ e~Pl~~~~]

dE ~4

(n~ -m~) (17)

where

ks

is the Boltzmann constant,

p

=

1/ks

T and trie

integration

must be extended over trie

two intervals for which A w E

Eo

w

~.

From section 2, %

(E)

is symmetn-

2 2

(7)

428 JOURNAL DE PHYSIQUE I

cal with respect to E

=

Eo

and normalised to

unity

for each one of trie two

subbands,

as it includes trie two spm states. Thus expression

(17)

becomes

n(T, p,A)=

F2

u

~ ~

=-p

+Eo-ksT p(F)Ln [2chpe+2chp(p -Eo)]de--(n

-m

(18)

~~

4

with

e=E-Eo, p(e)=d~(E), ej=-),fi

and

e~=-)A.

As trie Fermi energy, or chemical

potential,

lies closes to one of trie

edges

of trie band gap, trie

grand potential depends only

very little on trie exact expression of p

(e)

far from these

edges.

Thus, we shall

replace

p

(e) by

its

simplified expression (15)

extended to trie entire range of trie two

subbands,

but

adequately

normalised as indicated at trie end of section 2.

Then,

mtroducing

the dimensionless variable a~

=

tilt,

as well as the dimensionless parameters r =

ks

T/t, q

= t/U, and a~~ =

(p Eo)/t,

X

=

mU/2 t, and thus A

=

2 t

(X(,

one gets

n(r,

7~~,

X)

t

=a~~-(j~Ln(~))Ln(2chfi+2ch)jda~+qX~-£ (19)

W o q

The chemical

potential

p

(or

a~~) is related to trie

doping

ratio x

by

trie

following equation

fit1-X#-

(~

H T,~ ,

which leads to trie

equation

Sh

~~

4 j6

d~

~

(2°)

~2

~~

~

fi

~ '~F

C

~

~ ~

y

where ~~

depends

on x

through Eo

= E~~ +

j

nU.

By denvmg

equation

(19)

with respect to X, for fixed values of T and p, une gets

~~

=

2

tXg(r,

~~,

X) (21)

ôX T,

~

with

j16 ~,/~~+X~

4~~

~

~~~'~~'~~"~~PÎO ~/~~~~,fi~~~j~~'

~~~~

r r

Equation (21)

vanishes either when X

=

0 or when

g(T,

~F, X

=

0.

(23)

(8)

N° 3 ANTIFERROMAGNETIC STABILITY IN

La~_ôr~cuo~

429

For given values of r and x,

equations (20)

and

(23)

can be

numencally

solved tu determine

both ~~ and X. A solution with a

non-vanishing

value of X will charactense a stable

antiferromagnetic

state if the

corresponding

extremum of D

(r,

~~, X is a minimum. An the

equation

of the frontier of trie

antiferromagnetic

domain m trie

(x, ri plane

wùl be

g(r,

~~,

0)

=

0,

with ~~ determined

by equation (20)

with X

= 0.

Now,

trie

stabihty

of trie paramagnetic state

(X

=

0) depends

on trie

sign

of trie second denvative

lf) (X=0)=2tg(r, ~~,0). (24)

ôX T.~

But it is easy to show from

equations (20)

and

(22)

with X

=

0 that, for a given value of r,

g(r,

~~,

0) monotonously

mcreases with ~r and

thus,

as it vanishes on trie frontier of trie

antiferromagnetic domain,

is

negative

inside this domain and

positive

outside

(Fig. 3).

This demonstrates that within trie

antiferromagnetic

demain D

(r,

~~,

X)

bas a local maximum for X

= 0.

Thus,

as

D(r, a~~,X)

goes toward an mfinite

positive

value when X

infinitely

increases, the previous solution of equations

(20)

and

(23)

with a

non-vanishing

value of

X

corresponds

to an absolute minimum of

D(r,

a~~,

X),

and so charactenses a stable

antiferromagnetic

state.

o o.05 o-i o.15

~°'~

PARA

°'~

M

o.1

~

Xc ~

Fig. 3. Phase diagram m the plane (x, r) showmg the transition fine between the antiferromagnetic (AF) and the paramagnetic (PARA) phases, calculated for q

=

t/U

=

0.5.

The frontier between trie

antiferromagnetic

and trie paramagnetic

phase

m

figure

3 has been

numencally computed.

At zero

temperature (r

=

0),

equation

(20)

reduces to

x=

~~a~)(1+Ln ~~), (25)

iT 71F

with

a~/

=

fiwhen

x #

0,

but

a~/

= a~~ = 0 when x

=

0.

Furthermore, when r

=

0, the

equilibrium

condition

(23)

becomes

~ iô

4 n

~

~

~~

~

~

Î~j,fi ~'~

~~~~

The variation at r = 0 of the gap

(X

versus the

doping

ratio x can be

numerically

calculated

(9)

430 JOURNAL DE PHYSIQUE I N° 3

from

equations (25)

and

(26).

The result is

plotted

in

figure

4. From

equation (26),

the critical value xc of x for which X vanishes at r

=

o

corresponds, by

equation

(25),

to the value

a~/c

of

a~/

the

expression

of which is

7~

)~

= )6

~-'fi

~~~

which, for q »

0.05, roughly gives a~)c

=

16 e~ ~ "

à

0 0.02 o-M 0.06 0.08 o-1

x~

0A

~0.3

0.2

(X(

o-1

o

~ x

X

~

Fig.

4. The variation of the reduced gap

[X[

=

[m[

U/2 t versus

x at r = 0, calculated for t/U

= 0.5.

The gap X gets its maximum value

Xo

when x = o and thus

a~)

= o.

Therefore,

for

r = o,

Xo

is determined

by

condition

(26)

with

a~)

=

o,

which leads to :

~

"~

~ ~~

Î ~~~~~ o )~ ) ~~

~~~~

One can subtract trie

vanishing

contribution from trie last

integral

m

equation (28)

~

~~~~~

)

dY

~

°

o + y

Then, looking

for an approximate solution

Xo

« with trie remaming ternis of equation

(28),

one finds

Xo

~

32

e~'&

«~q

+ o.33 ~~~

which, for q »

0.01, roughly

grues

Xo

~ 32 e~ ~ "

à

Thus trie

expression

for trie maximum

value mo =

(2 t/U) Xo

of trie magnetic moment per copper atom m trie

antiferromagnetic phase

at zero temperature is

roughly

mo m 64

e-2«@

~

(30)

A

striking

feature of

expression (30)

is trie

exponential dependence

of trie last factor on

ÀÎ

instead of

t/U,

as wùl be found for trie

ferromagnetic

solution m section 4.

To compare trie stabilities of trie

antiferromagnetic

and

ferromagnetic phases

at zero

(10)

N° 3 ANTIFERROMAGNETIC STABILITY IN

La~_~Sr~CUO~

431

temperature, we will bave to use in section 4 the

following expression

of trie

grand potential

per copper atom in trie

antiferromagnetic phase

at r = o

~

~~'

~~

~~

=

(l x)

a~F

~

j~ fi

Ln ~~

da~ +

qX~ (31)

t gr

~j

a~

The curve in

figure 3,

which separates trie

antiferromagnetic

from trie

paramagnetic domam,

grues trie variation, versus the

doping

ratio x, of trie critical temperature r~ at which the atomic

magnetic

moment on each copper site vanishes. As

long

as x remains much smaller than xc, r~

slowly

decreases as x increases, with a

vanishing slope

for x

= 0. Trie value ro~ of r~ for x

= 0 is determined

by

the condition

g(ro~,

a~~

= 0, X

=

0)

= 0,

leading

to 2 gr~ q

=

j~ ~'~

Ln ~~ th ~ '~

(32)

o 71 71 TO

m

Equation (32)

is

entirely

similar to that

determining

the

superconducting

critical temperature m

trie same

compounds,

which had been denved in a

previous

paper

[4]. Solving

it

by

trie same

method,

ones finds

~°m " 18.14

e'~

~~~~

which,

for q »

ù-ù15, roughly gives

ro

~ -

l 8.14 e ~ "

à.

The curve in

figure

3,

exhibits,

above trie critical

point (r

=

0,

xc

),

a

prominent

part which

actually

bas a clear

physical meaning.

To understand

it,

one

merely

bas to realise that trie

mstabihty

of trie

paramagnetic phase

arîses from the Bloch states

Iying just

below trie middle of trie band in this

phase

because trie energies of these states are decreased

by

trie

opening

of an

antiferromagnetic

gap when it

happens. New,

when x becomes

Iarger

than xc

along

trie axis

r =

0 in

figure

3, trie Fermi Ievel moves away from trie middle of he band and trie

paramagnetic phase

recovers its

stability. Then,

when

starting

from a

paramagnetic

state with

r =

0 and x

just

a little

larger

than xc, the temperature r is increased with x

kept

constant, the

smearing

of the Fermi Dirac distribution

partly repopulates

the states

lying just

below trie middle of trie band and, for

r

larger

than a critical value

(which

of course

depends

on

x),

the

antiferromagnetic phase

recovers its

stability.

But this

stability

of the

antiferromagnetic

phase

it lost

again

after a further increase of r

large enough

to excite a

non-negligible

number of electrons mto trie states above the

antiferromagnetic

gap.

By expanding

expressions

(20)

and

(22)

with X

=

0 for r much smaller than a~~, one obtains the

following approximate

equation

of trie curve m

figure

3 in the immediate

neighbourhood

of the critical

point (r~

=

0, xc)

12

y 2

x m xc +

Ù j (34)

~ 'ÎFC

Equation (34),

which is valid for r~ « a~

)~ only, clearly

shows that x staffs increasing from its initial value xc when r~ mcreases from zero.

Trie numerical values of the parameters U and t in these

compounds

are

extensively

controverted

by

different authors. From our

results,

two

physical quantities depend

on the

single

dimensionless parameter q = t/U. The first one is the maximum value mo pB of the

magnetic

moment per copper atom, where pB is the Bohr magneton andis given

by

equation

(30).

The second one is the cntical

doping

ratio xc at which the atomic moments on copper vanish at T

= 0, and which can be calculated from trie

equations (25)

and

(27).

Another

(11)

432 JOURNAL DE PHYSIQUE I N° 3

mteresting physical

quantity is trie maximum value

To~

=

ro~t/k~,

which occurs for

,r =

o,

of trie critical temperature

T~

at which trie atomic moments on copper vanish. with ro~

given by equation (33).

It seems to exist a

general

agreement for trie measured value mû =

0.4 in trie

compound La~CUO~ [5, 6]. By introducing

this value into

equation (30),

one gets t/U

>

0.475,

and then, from

equations (25)

and

(27),

one finds xc > 0.095.

Besides,

with for instance t = 0.5

eV, equation (33)

grues

To

~ =

I 390 K

(a

direct numerical calculation from equation

(26)

leads to more exact values q w

0.496,

xc

~ 0.097 and To

~ >

I 270

K).

It must be

emphasised

that the cntical values of the

doping

rate x and the

temperature

T which bave been calculated in this

section are those for which trie atomic

magnetic

moment goes to zero, and

they

are

certamly

larger

than trie other critical vlues of x or

T,

which remain to be calculated, for which trie

long-

range order between the non yen

vanishing

atomic moments

disappears.

From ibis

point

of

view, trie above calculated numencal values of xc and To

~

are not unreasonable, as

compared

to trie extension of the

antiferromagnetic

domain in the measured

phase diagram

of these

compounds,

which appears to exist for,r smaller than

roughly

0.03 and T smaller than a few hundred of kelvins.

Finally, by

using trie above numencal value of q, we bave calculated trie map of trie atomic

magnetic

moments for a discrete set of values of x and r. Trie results are shown in

figure

5.

o

o.2

~

~~

x

o.2

~

o-1

0

~

Fig.

5. The map of the atomic magnetic moments for a discrete set of values of x and

r calculated for t/U

= 0.5.

4.

Companson

with a

ferromagnetic

solution.

In a

ferromagnetic

state, the

penodicity

is the same as m trie paramagnetic state, trie expectation value

(n~)

of the number operator n~~

being

site

independent,

and thus also the magnetic moment m =

(ni ) (nj )

per copper site. In the Hartree-Fock

approximation,

the

dispersion

relation

(1)

has

simply

to be

replaced by

a new one

E~(k)

=

E(k

+ U

(n_ ~) (35)

By mtroducmg

here agam the

expectation

value n

=

(ni )

+

(ni )

of the total number of electrons per copper

site, equation (35)

can also be written as

Eu (k)

=

E

(k)

+

) (n

wm

(36)

(12)

N° 3 ANTIFERROMAGNETIC STABILITY IN La~

_~Sr~Cu04

433

As a result from the new

dispersion

relation

(36),

the band is

split

into two identical subbands with

opposite

spms w

= ±

,

shifted from trie band in the

paramagnetic

state for one spm

by

trie two

opposite

energies wUm. Trie

densky

of state of trie subband with trie spm

2

w is

S)[(E)

=

~1°~(E

+ w

~"~

(37)

where

d~1°~(E)

is trie

density

of state per copper atom and per spm in trie

paramagnetic

state.

Trie expression of trie

grand potential

per copper atom m a

ferromagnetic

state is

D'(T,

p, m

= kB T

jj S)[ (E )

Ln [1 + e~ POE ~

~] dE

) (n~ nt~ ) (38)

«

where the

integration

is extended from

Eo

4 t wUm to

Eo

+ 4 t wUm.

By

usmg the

2

density

of states which results from

equations (37)

and

(16),

and

by introducmg

the dimensionless variable a~

=

(E-Eo)/t

and trie dimensionless parameters r

=kBT/t,

X

=

mU/2 t, q =

t/U and a~~ =

(p Eo)/t,

ones gets

~'~~'~~~'~~=a~~-~j~~Ln(Ln(2ch~+2ch'~ '~~)da~+

2gr _4 71 T T

~2

+

qX~ (39)

4 q The chemical

potential

p

(or

a~~) is related to the

doping

ratio,r

by

trie condition

~~

ôD'j

ôH T,,n

leading

to trie

followmg equation

~Jp ~J

+4 16

~~

~ da~ ~~~~

~

2 7r~

-

4

~~

Î'~

ch ~

+ ch

~~ ~

~ r

The

equùibrium

value of the

magnetic

moment m =

2 tX/U per copper atom is determined

by

the condition

(ôD'/ôX)~

~ =

0, which leads to the condition

4gr~qX=sh~l~Ln

~~

~'~ (41)

T ~ Î711 X 71F~71

~~

r

~~~

r

For given values of r and x, trie

equilibrium

values of X and a~~ can be

numencally

calculated from equations

(40)

and

(41).

A

ferromagnetic

state is characterised

by

trie existence of a stable

solution with a

non-vanishing

value of X.

At

first,

let us compare the stabilities of the

ferromagnetic

and trie

antiferromagnetic phase

for x

= o and r

=

0. When x

=

0, equation (40)

grues a~~

=

o

anyhow

is the value of

r. When x

=

0 and

r = 0, expression

(39)

reduces to

~

x~

Ln x

~ ~

3 + 8 L~ ~

x~ (42)

~'~~j~'~~~~p~~~~~~~~~

2gr~ 4"~

(13)

434 JOURNAL DE PHYSIQUE I N° 3

Expression (42)

gets its minimum when X is

equal

to

Xi

=

16 e~ ~~ "~~

(43)

with the value

D '

(0, 0, Xi

4

X(~

=

-j(1+4Ln2)-j. (44)

t gr 4gr

For a same value of q, these results have to be

compared

with

Xo

and D

(0, 0, Xo)

in the

antiferromagnetic phase.

The value of

Xo

is given

by equation (29).

If we

replace

q m the term

qX( by

its

expression resulting

from

equation (26),

with a~~ =

a~)

=

0,

we get

n(o,

o,

Xo)

4

j4

(1J

/~)~

16

t

~2

~~ ~ ~ ~~ ~ ~

~2

~

fi

~~ ~

~'~

~~~~

71 + o

The

mtegral

in

equation (45)

is

easùy

calculated

by introducing

trie new variable u defined

by

a~ =

Xo

sh u. One finds

~ ~~~

~ ~~~ ~~

~ ~ ~~ ~

~~

~ 4

Î~ià

~

~~~~~

~~~~

The numerical evaluation of

equations (44)

and

(46),

with

Xo

and

Xi

given

by equations (43)

and

(29) respectively,

shows that trie

antiferromagnetic phase

is more stable than the

ferromagnetic phase

as far as q is

langer

than the small critical value qo >

0.092,

and thus as t is

larger

than trie critical value 0.092 U. For q much

larger

than qo, as it must be assumed for

our itmerant model to be valid, the minimum of trie

grand potential

for,r

= 0 and for

r = 0 is much lower m trie

antiferromagnetic

than m trie

ferromagnetic phase,

with a

larger

atomic

magnetic

moment. For instance with q =

0.5,

one finds

D

(0, 0, Xo)

D

(0, 0, 0)

= 2

qXo

~

> 0.4 and

> 2 x 10~

m trie

antiferromagnetic phase,

and

D'(0, 0, Xi D'(0, 0, 0) mi

~

= 2

qX(

> 0.003 and

> 2.5 x 10~

in trie

ferromagnetic phase,

with

D'(0, 0, 0)

=

4(1

+ 4 Ln 2

)Iv

~.

As m section

3,

the critical value

xi

of the

doping

ratio x for which the atomic

ferromagnetic

moment

m=2qX

would vamsh at zero temperature can

easùy

be calculated from

equations (10)

and

(41)

with r

=

o. For r

=

0,

equation (41)

reduces to

~F +X ~~

4

gr~ qX

=

Ln da~

(47)

~~ -X

Î'Î

For much smaller values than a~~, as is the case when x

approaches

the critical value

xi,

the

mtegral

m

equation (47)

can be

expanded

with respect to

Xla~~. By retaining

trie first

(14)

N° 3 ANTIFERROMAGNETIC STABILITY IN La~

_~Sr~Cu04

435

non-vanishing

terms

only,

one gets

4 gr~

qX

> 2 X Ln ~~

+

~~

~

(48)

71F 3 a~~

Equation (48)

bas two solutions. Trie first one is X

=

0 and trie second one is the

positive

solution of the

following equation

X~

= 6

a~j(2 gr~q

Ln

~~

(49)

71F

It

exists,

and is then trie more stable

solution,

as for as a~~ <

a~)(,

with

a~)(

= 16

e~~"~~, (50)

Besides

equation (40)

with r

= 0 and X

=

0 leads to

xi

=

'~~) 1'

l + Ln

~(, (51)

a~~c

and

thus, by using expression (50)

of ~

il,

to

x)

=

~~ (l

+ 2

gr~q) e~~"~~. (52)

w

It is

interesting

to compare trie cfitical value

xi

for trie

ferromagnetic solution, given by equation (52),

to the

corresponding quantity

x~ for trie

antiferromagnetic

solution, which from

equations (27)

and

(25) roughly

is

equal

to

xcw

~~(l

+2gr

à)e~~"à. (53)

gr

It appears that for q much

Iarger

than trie

already

found critical value qow

0.029,

xi

is much smaller than xc. For

instance,

with q =

0.5,

one finds

x[

m

0.01xc.

The critical temperature

r(~

at which the atomic

ferromagnetic

moment m = 2

qX

would

vanish for x

= 0 is

given by equation (41)

with X

=

0 and ~p =

0, leading

to

2 gr~

qr(~

=

~

Ln ~~

~~

(54)

° ~ l + ch

)

~o m

For q much

larger

than the previous critical value qo, trie

approximate

solution of equation

(54)

is

easily

found to be

r(~

w 18.14 e~ ~"~~

(55)

The

comparison

of the

expression (55)

of

r(~

in the

ferromagnetic

state with the ex-

pression

(33)

of ro~ m the

antiferromagnetic

state shows that, for q much smaller than

qo, ro~ is much

Iarger

than

ri

~.

For instance, with q =

0.5,

one finds ro~ > 200

ri

~.

The conclusion of this section is that,

although

the Stoner condition

Ufl~1°~(Ep)~

l is

automatically

satisfied when trie Fermi energy

E~

coincides with trie energy

Eo

at which trie

density

of state

d~1°1(E)

bas an infinite

smgulanty,

trie

antiferromagnetic

state is much more

(15)

436 JOURNAL DE PHYSIQUE I N° 3

stable than the

ferromagnetic

state as far as t is much

larger

than 0.092

U,

whatever trie values of trie temperature and trie

doping

ratio are. Thus, an itinerant electron model is also able to

explain why

a

ferromagnetic phase

has never been observed in these

compounds.

This follows from the fact that the

nesting

of trie two-dimensional Fermi surface for a half-filled, or

nearly

half-filled, subband,

which is the cause of

antiferromagnetism

in such an itinerant model,

produces

a much stronger effect than that

resulting

from the existence of an infinite Van Hove

singularity

in trie middle of

Eo

of trie subband, which would

give

use to

ferromagnetism

if it

were not dominated

by antiferromagnetism.

Trie effect which would be

produced by

the

infinite

singularity

is non dominant because this

singularity

is

only logarithmic,

and thus is not very

Sharp.

5. ERect of the fluctuations on the

density

of states.

One of the effects of the fluctuations is to introduce an orientational disorder among the atomic

moments. This

important phenomenon

has

already

been considered

by

several authors. In this

section we deal with another

phenomenon consisting

in the fluctuations of the

magnitude

of each atomic moment around ils

equilibrium

value, and the

resulting

effect on the electronic

density

of the states in the paramagnetic

phase.

It is

always

a very

complicated

matter to calculate the effect of fluctuations, as all the

physical quantities

fluctuate around their

averaged

values.

But,

in order to

simplify

the calculations, we will not take into account the fluctuations of trie temperature T and the

chemical

potential

p. For fixed T and p, trie value of trie atomic magnetic moment

m = 2

qX

which minimises trie

grand potential

is

only

the most

probable

value, around which it fluctuates. So, all the other values of m, between and + 1, bave some

probability

to exist

physically.

In a

paramagnetic

state, m fluctuates around its

equilibrium

value, which is

equal

to zero.

But when this

paramagnetic

state is close

enough

to trie transition hne, trie correlation

length

is

expected

to be

large,

and thus m to

keep

a

nearly

constant

value, equal

or not to ils

vanishing equilibrium value,

over a

large

distance. Then, at a given time, trie

crystal

can be

thought

of as

being

made of a

large

number of different extended areas. The atomic

magnetic

moment

m = 2

qX

varies from one area to

another,

but it

keeps

the same value on all the atomic sites

within each area, to which a local electronic

density

of states

àj~~(X, E),

as given

by

equation (15),

can thus be

assigned.

In each area, the electron number per copper site bas the local value

dE

(56)

nj~c(x)

= I

Xloc(X)

"

~~°~~~'~~

i +

e~~~

~~

In trie above equation, trie chemical

potential

p is assumed to bave a well defined uniform value,

mdependent

of X,

throughout

trie whole

crystal.

This allows us to assume that trie

electrons are

mstantaneously

redistributed between trie vafious areas of the

crystal,

so as to

keep

a uniform value of p, even if trie chemical composition is

homogeneous.

When

calculating

the total number of electrons in the whole

crystal

for fixed values of T and p, the statistical

weight

of trie contribution ansmg from all trie areas with a given value of X must be calculated from trie

grand potential D(T,

p,

X),

and is

equal

to

P~ ~(X)

=

poe~P'~l~.~~~~~~l~.~~°~' (57)

with

I

=

~~'~~

~-PiniT,~,xi-n(T.~,

oj) dx_

P0 1/2

q

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