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HAL Id: jpa-00210269

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Submitted on 1 Jan 1986

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Structural study of Be43HfxZr57-x metallic glasses by X-ray and neutron diffraction

M. Maret, C.N.J. Wagner, G. Etherington, A. Soper, L.E. Tanner

To cite this version:

M. Maret, C.N.J. Wagner, G. Etherington, A. Soper, L.E. Tanner. Structural study of Be43HfxZr57- x metallic glasses by X-ray and neutron diffraction. Journal de Physique, 1986, 47 (5), pp.863-871.

�10.1051/jphys:01986004705086300�. �jpa-00210269�

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Structural study of Be43HfxZr57-x metallic glasses by X-ray and neutron diffraction

M. Maret

(+),

C. N. J.

Wagner (+ +),

G.

Etherington (+ +),

A. Soper

(*)

and L. E. Tanner

(**)

(+) Institut Laue-Langevin, 156X, 38042 Grenoble, France

(+ +) Materials Science and Engineering Department, University of California,

Los Angeles, California 90024, U.S.A.

(*) Los Alamos National Laboratory, Los Alamos, New Mexico 87545, U.S.A. (1)

(**) Lawrence Livermore National Laboratory, University of California, Livermore, California 94551, U.S.A.

(Rep le 23 septembre 1985, révisé le 27 dgcembre 1985, accepti le 10 janvier 1986)

Résumé. 2014 Les facteurs de structure partiels de Faber-Ziman des amorphes Be43HfxZr57-x sont calculés à partir

de la combinaison d’une mesure de diffraction neutronique en temps de vol dans l’alliage avec x = 25 at % et trois

mesures de diffraction X dans les alliages avec x = 5, 25 et 54 at % en utilisant la substitution isomorphe entre

les atomes d’hafnium et de zirconium. Les facteurs de structure partiels de Bhatia-Thornton sont ensuite déduits.

A partir des fonctions de distribution radiale partielles, les nombres de coordination partiels sont calculés et per- mettent de déterminer le paramètre d’ordre chimique généralisé de Warren 03B11 dans la première couche de coor-

dination. Le rayon extérieur de la première couche est bien défini par la position du premier minimum de la fonc- tion GNN situé à 3,8 A. Nous trouvons ainsi une valeur de - 0,033 pour 03B11, qui montre une faible tendance de mise en ordre chimique.

Abstract. - The Faber-Ziman partial structure factors of the Be43HfxZr57-x glasses are calculated from the com-

bination of one time-of-flight neutron diffraction measurement in the alloy with x = 25 at % and three X-ray dif-

fraction measurements in the alloys with x = 5, 25, and 54 at % using the isomorphous substitution between Hf and Zr atoms. The Bhatia-Thornton partial structure factors are then deduced. From the partial radial distribution functions the partial coordination numbers are calculated and allow the generalized Warren chemical order parameter 03B11 in the first coordination shell to be determined. The upper radius of the first shell is well defined by

the position of the first minimum of the GNN function located at 3.8 A. Thus, we find a value of - 0.033 for 03B11 which indicates a slight tendency of chemical ordering.

Classification Physics Abstracts

61. lOF - 61.12D - 61.40D

1. Introduction

Binary

BeHf, BeZr and BeTi, and ternary BeHfZr and BeTiZr

amorphous alloys

have been

produced by ultra-rapid liquid quenching

for

composition

ranges

surrounding

the

respective

eutectics 34 at

%

Be-Zr, 33 at

%

Be-Hf and 37.5 at

%

Be-Ti. All these

glasses

but BeTi are

readily

fabricable in continuous ribbon form and

they

are of

particular

interest because of their

good

mechanical

properties,

such as

high specific strength [1].

A detailed

understanding

of the

mechanical or

magnetic properties

of metallic

glasses requires

structural information.

In this paper, we present the determination of the

local structure of the

Be43HfxZr57-.

ternary

glasses

which is

basically

described

by

a set of six

partial

structure factors

IiJ{K).

However the Hf and Zr elements have similar metallic atomic radii

(rw =

1.585

A,

rZr = 1.597

A)

and possess the same

hcp

structure; moreover

they

exhibit a similar chemical

behaviour when

alloyed

with Be, characterized

by

very close eutectic

compositions

(as

specified above)

and the same intermetallic

compounds Be2Hf(Be2Zr)

and

Be5Hf (BesZr).

For these reasons, we can assume

that zirconium and hafnium are

isomorphous

ele-

ments in the BeHfZr

glasses.

Then we may treat the ternary glasses

Be43HfxZr57 - x

as

pseudo-binary glas-

ses, formulated

Be43MT 57 (MT

= Hf or

Zr).

Conse-

quently

their structure is

simply

described

by

three

partial

structure factors

(PSF).

For the determination of PSF’s we use the

isomorphous

substitution method.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004705086300

(3)

864

This method was

already applied

for extracting partial functions from X-ray

experiments,

such as in

La (AIGa) glasses

[2] or

Ni (ZrHf) glasses

[3] Janot

et al. [4] have also used this method for neutron

experiments

in the

pseudo-ternary (FeMn),5P,5clo

glass. Since Fe and Mn have coherent scattering

lengths

of opposite signs, the substitution between Fe and Mn

drastically

changes the contrast between metal and metalloid atoms and

consequently,

the

weights

of

the

partial

functions in the total interference function.

When

using only

X-rays, the contrast

brought by

the

isomorphous

substitution method is insufficient to extract all the

partial

structure factors, and

generally

this method is

applied

with a combination of X-ray

and neutron measurements [3]. Moreover, it is often

judicious

to check the

consistency

of the

partial

structure factors extracted from three measurements

by

redundant measurements.

For the structural

analysis

of the

Be 43 HfZr . 57-., glasses,

we

performed

three X-ray diffraction

experi-

ments in the

alloys

with x = 5, 25 and 54

%

which correspond

approximately

to the minimum, maximum

and intermediate

compositions

in hafnium. Since the

light

element (Be) is not visible

by

X-rays, we

realized one

time-of-flight

neutron

experiment

in

the

Be43Hf25Zr32 amorphous alloy

which is the most

easily

fabricable

glass

in ribbon form. From the four total interference functions, first the Faber-Ziman par- tial structure factors

Iij(K)

are determined, and then the Bhatia-Thornton functions are deduced from

Iij(K).

The calculation of all the

partial

coordination numbers from the radial distribution functions

RDFij(r)

are

performed,

estimates of some of them

were

previously given by

us in

[5].

Finally

the

generalized

Warren chemical parameter ai is calculated in the first coordination shell, and an

extension of this parameter is

proposed

for

describing

the chemical

ordering

as a function of the distance r.

2.

Experimental technique

and data

analysis.

The ribbons of

Be43Hf,,Zr,7-,, glasses

35 J.1m thick and 1.5 mm wide were

prepared by

the

melt-spinning

process. The average atomic

density

of these ternary

glasses

is taken

equal

to 0.0565

at/A3 (value

of the

Be43Zr57 glass

measured

by

Tanner et al.

[1]).

We

checked that this value was in agreement with those deduced from the

slope

of the reduced distribution functions

G(r)

at small r.

2. 1 X-RAY DIFFRACTION MEASUREMENTS. - The scattered X-ray intensities of the

alloys

with x = 5, 25 and 54 at

%

were measured in transmission

using AgKa

radiation

(with A

= 0.5594

A)

in the conven-

tional

scanning

20-method, described in

[6].

The

X-ray samples

were formed

by sticking

ribbons

parallel

to one another, thus

covering

the whole

opening

of the holder of 12.5 x 12.5 mm2. The

samples

were

placed, initially perpendicular

to the incident

beam, in a vacuum chamber for

minimizing

air

scattering.

X-ray diffracted were selected

by

a

Si(Li)

solid-state detector in

conjunction

with a

single

channel pulse height analyser which permitted removal

of the white spectrum, the fluorescent radiation and a

large

part of the Compton

scattering.

Raw data were

registered

on a multichannel

analyser

for diffraction

angles

between 20 and 1000 in step of 0.250. The measured intensities were then corrected for

sample absorption, polarization,

and

Compton scattering,

as

described elsewhere in

[7].

The values of

Compton scattering

were calculated for Hf and Zr from the ana-

lytic expressions given by

Palinkas

[8]

while those of Be were

interpolated

from the tables of Cromer

et al. [9]. The normalization of the scattered intensities

was done using the sum rule of the interference function

I(K)

which

yielded

the coherent

scattering

per atom

Ia(K).

2.2 NEUTRON DIFFRACTION MEASUREMENT. - The

time-of-flight neutron diffraction measurement on the

Be43Hf25Zr32

glass was

performed

on the General

Purpose Diffractometer at the

pulsed

neutron

spal-

lation source of the WNR

Facility

in Los Alamos,

utilizing

the

high epithermal

flux to extend measure-

ments to

higher

values of K than are

possible

with

conventional neutron sources. We recall the relation between the

scattering

vector K and the

time-of-flight

of neutron t(À)

given by :

where mn is the mass of neutron, h is Planck’s constant, 2 0 the

scattering angle, Lo

the incident

flight path

between the moderator and the

sample

and L the

diffracted

flight path

between the

sample

and the

detector.

The neutron specimen was prepared

by

wrapping

melt-spun

ribbons around a frame such that the final

shape of the

sample

was a

cylinder

of 6 mm diameter

and 6 cm

height.

The mass of

wrapped

ribbons

(5.7 g)

and the

cylinder

volume lead to an effective atomic

density peff

of 0.026

at/A’.

This value was used for the calculation of the

absorption

and

self-shielding

coef-

ficients. The scattered

intensity

was measured

by

three banks of 16 detectors each, located at the average

scattering angles

of 1 4.4°, 40.5° and 1 5 1 . 1 ° and

covering respectively

the

K-ranges

of 0.5 to 5

A-1,

1.4 to

10 A-’ and 7 to 25 A -1

(the

upper limits were deter- mined

by

a strong resonance of Hf around an incident energy of 1 eV). The neutron data of each bank were

separately

corrected first for

background, sample absorption, self-shielding

and

multiple scattering.

The correction factors for

absorption Aa(6, R)

and

self-shielding ASS(8, R)

are calculated

using

the relation

for

cylinders given by

Rouse et al.

[10] ; they

are

function of the radius of the

sample cylinder

R, the

effective atomic

density peff

and the

absorption

cross-

section for

Aa(9, R)

or the total

scattering

cross-

section for

ASS(e, R).

Data were then corrected for incoherent

scattering

and for deviations from the static

approximation using

Placzek’s method, which

(4)

was

applied by

A. C. Wright [11] to

time-of-flight

measurements for a detector with an

energy-dependent efficiency.

The

efficiency

of He3 detectors is repre- sented

by

1 -

exp( -

0.794 A). In table I, we

give

the

coherent scattering

lengths,

the incoherent and

absorp-

tion cross-sections for the pure elements taken in the data

analysis.

The

scattering

from a vanadium rod of known incoherent

scattering

allowed, on the one hand, to determine the incident neutron spectrum necessary for Placzek’s correction, and on the other hand to normalize the scattered

intensity

of the

Be43Hf2sZr 32

glass. The

overlappings

of the normalized intensities of the detector banks at 14.40 and 40.50, and of the

banks at 40.50 and 151° was checked

by complemen-

tary neutron measurements on the same

sample

res-

pectively

on the DIB and D2 spectrometers at the HFR at the ILL in Grenoble,

using

the

respective wavelengths

of 2.52 and 0.94 A. A

supplementary

cor-

rection was

applied

to remove incoherent

scattering

due to the presence of

hydrogen

in the ribbons.

Using

the values for differential

scattering

cross-section of an

H20

molecule measured

by Beyster [12]

a

hydrogen

concentration of about 2 mol

%

was evaluated to

account for the observed

background.

3. Results and discussion.

3.1 TOTAL INTERFERENCE FUNCTIONS AND PAIR DISTRI- BUTION FUNCTIONS. - When

using

the Faber-Ziman formalism [13], it is usual to define the total inter- ference function I(K) from the coherent

scattering intensity

per atom,

I.(K), by

the

following

normaliza-

tion :

where

,fi

are the atomic

scattering amplitudes (called bi

for

neutrons, and

fMT = (xjf

+ (57 - x)

fZr)/57). Ci

are

the atomic concentrations

(note CMT

=

0.57).

I(K)

is a linear combination of the three

pair partial

structure factors

I ij( K).

Table I. - Values

of

coherent scattering lengths,

incoherent and

absorption

cross-sections (given

for

A = 1.8

A) for

the Be, Zr and Hf elements.

In some cases the Bhatia-Thomton formalism [14] is

more

advantageous

and the total interference function

or total structure factor, noted

S(K),

which is a linear

combination of the three number-concentration struc- ture factors

SN,c(K),

is obtained

by

the

following

normalization :

and

with

The normalization

(3)

is more

general

than the norma-

lization

(1),

since it is still

applicable

to a zero

alloy (i.e. when b > = 0).

The relation between I(K) and S(K) is given

by :

The contribution of each PSF in the total interference function

I(K)

or

S(K)

is

strongly dependent

on the

value of the

Wij

factors. In table II, we

give

the values

of

Wij

in both formalisms for the different glasses

studied when

using X-rays

or neutrons.

Figure

1 shows the

I(K)

functions for the

melt-spun alloys

obtained from X-ray

(Ix(K))

and neutron

(IN(K»)

data. It is clear from table II that the

IX(K)

functions are dominated

by

the MT-MT pairs, while

the contribution of

IBeBe(K)

can

always

be

neglected.

The three X-ray curves are identical and present a well defined first

peak

at 2.56 Å -1. The neutron curve

IN(K)

is

equivalent

to

SNN(K),

because

IN (K)

and

SN(K)

are

Table II. - Values

of the Wijfactorsfor

the

Be43HfxZrS7-x

glasses using

X-rays(XR) for

K = 0, and neutrons (N).

(5)

866

Fig. 1. - Total interference functions I(K) of the Be43HfxZrs7-x glasses measured by X-rays for x = 5, 25, 54 at % and by neutrons for x = 25 at %.

identical since the ratio

b )2/ b2 )

in

equation (5)

is

equal

to 0.9994 and the co-factors

WNc

and

Wcc

are

very small in the

SN(K)

function

(see

Table

II).

The

first

peak

of

IN (K)

is centred at 2.69 Å - 1 and a small

prepeak

can be observed around

1.4 A-1;

the shift

of the first

peak

to

higher

K,

compared

to this one of

IX(K),

results from the

larger

contribution of the Be- MT

pairs.

The uncorrelated La.ue term

f ’ > _ f >2

in the normalization

(1), equal

also to

CBe CMTCfBe - fMT)2

is

large

for

X-rays

and almost

negligible

for

neutrons

(see

values of Table

I).

It

explains

the diffe-

rence in

sign

of the limits

Ix(O)

and

IN(0) .

The Fourier transform of

K [I(K) - 1] yields

the reduced distribu- tion function

G(r) :

Figure

2 shows the curves of

G(r)

for the

Be43Hf2sZr32 glass

obtained from

X-rays

and neu-

trons,

using

the upper

integration

limits of 15.45 Å - 1

and 15.15 Å -1

respectively.

These values

correspond

to nodes in the

K(I(K) - 1)

functions.

Fig. 2. 2013 Reduced distribution functions G(r) of the Be,3Hf,,Zr3l glass obtained from X-rays and neutrons.

The three

G X (r)

functions

(only

one

shown)

are

identical with a first

peak

at 3.18

A,

which

corresponds

to the MT-MT interatomic distances. This confirms the

isomorphous

behaviour of the Hf and Zr elements.

The

G N(r)

function shows the

splitting

of the first

peak

into three maxima at 2.2, 2.72 and 3.15 A. Since these three distances are very close to those found in the

Be2Hf

or

Be2Zr compounds (see

Table III),

they

must

correspond respectively

to the first BeBe, BeMT and MTMT interatomic distances. Such a

splitting

is

quite

seldom because it

requires

an

important

size effect and atomic concentrations close to 50

%.

3.2 PARTIAL STRUCTURE FACTORS AND ATOMIC CORRE- LATION FUNCTIONS. - The

partial

structure factors

cannot be obtained

simultaneously by solving

a system of three linear

equations

such as

(2)

or

(3),

chosen among the four total interference functions,

because any combination

yields

a very small deter- minant of the matrix formed

by

the factors

Wij.

Therefore, we used the

following procedure concerning

the Faber-Ziman formalism :

- first, the function

IMTMT(K)

is derived from the

Ix(K) 1

function of

Be43HfsZrs2

and

I;(K)

of

Be43Hf54Zr3 by neglecting

the contribution of

I BeBe (K).

- then the function

IBMT(K) is

determined from the two other interference functions

Ix(K)

and

IN (K)

of

Be43Hf25Zr32,

and the

partial

function

IMTMT(K), using

an

algorithm

similar to the one

proposed by

Edwards et ale [ 15] ;

-

lastly,

the function

IB.B.(K)

is deduced from

(6)

IN(K),

when

knowing

the two other functions

IMTMT(K)

and

IBw(K).

The Bhatia-Thornton PSF

are deduced from the

IiJ{K)’s using

the well known

linear relations

given

in

[14].

- Faber-Ziman formalism :

The function

ImTmT(K),

shown in

figure

3,

strongly

resembles the

I’(K)’s

with a first

peak

centred at

2.55 Å - 1 .

The two other functions

IBeBe(K)

and

IBeMT(K)

which are obtained

by solving

the two linear

equations

formed

by I3X(K)

and

IN(K)

and

using

the values of

IMTMT previously

determined, exhibit very

large

oscilla-

tions and cannot be retained.

Indeed it is necessary to take into consideration the

errors of

13 (K),1N(K)

and

IMTMT(K).

The solutions of

IBeMT(K)

and

IBeBe(K)

are then

given by :

A-1 is the inverse matrix of A =

the coefficients are relative to x = 25 at

%.

After the data treatment, we estimate the relative

errors in the total interference function at 6

%.

This

quite large

error takes account the absence of cor-

rections for the different resolution in K of the three banks of detectors of the

time-of-flight

spectro-

meter and also for the different resolutions of X-ray

and neutrons methods.

By neglecting

errors in the co-

factors

Wij,

the absolute error in

IMTMT(K) is equal

to

±

(I

(XII 0.06

1 lx(K)

I +

I (X12

0.06

If(K) I).

x 11

and a12

are the inverse matrices formed

by

the factors

Win

related to

I1X(K)

and

I2X(K).

For instance, at

K =

10 A-1,

an = - 1.36 and (Xt2 = 2.36 and the

error in

IMTMT(K)

is

approximately

22

%.

In the solution

(6), bx(K), 6’(K)

and

bmT(K)

are

allowed to vary

respectively

between ±

0.06 1 Ix(K) [

±

0.06 I IN(K) I

and

We

keep

the solutions of

IB,,MT(K)

and

IBeBe(K)

obtained

by equation (6)

which both fall inside the range defined in

figure

4 and check the

following inequalities :

and

For each K an average value of these retained solu- tions is calculated. The function

IBeMT(K),

so obtained,

is shown in

figure

3 and presents a minimum at 2.2 Å - 1 and a first

peak

at 2.75 Å - 1. The oscillations of the function

IBeBe(K)

evaluated

by

the same pro- cedure

damp

down too

rapidly;

so it is better to

finally

deduce

IBeBe(K)

from

equation

(2)

using

the

values of

IN(K), IMTMT(K)

and

I...(K).

The function

IBeBe(K)

exhibits a

prepeak

around 1.70

Å -1,

which

Fig. 3. - Faber-Ziman partial structure factors

Iij(K)

of the Be43HfxZr S 7 - x glasses.

indicates a

pseudo-periodicity

Be-MT-Be, and a first peak centred at

3.4 Å - 1.

The limits of the

partial

functions relative to homoatomic

pairs

are

negative,

while the limit of the function relative to heteroatomic

pairs

is

positive;

these features characterize

chemically

ordered systems

(such

NiB [16] or NiTi

[17] glasses).

For

liquid alloys

these limits are related to the thermo-

dynamic

data

[18].

We must

precise

that the functions

IB.B. (K)

and

IB.mT(K)

shown in

figure

3 are

only

(7)

868

Fig. 4. - Range of allowed structure factors versus K.

approximate

solutions. The Fourier transforms of

IMTMT(K), IBeMT(K),

and

IBeBe(K),

calculated with the upper

integration

limits of

13 Å - 1,

12.9 Å - 1 and

9.4A-’

respectively, yield

the reduced atomic

pair

distribution functions

GiJ{r),

shown in

figure

5. The

partial

radial distribution functions are then deduced from

Gij(r) by :

The fitting of the nearest

neighbour regions ofRDFij(r)

by

Gaussian components

(as

shown in

Fig. 6) permits

to divide the first shell into sub-shells and also to

Fig. 5. - Reduced atomic pair distribution functions

Gij(r)

of the Be43HfxZrs-x glasses.

Fig. 6. - Partial radial distribution functions

RDFij(r)

of

the Be43HfxZr 57 - x glasses and Gaussian components of the

nearest neighbour regions.

discard the

spurious ripples

due to the truncation in the Fourier transform, such as the oscillation of

RDFB.mT(r)

around 2.2 A. The

partial

coordination number

4r)

are calculated from the

height

and the

width at

half-height

of the Gaussian

peaks

centred at

rT).

The values of

ziP

are summed up in table III. For

comparison,

the interatomic distances and the coor-

dination numbers found in the

crystalline compounds Be2Hf

and

Be2Zr

are also

given

in table III. The lattice constants of

Be2Hf

and

Be2Zr

with the

hexago-

nal

AIB2

structure type are

respectively

ao = 3.786

A,

Co = 3.163 A

and

= 3.81

A, co

= 3.23 A.

The distribution of the first

pairs

BeBe is

quite large

and can be divided around the

positions

2.2 and

2.86 A.

Concerning

the distribution of the first

pairs

BeMT and MTMT,

they

are

asymmetric

and can be

represented by

two Gaussians; nevertheless the

posi-

tion of the small second Gaussian is

certainly

affected

by

truncation errors in the Fourier transform. It can

be also noted that there is an inversion of the coordina- tion numbers

ZgtMT

and

z(2)MTMT

between the

glass

and

the

crystalline compounds.

In average, the distance

(8)

Table III. - Interatomic distances and coordination numbers in the

Be43HfxZrS7-x

glasses and the

crystalline compounds Be2Hf

and

Be2Zr.

(*) Errors are only related to the Gaussian parameters and do not account for the inaccuracy of the

RDFij

functions.

Fig. 7. - Bhatia-Thornton partial structure factors

SN,c(K)

of the Be43HfxZrs7 -x glasses.

MTMT is shorter in the amorphous phase than in

Be2Hf

or

Be2Zr compounds.

As shown in table III, the first interatomic distances in the

Be43Hf,,Zr57-x glasses

are very close to those of the

crystalline compounds Be2Zr

(or

Be2Hf),

except for the distance BeBe at 2.86 A which lies

between the distances of 3.16

(or

3.23

A)

in

Be2Hf (or Be2Zr)

and 2.635 A of the

crystalline compound Be5Zr.

- Bhatia-Thornton formalism

The Bhatia-Thornton number-concentration struc- ture factors

SN,c(K)

are deduced from the

Iij(K)’s

using the linear relations in

[14],

and shown in

figure

7.

The

equivalence

between

SNN(K)

and

IN(K)

is well

checked, with a first

peak

in

SNN(K)

at 2.69 A-1

and a

prepeak

around 1.4 A-1. The first

peak

of

Scc(K)

is

quite pronounced,

centred at

2.3 A - I ;

the oscillations of

SNC(K)

around zero reflect the size effect between the two atomic

species

but remain weak

compared

to those of

SNN(K)

in

spite

of a

high

ratio

of atomic radii of 1.4.

The Fourier transforms of

K[SNN(K) - 1], K[Scc(Kl ’ 1]

and

KSNc(K),

are calculated with truncation values of 15, 11.4 and 13 A-1 respectively,

which

correspond

to nodes in these functions. The number-concentration correlation functions

GN.c(r),

so obtained, are

presented

in

figure

8. The function

GNN(R)

is similar to

GN(r) ;

the maximum of

GNN(r)

at

2.72 A

corresponds

to a minimum in

Gcc(r)

better

pronounced

than the positive

peaks

at 2.3 A and 3.17 A

indicating

a

preference

for unlike atom pairs.

3.3 CHEMICAL SHORT-RANGE ORDER

(CSRO)

PARA-

METER. - The

generalized

Warren CSRO parameter

a1 relative to the first shell is

given according

to [6]

by :

where

zie

and

zMT

are the total coordination numbers of each species. The value pf ai is

directly dependent

on the way of

defining

the shell of the first

neighbours,

(9)

870

Fig. 8. - Number-concentration correlation functions

GN,,(r) of the Be,, Hf.Zrl 7 -., glasses.

since the numbers

zij

are, obtained from :

The upper radius of the first shell,

r’,

is defined

by

the abscissa of the first minimum of

GNN

located at

3.8 A. The lower limits

r""

allow to discard the

spurious ripples

in

RDFJ. Using

the

integrand (9)

with rl = 3.8

A, I Z1BeMT

and

z1MTMT

are

equal

to 4.2,

7.4 and 8.2

respectively.

Thus, a1 is

slightly negative

with a value of - 0.035. This value is very different from - 0.16, our

previous

estimate, which was deduced from a function

ARDF(R) containing

both

contributions of BeBe and BeMT and calculated for a

first shell limited at

3.4 A (radius

defined

by

the

position

of the first minimum of

ARDF(r)).

This

discrepancy clearly

shows that the limit of the first shell

largely

influences the chemical short range order parameter ai.

The value of - 0.035 for the

Be4:5Hf ., Zr 5 7 -., glasses

is similar to that calculated for the

Be37.5Ti62.5

Fig. 9. - Evolution of the generalized Warren chemical

order parameter a(r) as a function of r.

glass [19]

with

partial

coordination numbers

equal

to

ZB.B. = 2.9, ZB.TI = 6.9 and ZTiTi = 8.

In this series of

glasses,

the chemical

ordering

is weak

compared

to those

existing

in metal-metalloid

glasses :

(Ni8oB20 [16])

or, metal-metal

glasses (Ni33 Y 67 [20]).

We must

emphasize

that in most

previous

structural

studies of metallic

glasses,

the

zi’j

numbers are calculat-

ed with different upper

integration

limits

r’

which

correspond

each to the

position

of the first minimum in

RDFiï

If the two

species

are different atomic radii,

the three minima do not coincide with the minimum of

GNN

and

consequently,

the CSRO parameter ai calculated with

specific r1ij

can be somewhat different from the value obtained with a

unique

value rl.

Therefore for

binary

systems with strong size effect,

the

importance

of the chemical

ordering

and its

extent could be described

by

a function

a(r)

defined

in the same way as al, i.e. :

with

Figure

9 shows the variation of

a(r)

for the

Be43HfxZrs7_x glasses.

Between 3 and 4.25 A

a(r)

is an

increasing

function, which becomes

positive beyond

3.9 A. The oscillations of

a(r)

around 0

damp

down

rapidly beyond

4.5 A and it shows the local

character of the chemical

ordering.

This function could be

easily

used for a

comparison

of chemical

orders in different

glasses.

Acknowledgments.

This research was

supported

in part

by

grant DMR80- 07939 and 83-10025 from the National Science Foun- dation. Thanks are due to the WNR

Facility

in Los

Alamos and to the Institut

Laue-Langevin

for the

allocation of beam time at their

respective

neutron

sources.

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