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Microscopic analysis of structure stabilities in the ionic

compounds

B. Piveteau, Claudine Noguera

To cite this version:

(2)

2005

Short Communication

Microscopic

analysis

of

structure

stabilities

in the ionic

compounds

B. Piveteau and C.

Noguera

Laboratoire de

Physique

des

Solides,

Université de

Paris-Sud,

91405

Orsay,

France

(Received

on

July 9, 1990, accepted

on

July

13,1990)

Résumé. 2014 En

associant,

pour la

première

fois,

un calcul

d’énergie

de cohésion et une

approche

à la Landau des transitions de

phase,

nous

présentons

une

analyse

de la stabilité relative de deux

phases

structurales d’un

composé

ionique à 0

K. Cette association de deux

méthodes,

en elles mêmes

classiques, permet

de découvrir

progressivement

les interactions

microscopiques

associées à

chaque

distortion,

et fournit les valeurs

numériques

des coefficients de Landau dans le

développement

d’éner-gie correspondant.

Cette méthode illustrée ici sur le

composé

La2CuO4

ouvre un

large champ

d’in-vestigation

dans le domaine des stabilités structurales des

composés

ioniques.

Abstract. 2014

Associating

for the first time a total energy calculation and a

phase

transition

approach,

we

present

an

analysis

of the relative

stability

of two structural

phases

in an ionic

compound

at zero

temperature.

This new combination of two classical methods allows a

progressive discovery

of the

microscopic

relevant interactions associated with each

distortion,

and

yields

the value of the Landau coefficients in the

development

of the energy. Illustrated on the

compound

La2CuO4,

this method has a wide

applicability

in the field of the structural

stability

of ionic

systems.

LE

JOURNAL

DE

PHYSIQUE

1

Phys.

France 51

( 1990)

2005-2010 15 SEPTEMBRE

1990,

1

Classification

Physics

Abstracts

61.SOL - 61.60 - 64.70K - 74.70V

Over the

past,

there has been a constant interest in

understanding why

a

given

ionic

compound

cristallizes in one structure rather than in another one

[1] .

But

only recently

did one

apply

elabo-rate numerical methods to this

problem.

livo families of

approaches

now exist : the first one relies

on electronic structure calculations such as the ab-initio

pseudo-potential

method

[2]

or the self-consistent

tight binding

one

[3] ;

the second one is based

upon

the use of ionic

pair-potentials [4],

at various levels of

sophistication,

and was

proved

to

reproduce

well static and

dynamic properties

of

perfect

and defected structures

[4,5].

Yet,

most of the

time,

the

heavy

numerical methods hinder the

physical insight.

The calculations

(3)

2006

currently

tell which structure is more stable at zero

temperature, but,

not

why

the other

possible

structures lie

higher

in

energy.

As a

consequence,

no theoretical

prediction

can be made on how

a structure evolves

upon

replacement

of one kind of atom

by

another one.

We

propose

in this letter to associate a total

energy

calculation with a

phase

transition

approach,

in order to

analyze

the relative

stability

of two structural

phases

1 and II in an ionic

compound

at zero

temperature.

These two methods

by

themselves are not new, but we demonstrate that their

combination allows to establish a

hierarchy

between the various distortions of the

structure,

in close

relationship

with the order

parameters

of the

(possibly fictituous)

phase

transition between 1 and II

(assumed

here to be a second order

one).

It is then

possible, by performing partial

energy

minimizations,

to make detailed energy counts associated with each

primary

order

distortion,

and thus find the

microscopic

interactions

responsible

for the

symmetry

breaking,

at the

origin

of the

higher stability

of one of the

phases.

We have chosen to illustrate these

general

concepts

on two structural

phases

met in the

com-pound

LaZCu04. La2Cu04,

which became famous because of the occurrence

of high

Tc

supercon-ductivity

upon

doping,

presents

a

phase

transition between a

high

temperature

tetragonal phase

(HTT ;

space group I4/mmm

called

phase

1 in the

following)

to an orthorhombic one

(ORTHO

;

space group

Bmab,

subgroup

of

I4/mmm ;

phase

Il)[7] .

The transition occurs at 500 K at

am-bient

pressure

and

disappears

above a critical

pressure

of about 60 kbars

[8] .

In the

pressure

range

in which it was

studied,

the transition was found to be second order. Earlier studies of the

mechanism of the HTT to ORTHO transition discussed the role of the electronic structure close

to the Fermi level

[9, 10].

Quantitative

total

energy

calculations were also

performed

[4, 5,11] .

But none of these

provided

a detailed

explanation

of the mechanism of the

phase

transition. A

thorough

report

of this

study

will be

presented

elsewhere,

together

with a

development

of this method for first order transitions

[12].

We have chosen the

simplest

version of the ionic

pair

potential

method

[5]

as a

computationnal

support

to our

analysis.

It is worth

stressing

that the choice of another numerical code would

only modify

some of the details of the

specific analysis

of

La2Cu04.

But it would not alter the

general

conclusion of this

letter, i.e.,

the interest of

associating

a total

energy

calculation and

a

phase

transition

approach.

The ionic

pair potential

method

expresses

the total

energy

E

per

formula unit as a sum of

pair

interactions between a central unit and all the other units. Three

contributions are considered : the direct Coulomb

interaction,

a hard core

repulsion

of the Born

Mayer

type

and a small Van der waals term. For two ions labelled i

and j,

at a distance

Rij,

with

charges

equal

respectively

to

Qi

and

Q3 ,

the interaction

energy

reads :

The constants

Bij,

pij and

Cij

are derived

[5]

from atomic values

BH,

pis,

which were shown

to

reproduce correctly

the structures of

La203

and CuO. Th

perform

the

summations,

we

group

the atoms in neutral entities

La2CU06,

as

displayed

in

figure

1.

We discuss elsewhere

[12]

the details of the

computation.

Let us

just

say

that the achieved

convergence

of the summations

gives

an

accuracy

of 10 meV on the total

energy per

formula

unit

(i.e. 0.006% )

and an

accuracy

better than 1 meV on

energy

différences. We

improved

the

agreement

with

experimental

data

[13] ,

by adding

to the ionic contributions

(Madelung,

Born

Mayer,

Van der

Waals)

a term

Ecov=

-Aexp(-qd2)

mimicking

the delocalization of electrons in

the

CU02

planes (withA=25

eV and

q=1.5

A-’).

We also studied the

stability

of the ORTHO

phase

under

pressure,

by

minimizing

the

enthalpy

E + PV of the

system.

We found that ORTHO is

destroyed

above a critical

pressure

of about 57 kbar in

agreement

with the

extrapolation

of X

Ray

data

[8] ;

the orders of

magnitude

for the

compressibility

coefficients

[14]

are correct and

(4)

Fig.

1. -

Representation

of the

La2Cu04

unit in the orthorhombic

phase

and definition of the

eight

struc-tural

parameters

dl, d’2J Z, 0’, 60’,

u and

{3.

The units are titlted with respect to the

[110]

direction of the

tetragonal

axis.

They

include a

Copper

atom surrounded

by

four

in-plane-oxygen

atoms

(called

02 in the

text),

two

out-of-plane

oxygen atoms

(called

01)

and two lanthanum atoms, with

chemically

strong

La=O1 bonds

(the

associated interatomic distance is less than the sum of Van der Waals

radii,

while the

eight

other La-0 distances are much

larger

[13]

).

structural behaviour of

La2

CU04

is

correctly

reproduced

by

our numerical

approach,

and that we

may

safely

use it to understand the

microscopic

origin

of the ORTHO

stability.

We first

study

the

origin

of the cohesion in the HTT

phase.

The total energy is

conveniently

analyzed

as a sum of a

Madelung

contribution

EM

and a Born

Mayer plus

Van der Waals one

EBM.

Each of them can be further

decomposed

into terms

EnM

(respectivcly EnBM) equal

to

the Coulomb

(resp.

Born

Mayer

plus

Van der

Waals)

interaction energy of the central unit with units located in

planes

f(n -1)z

(n >

1).

The

complete

calculation

(lhb.

I,

column

1)

reveals that the cohesion in the HTT

phase

is

mainly

due to attractive

interplane

Coulomb interactions

(E2M

0),

whereas the

intraplane

Coulomb forces are

highly repulsive (EIM

>

0).

The

sign

of these interactions can be understood

by

making

a

development

in

multipolar

mo-ments : the

La2Cu04

units are neutral and have a zero

dipolar

momentum ; their

quadrupolar

mo-. mentum is

highly

anisotropic

and

elongated along

the

[001]

direction of the

tetragonal phase.

In

(5)

2008

lhble 1. - Calculated contributions to the total

energy :

EnM

and

EnBM

refer respectively

to the

Madelung

(M)

and to the Born

Mayer plus

Van der Waals

(BM)

interaction

energies of

a central

La2CU04

unit with all units located in the

planes

at a distance

:1:( n -1 )z.

Column 1 : HTT cohesion energy

(in

eV)

at

equilibrium ,.

the set

of

structural parameters

which minimizes the energy

is found

equal

to

{C} = {d2

= 1.882

Â,

dr

= 2.4i2

Â,

d = 2.379

Â,

z = fi.fi0i

A} ;

Column 2 : energy

difference

En ( 0:) -

El

in

meV,

between tire

HTT phase

and an

ORTHO phase

characterized

by

a

rigid

tilt a=3.6° and the

structural parameters

{C} ;

column 3 : energy

difference

Eu( 0’,

u,

ba) -

El

in meV between the

HTT phase

and an

ORTHO phase

characterized

by

the

three primary

order

parameters

a4 =

3.6°,

u = 0.284

Â

and ba

= -0.5°,

and the set

of parameters

{C}.

These values minimize

EJI(A,

u,

ba)

when

{C}

is

kept

constant. Column 4 : energy

difference

in meV between

the actual ORTHO

phase

and the HTT one when

all primary

and

secondary order parameters

are considered. The

structural parameters

which minimize

En

are found equal

to

d2

=1.906,

dl

= 2.415

A, d = 2.375 A, z = 6.554 A, 0: = 6.23°,60: = -0.18°, fi = 89.0°, u = 0.557 A.

répulsion

is however

compensated by

a

large

attraction of the central unit with the

quadrupoles

of the

neighbouring planes

placed

in a

body

centered

arrangement (E2M large

and

negative ;

EIM

+

E2M

0).

This

representation

of

La2CU04

units as

quadrupoles

thus

gives

a

physical

support

to the results of the

energy

calculation.

The orthorhombic distortion

[13]

involves a

rigid

:f:a tilt of the entities relative to the

[110]

axis of the HTT

structure,

accompanied by

a small additionnal ±ba tilt of the Cu-01

bond,

and

by

a

rotation of the 01-La bond

(displacement

u of the La

atoms ;

the

Cu,

01 and La atoms are no

longer

aligned) (Fig. 1).

Minor modifications of the HTT

parameters 6d, 6d1, bd2,

6z and

a square

to

rectangle

shear distortion of the

CU02

basal

planes

of the units

(,0 # 7r/2)

are also observed.

The ORTHO to HTT

phase

transition is thus a

complex

one, with

primary

as well as

secondary

order

parameters :

we find that

(a,

6a,

u),

which alternate in

space,

are the three

primary

order

parameters,

while the other uniform distortions are the

secondary

order ones, in

agreement

with

simple

symmetry arguments.

The distortion a, associated with a

rigid

tilt

(OE #

0,

6a =

0,

u =

0,

unchanged

HTT

parameters);

induces an

energyvariation DE(a)

which has the form of a Landau

development : DE(a)

=

Aa2+

Ba4.

We find that both A and B are

positive,

which shows that the tilt alone is not stable. The

(6)

fraction of the

intraplane

Coulomb

repulsions (EIM)

is

relaxed ;

b)

since

coplanar

units share

oxygen

atoms

by

their corner, the

alternating

tilt induces a contraction of the Cu-Cu distances in the direction of the

CU02

plane

normal to the tilt

axis ;

this increases

significantly

the

interplane

Coulomb attraction

(E2M).

For medium or

long

range

interactions both

processes

a)

and

b)

lower the

energy

of the

system.

Yet,

at

very

short

distances,

two other effects act

against

this

gain

of energy :

c)

two La atoms of

coplanar neighbouring

units come

significantly

closer to each

other,

and induce

large intraplane

Coulomb

repulsions (bE,m

> 0 in Thb. 1 column

(2)) ; d)

there is an

important

decrease of

interplane La-oxygen (01

and

02)

distances which induces

predominantly

an increase of Born

Mayer repulsion (6E2BM

>

0,

in ’Iab. 1 column

(2)).

Thé coefficient A in the Landau

development

is thus

equal

to the sum of two terms, A 1 small and

negative

due to

a)

and

b),

andA2

large

and

positive

due to

c)

and

d).

We conclude that the

stability

of the ORTHO

phase

is not driven

by

the

rigid

tilt alone

(A

>

0),

because this tilt induces too

large

short range Coulomb and Born

Mayer repulsions.

We now

analyse

the role of the

primary

order

parameter

u associated with the rotation of the

La-01 bond

[15].

The energy variation

due to u and a takes the form :

AE(a, u)

=

Aa2+Cau+Du2

to lowest order. HereA and D are

positive, showing

that each distortion alone is

unstable,

but the

structure with

both Q’ =F

0 and

u =F

0 is nevertheless more stable than HTT because

C2

> 4AD. In

order to understand the

microscopic origin

of the

large

linear

coupling

between u and a, we use

the numerical

program

to calculate

the quantity

AE(a, u) -AE(a,

tt =

0) -AE(OE

=

0,

u) N

Cau

and

decompose

it into

elementary

contributions. We find that it is

unambiguously

due to Coulomb and Born

Mayer

interactions between

coplanar

La-La

pairs

and non

coplanar

La-0

neighbouring

atoms. These same short range interactions were

responsible

for the unfavourable contribution

A2a 2 noted

above. It is thus not

surprising

to find

that,

since the rotation of the La-0 bound

puts

the La atoms close to their HTT

positions,

the energy increase due to effects

c)

and

d)

is erased and the

energy

lowering

due to effects

a)

and

b)

becomes efficient. This

may

be seen in table

I,

in

comparing

columns

(2)

and

(3).

This

analysis

demonstrates that the ORTHO

phase

is stabilized with

respect

to the HTT

phase,

thanks to a

disalignment

of the

quadrupole

axis

accompanied by

a

contraction of the lattice. The

alternating

tilt of the

La2Cu04

entities is

responsible

for this effect but a rotation of the La-01 bonds is also necessary to

impeede

too

strong

short range Coulomb and Born

Mayer repulsions.

This

study

of the

primary

order

parameters

answers the

question :

why

is ORTHO more stable than HTT?

Th achieve a

complete description

of the ORTHO

phase,

we have considered the

secondary

order

parameters.

These latter are of no

importance

as concems the mechanism of stabilization but

they

yield

increased values of the stabilization

energy

and of the

primary

order

parameters.

The variations

ôd2

and az of the Cu-02 and

interplane

distances are of

special importance.

A

Landau

development

of the

type :

AF(A, c)

=

Aà2

+

BA4

+

Cê2

+

FE02

(here

e

represents

lad2, az}

and à

{a, u})

accounts for the energy difference between ORTHO and HTT. We found

that the

coupling

term

FA2,-

between first order and

secondary

order distortions comes

entirely

from Born

Mayer

interactions between closest non

coplanar

La and 01 atoms. These interactions

indeed limited the value of the tilt

angle

at constant values of the HTT

parameters.

An increase

in

d 2

relaxes a

part

of the

repulsions

and

consequently

authorizes an additionnal increase of a

and an additionnal stabilization energy, as seen in table 1 column 4.

We wish to conclude this

letter,

by

stressing

the wide range of

applicability

of our

approach

in the

study

of the relative

stability

of structural

phases,

in

compounds

in which the cohesion is

mainly

due to ionic forces. It

appears

that the more

complex

the difference in the structures of 1 and

II,

the more

precious

the method of

analysis

we

propose.

This

happens

because it allows

a classification of the effects and a discrimination between the

distortion(s)

which are

primarily

responsible

for the

stability

and the ones which are a mere

consequence

of the others. The method

(7)

2010

the

physical

parameters

which influence the energy balance associated with the

primary

order

parameters.

Finally,

our method reveals the

microscopic

origin

of

phase

transitions,

since it is

able to

assign

numerical values to the Landau coefhcients and to reveal the

underlying

physics ;

but at the

present

time it is restricted to zero

temperature.

Acknowledgements.

We are

greatly

indebted to J.R

Pouget

for many discussions all

along

this work. We also

acknowl-edge

fruitful comments from J.

Friedel,

S.

Barisic,

M.K.

Whangbo

and H. Moudden. We thank P. Garoche and R Batail for a critical

reading

of the

manuscript.

References

[1]

PHILLIPS

J.C.,

Bonds and Bands in semiconductors

(Academic,

New

York)

1973.

[2]

CHELIKOWSKY J.R. and BURDETT

J.K.,

Phys.

Rev. Lett. 56

(1986)

961.

[3]

MAJEWSKY J.A. and VOGL

P., Phys.

Rev. Lett. 57

(1986)

1366.

[4]

ALLAN N.L. and MACKRODT

W.C.,

Philos.

Mag.

A58

(1988)

555.

[5]

EVAIN

M.,

WHANGBO

M.H.,

BENO

M.A.,

GEISER U. and WILLIAMS

J.M.,

J. Am. Chem. Soc. 109

(1987)

7917.

[6]

The

secondary

order

parameters

correspond

to the distortions of the

low-symmetry phase,

which do

not break as many

symmetry

elements of the

high-symmetry phase

as the

primary

order

parameters.

At a second order

phase

transition, they

vanish as

(

Tc -

T)03B4with

an

exponent 03B4 larger

than the

exponent

characterizing

the

primary

order

parameter.

e.g. : COWLEY

R.A., Adv. Phys.

29

(1980)

1.

[7]

MORET

R.,

POUGET J.P. and COLLIN

G.,

Europhys.

Lett. 4

(1987)

365.

[8]

KIM H.J. and MORET

R.,

Physica

C156

(1988)

363.

[9]

POUGET

J.P.,

NOGUERA C. and MORET

R., J.

Phys.

France 49

(1988)

375 and references herein.

[10]

BURDETI J.K. and KULKARNI

G.V,

Phys.

Rev. B40

(1989)

8908.

[11]

COHEN

R.E.,

PICKETT W.E. and KRAKAUER

H.,

Phys.

Rev. Lett. 62

(1989)

831.

[12]

PIVETEAU B. and NOGUERA

C.,

to be submitted to

Phys.

Rev. B.

[13]

JORGENSEN

J.D.,

DABROWSKI

B.,

SHIYOU

PEI,

HINKS

D.G.,

SODERHOLM

L.,

MOROSIN

B.,

SCHIRBER

J.E.,

VENTURINI E.L. and GINLEY

D.S.,

Phys.

Rev. B38

(1988)

11337.

[14]

LAUNOIS

P.,

HENNION

B.,

MoussA E and

POUGET J.P.,

private

communication.

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