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ELECTRONIC VERSUS ATOMIC STRUCTURE IN

LIQUIDS

W. Young

To cite this version:

(2)

JOURNAL DE PHYSIQUE

Colloque C8, supplément au n°12, Tome k(>, décembre 1985 page C8-427

ELECTRONIC VERSUS ATOMIC STRUCTURE IN LIQUIDS

W.H. Young

School of Mathematics and Physics, University of East Anglia, Norwich NR4 7TJ, U.K.

Résumé - Un modèle de sphères dures correspond assez bien au facteur de struc-ture S(q) d'un métal liquide. L'addition d'une contribution attractive augmente le S(o) des sphères dures et modifie de façon négligeable les pics principaux. Une contribution répulsive annule S(o) et produit des anomalies aux grandes valeurs de q. Ces résultats sont bien en accord avec les théories de pseudo-potentiel. De plus, les modèles de mélange de sphères dures fournissent des indications sur le Scc(q) des alliages. Des contributions supplémentaires

in-troduisent un potentiel d'ordre qui, s'il est attractif (ou répulsif),

augmente (ou diminue) Scc(o) par rapport à la valeur des sphères dures et il y

a tendance à une séparation de phase (formation de composés). Les théories de pseudopotentiel s'appliquent formellement mais introduisent des contribu-tions où se concentrent les potentiels d'ordre ; les calculs ab initio sont évidemment risqués.

Abstract - Hard spheres provide a suitable reference fluid for liquid metal S(q)'s. Supplementary attractive tails enhance the hard sphere S(0) and yields featureless principal peaks; repulsive tails suppress S(0) and explain higher-q anomalies. These conclusions are consistent with NFE pseudopotential theory. Likewise, hard sphere mixtures provide insight into S (q) for an alloy. Supplementary tails define an ordering potential which, if repulsive (attractive), means S (0) is elevated (suppressed) relative to hard sphere values and there is a phase separating (compound forming) tendency. NFE pseudopotential theory formally applies but, even if valid, yields tails the inevitable errors in which accumulate in the ordering potential; ab initio calculation is evidently risky.

I - INTRODUCTION

The present paper, exceptionally at this conference on amorphous solids, concerns liquids. It shows how observed structure factors broadly delineate interatomic forces; this allows an assessment of how well the latter are specified by ab initio electron theory. It is interesting to note that structure factors depend on the full interatomic potentials in liquids and amorphous solids since all parts (exclud-ing the impenetrable cores) are sampled and appear in the configurational averages. Crystals, on the other hand, are characterised by static lattice configurations and those nearby accessible by thermal vibration and so cannot, in principle, provide as much information.

Liquids and amorphous solids differ in that the former are in thermodynamic equilib-rium whereas the latter are not. Thus, although the concept of the distribution function is used in both cases, only in the former is it governed by the principles of equilibrium statistical mechanics. This is of immense significance and help as is seen below.

We consider monatomic and binary metallic systems only. The former are of consider-able intrinsic interest, illustrate some general principles and are, therefore, con-sidered first (,§II). Later, the binary problem is examined (§11) and a summary pre-sented (§IV).

II - MONATOMIC FLUIDS

(i) Generalities

Consider a monatomic fluid of mean number density n. The radial distribution

(3)

C8-428 JOURNAL DE PHY SlQUE

tion g(r) is obtainable from the interatomic forces using statistical mechanics and connection with experiment is made via the structure factor

S(q) = I + n {g(r)

I

-

1) exp(i_q._r)d_r

.

( 1 ) At long wavelengths, density fluctuation theory yields the identity

Here, KT is the isothermal compressibility and so S(0) is measurable thermo- dynamically; it diverges as the critical point is approached.

The direct correlation function c(r) is defined by the Ornstein-Zernike (OZ) equation

where h(r) = g(r)

-

1. Alternatively, in Fourier transform, and using (I),

The direct correlation function reflects closely the potential; if the latter is pairwise and given by v(r), statistical mechanics yields

~ ( r ) %

-

v(r)/kgT (large r) (4)

and experience suggests (5) is quite accurate anywhere outside the core. If c(q) in (4) Taylor expands, we obtain the OZ form

S(q) = S(o)1(1 + SZqZ) (low q)

.

(6) Near the critical point, the correlation length,

6

,

indicates the size of the density fluctuations; near the triple point, often (always in metals?) Su(0)

>

0 with (formally)

c2

<

0.

Real fluid's resemble, in zeroth order, hard sphere systems which have, therefore, been subject to much theoretical study. The results obtained will be drawn upon as required below.

(ii) The alkalis; illustrative example of Rb

Fig. 1 shows some observed structure factors

Ill

for Rb and their fit to hard sphere data. This is moderately satisfactory at large q but incorrect for small q, high T. Evidently, (6) applies in the latter circumstances, hard spheres alone being inappropriate.

The problem is simply solved thus: (a) calculate v(r) (at each density) using pseudopotential theory, (b) separate core and tail parts 121 (Fig. 2 ) , (c) approx- imate the cores by hard spheres. (d) treat the tails as perturbations. The core scarcely varies with density and one reads off effective diameters 0 using 141 v (0) a k T, the probing of the increasingly steep parts explaining the satura- t%Senoted !i Fig. 1. The tails may be incorporated using the random phase approx- mation (RPA) 151

which recognises basic core and tail aspects (eq. (5). Fourier transformation of

(7)

and use of (4) gives the Fig. 1 OZ behaviour.

(4)

(iii) Polyvalent metals; Waseda types.

We focus on the triple points. Here Waseda 1101 has identified three S(q) types, mainly via the principal peak shapes (Fig. 3 ) , and their distribution throughout the Periodic Table is as in Fig.

4.

The sec. (ii) description for Rb offers an explanation for other type a cases which appears to be correct (see below) for groups 1A and 2A (excluding Be). An explanation /9,6/ for the others (although not the only one mooted) is that tails are essentially repulsive (eg. as used in ( 7 ) ) . Such a feature has been shown to underlie (depending upon detail) not only cases of type b and c, but also some of type a such as Pb /8,9/. This viewpoint is consistent with recent systematic- ally calculated pseudopotential results I101 (Fig. 5) which, although inevitably open to q~antitatat~ve revision, have the right general forms. For example, the pronounced minima in groups 1A and 2A are consist- ent with the observed closer packing in the solids

__-

A

_---_

while the loss of minimum allows possible, but not in-

-

-L evitable (cf. Pb), destablisation to more open struct-

ures. Also, for liquids, as we have seen, such curves are suitable for explaining the Waseda classification.

-.'

9 / r 1 A detailed study I111 lends credence to this view.

0

1

2

3

4

(iv) Low q limit of structure factors

Fig.

-

(-1 and We next show how the S(0) values of,Fig. 4 are hard sphere fits (---I for qualitatively understood. Consider a reference S(q) for R b saturation. fluid of hard sphere cores; then the attractivetail

?erturbations(Fig.5) of the 1A,2A elements enhance S (0) (cf. Rb, sec. (ii)) while the overall . . , , . , . . .

.

. . .

.

.

.

. . .

.

. . . . repuls??e character of the others suppress it. Scrutiny

of the data (Fig. 4) and the curves (Fig. 5) suggest S (0)

" 0.020 and it remains to understand this number.

lo

-1

hs

Now the Gibbs-Bogoliubov method replaces the actual core by a truly 'all purpose' hard sphere with diameter given by 1121 v (0)"

3

kBT. This implies % 45% packing

and S(0) G06%28

-

too large! But the subtler WCA -method yields a 'squashy' sphere characterised essent-

iall-y by a diameter 0 and a force v' (0) 141. The criterion for U becomes v (0)

=

$OFe and the larger value thus produced c$%fnes wita the force to

) describe S(q) generally. However 0

alone

is appro- priate to q = 0 and yields S(0) " 0.020 (correspond-

4

ing to an apparent packing (n/6)na3

"

0.50. r/ll

Fiz. 2 Core and tails (in This account of S(0) bears closer analysis, e.g. mRy)-sor Rb at 350 K (;.46 the increasing attractiveness of the tail (Fiz. 5) g ~ m - ~ ) and 1400 K (0.64 through the sequence Hg? Cd, Zn, ME, Ca, Sr, Ba g cm ) 131. is reflected in the S(0) trend in Fis. 4 (Sr

being, perhaps, a minor exception). Other correct trends are discernable but numerical uncertainity suggests caution at this point. 111

-

_B_I_NAFiY MIXTUES

(i ) Generalities

(5)

C8-430 JOURNAL

DE

PHYSIQUE

Fig. /+(above)

-

Solid (room T) and liquid struct- ures; also S(0) at melting from eq. (2) and ob- served data. Some solid structures vary with T but the distinction between closer and looser pack- ing persists.

Fig. 3(left)

-

Waseda S(q) types: (a) hard sphere, (b) skew peak, (c) shouldered peak.

Group

4

Fig. 5

-

Hafner-Heine potentials (energies: z2e2/~,; lengths: n/k ) .

D

= inter- atomic distance in close packed solid. Arrows denote liquid statg diamgters for

45%

-

50% packing (scarcely distinguishable on this scale).

where S.

.

= S . -

6.

,

and

( 3 )

becomes IJ ~j lj

h. .(r) = c .(I-) + inkjhik(lf

-

EII)ckj(rl)dfl

,

1 J 1 3 ( 9 )

where h.

.

= g - 1

,

and the c. so defined satisfy (cf.

(5)

)

1~ ij l j

c.

.

(r) 2.

-

V.

.

(r)/kgT (large r)

.

(6)

Eqs. (9) transform (cf.

(4))

to

Often, one stresses the concentration variable, c 1131. Consider /I&/

which governs the concentration fluctuations; it is species-sensitive and indicates (by size and sign) the 'chemical short range order1. The corresponding structure factor is

sC,(q)

: clc2 + n jgcc(r)exp(ig.E)

,

for which (cf. (2)) there is a thermodynamic limit /13/

Scc(0) = NkBT/(a2G/ac2)p,T,N

,

(14)

N being the total number of ions and G the Gibbs free energy. Eq. (13) connects, via (12) and ( 8 ) , to the c. /13/ to give

1 j

where f = f(c. .) is simple but longish so is not given here. Eq. (15) is the analogue of (411dnd yields (cf

.

(6)

)

Scc(q) = Scc(0)/(l + (low q)

(16)

Ju$t as S(O) diverges at T

,

so does S (0) at phase separation (PS) and

s ~ ( o )

on compound formation

(~5).

If ~ ~ ~is large (small) we have a PS(CF) ( 0 ) ~ ~ tendency.

(ii) Snn(q) for some binary alloys

\

I .

. - a - . ~ i Pb~.2 ~ . ~ core

\ * \ c1 J r c 1 .J (r)-nvtai1(r)/kBT(17) ij 2 - \

I

.

\

-

1

and find Scc(q) from (15). The

result is governed by an ordering potential

1 tail -

tail + vtaill

.

(18) 'ord = '12 &Iv1 1 22

Fig.

6

shows three measured /14/ S(q)'s. That for the Ca alloy is close to hard sphere form (oscillating; near c1c2) with diameters quite well decided externally from pure liquid considerations. The

I

/ 2

3

c&-I

When, predominantly vord

2

0, like

0

-..

(unlike) neighbour coordination is preferred and there is a PS(GF) tend- Fig.

6

-

Scc(q)/c1c2 for the three alloys ency. This rule emerges by using

near melting. (17), (18) in (15) and writing fcore

(q)

z

f

( q ) /13,15/ and

~z:~(~)

c,c2 to obtain

others illustrate PS and GF tenden- cies; to interpret, we identify cores and tails and, in RPA (cf. (7)), write

3 , -

The general character described above follows when q = 0.

I

I

\

1

Li(;.

6t?

CaO. 32

(7)

C8-432 JOURNAL DE PHYSIQUE

Ab initio calculation of the v is risky both intrinsically (electrontheory un- certainty) and because of errorijaccumulation in (18). Insteadta&tzvand Bhatia /16/ chose hard sphere cores without tails for like ions, so

v12 ord

'

by (181,

and

A

(r < o12)

vord(r) =

{

A(o12/r)exp(- h(r

-

oI2)) (r >

oI2)

(20) 1

With diameters externall~r specified and (arbitrarily) h =

o - ~ ,

the single adjusted parameter A = 3.7 x

lo-'

eV accounts reasonably for Li

-

$a in Fig.

6.

Conversely, transformation of (19) using observed data for leads /15/ to a similar

LiO'~Pb?;$ternally required and picture with

A %

-0.4 eV, h = 1.1

8

and U12sJ, 3

internally satisfied).

(iii) Low q limit of Spp(q)

As in 1I(iv), q = 0 is of interest and some thermodynamically measured data are shown in ~ i 7. (Na ~ .

-

Cs is substituted for Li

-

Na since results for the latter

are not known). Only

vord ! Sv (r)dr, rather than the detail ofO@O), is needed and one findsthat fixed externally pres~rib- ed diameters and v ord = 3.7 eV

8

describes the

whole

curve quite well. But such a parametrisation fails for Li - Pb; e.g. the v required at c = 0.5 is < 20% of t@P at0.8

1191.

The above, unfortunately, lacks a de- pendable electron basis. Pseudopot- ential theory, quite successful in 52 1.0.

0.5

.

. formally applies to alloys but, even if valid, the errors in finding the Fig. 7 - S (0) versus c. Ref.

/ l a /

d ~ t n v.. accumulate in v rd. Here, clearly, interpolat% by present writer. mhhh remains to be 8one.

Acknowledgements I am grateful to my colleagues and coworkers for their influence on this work, to SERC for its support and to Mrs. A. Steven for typing this difficult manuscript.

REFERENCES

/I/ Franz, G., Freyland, W., Glbser,

W.,

Hensel, F. and Schneider,

E.,

J. Physique C8 Q (1980) 194.

/2/ Weeks, J.D., Chandler, D. and Anderson, H.C., J.Chem.Phys.

&

(1971 ) 5237. /3/ McLaughlin, I.L. and Young, W.H., J.Non-Cryst. Sol.

61

&

(1984)

89.

/,!+I ~ e ~ e r , A., Silbert, M. and Young, W.H., Phys.Chem.Liq. 13 (1984) 293 /5/ Evans, E. and Sluckin,

T.,

J. Phys. C Q (1981) 2569, 3 1 3 7 7

/6/ McLaughlin, I.L. and Young, W.H., Phys. Ghem.Liq.

2

(1982) 263. /7/ Meyer, A., Silbert, M. and Young, W.H. Phys.Chem.Liq. Q (1984) 1.

/ 8 / Waseda, Y., The Structure of Non-Crystalline Materials (~cGraw-Hill, New York, 1980),

PP

56, 62.

/9/ Silbert,

M.

and Young,

W.H.,

Phys. Lett.

58A

(1976)

469.

/lo/ Hafner, J. and Heine, V., J. Phys. F

5

(1983) 2479. /If/ Hafner, J. and Kahl, G., J. Phys.

F

2

(1984)

2259. 1121 Silbert, M. and Young, W.H., J.Phys. C

2

(1981) 2425.

/13/ BhatiaA.B. and Thornton, D., Phys. Rev. (1970) 3004; Bhatia, A.B., Liquid Metals 1976, Conf. Series No.30, Inst. of Fhys., Bristol (1977) p. 21.

1141

Chieux, P. and Ruppersberg, H.,

J.

Physique C8 (1980) 145.

/I 5/ Copestake, A.P., Evans, R., Ruppersberg, H. and Schicmacher, W., J.Phys. C

13

1161

Ratti, V.K. and Bhatia, A.B., Nuovo Cim.@ (1978) 1.

-

13 (1983) 1993.

/17/ Neale, F.E. and Cusack, N.E., J.Phys.F

2

(1982) 2839.

/18/ Saboungi, M.L., Marr, M. and Blander, M., J.Chem.Phys.& (1978) 1375.

1191

Bowles, R.J. and Silbert, M.,

J.

Phys.F

2

(1985) L105.

/'

....

c c (%hard spheres) 1 2

----

NacCsl -c /IT/

\

.

Lic Ybl-c /In/

/

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