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Atomic displacements in low temperature irradiated chromium crystals

M. Biget, F. Maury, P. Vajda, A. Lucasson, P. Lucasson

To cite this version:

M. Biget, F. Maury, P. Vajda, A. Lucasson, P. Lucasson. Atomic displacements in low temperature irradiated chromium crystals. Journal de Physique, 1979, 40 (3), pp.293-298.

�10.1051/jphys:01979004003029300�. �jpa-00209108�

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Atomic displacements in low temperature irradiated chromium crystals

M.

Biget,

F. Maury, P.

Vajda,

A. Lucasson (*) and P. Lucasson

Bât. 350 (**), Université Paris XI, F 91405 Orsay, France (Reçu le 26 septembre 1978, accepté le 23 novembre 1978)

Résumé. 2014 Nous avons irradié des échantillons monocristallins de chrome parallèles aux plans (100), (110) et (111),

avec des électrons d’énergie comprise entre 0,48 et 1,7 MeV. Nous avons trouvé que l’énergie seuil de déplacement atomique est sensiblement la meme dans les deux directions cristallographiques ~100~ et ~111~ bien

que

les

mécanismes de déplacement soient vraisemblablement différents. Nous avons étudié le recuit des défauts créés, après irradiation à 0,525 MeV (jusqu’à 60 K), 0,5 et 0,75 MeV. L’anisotropie des premières sous-étapes de recuit présente plusieurs points communs avec le recuit du tungstène dans le même domaine de température. Nous suggérons une interprétation des différentes sous-étapes jusqu’à 40 K.

Abstract. 2014 Monocrystalline specimens of chromium, cut parallel to the (100), (110) and (111) planes, have been

irradiated with electrons in the energy range 0.48-1.7 MeV. The threshold energy for atomic displacement is found

to be about equal in the two crystallographic directions ~ 100~ and ~ 111~ , although the mechanisms for displa-

cement may be quite different in the two cases. The recovery of the defects has been studied up to 60 K, and after irradiations at 0.5,0.525 and 0.75 MeV. The anisotropy of the different substages appears to bear some resemblance to the low temperature recovery of tungsten. A tentative attribution is given for the various substages up to 40 K.

Classification Physics A bstracts 61.80F - 61.70E

1. Introduction. - This work is part of an extensive study of Frenkel defect creation and recovery in bcc metals [1]. This study has been undertaken in order to obtain some information on the threshold energy surface for atomic

displacements

in bcc

crystals,

and

check whether this surface would

depend

on the

particular

metal under consideration. Results have been obtained in the cases of Mo [2, 3], a-Fe [4], Ta [5]

and W [6]. For all these metals, the threshold energy for atomic

displacement

has been found to be mini-

mum in the ( 100 > direction in agreement with the first

experimental

data of Lomer and Pepper

[7]

as

well as with the results of the Brookhaven

computation

group [8]. On the other hand, the threshold energy in the ( 111 > direction has always been found to be

relatively

lower than that

predicted

by the compu- tations on iron

[8],

the ratio

Td’ IT100> varying

from 1.05 in the case of W to 1.3 in the case of Mo.

The ratio of the threshold

energies

in the ( 100 )

and ( 111 ) directions is a

significant

parameter which

might

account, at least

partly,

for the differences in the stage 1 recovery spectrum, observed in different bcc metals : it may directly influence the relative

populations

of the various substages. Moreover, it

may be

indirectly

related to the stage 1 recovery spectrum by the fact that, like the interaction between interstitial and vacancy

specific

to each Frenkel

pair configuration,

it

originates

from the interatomic

potential particular

to each metal. Very little is

known about low temperature irradiated chromium.

To our knowledge the only

existing

data have been obtained in our group [9] on

polycrystalline specimens.

A

single-step displacement probability

function P(T)

with a

unique

threshold at 28 ± 1 eV could account for the defect

production

rate up to a transmitted energy Tm l"to.I 100 eV. The recovery spectrum has been studied from 10 to 60 K. Distinct peaks showed up below 40 K ; yet, as for other bcc metals (W, for

example),

it was not

possible

to determine exactly

the end of stage 1 since no long range

migration

was

evident below 60 K.

2. Expérimental. - The

specimens

were

prepared

from a zone-refined chromium bar obtained

by

the

courtesy of J.

Bigot (CECM-Vitry,

France)

[10].

Several

grains

with their axes

parallel

to ( 111 ) and (110) were detected by a systematic X-ray explo-

ration of the bar and then cut out of it. The

slicing

was

performed

with a

goniometric

adaptor described in reference [11]. The final thickness was achieved by

mechanical

polishing,

followed by

electropolishing

in a mixture of 95 %

CH3COOH

+ 5 % HCI04. No

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01979004003029300

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294

Table 1. - Specimen characteristics

The tickness of the samples was measured at both ends (xi, x2) and in the middle of the sample (xm) with a micrometer. A mean thick-

ness was deduced either by weighing the sample or from its measured resistance. XFOR is the mean thickness which has been used in the cal- culations. 3l is the measured resistivity ratio between room temperature and liquid helium.

anneal was

performed

before irradiation. The different characteristics of the samples are listed in table I.

An indication of the

purity

is

given by

the

resistivity

ratio A (see Table I), the main

impurities being

Fe (10

ppm)

and N (10

ppm) (cf.

Ref.

[10]).

As can be seen, the thickness of the

samples

is

highly

non uniform, the

samples being

thinner at both

ends

(xi, x2)

than in their middle

(xm).

Since the very ends of the

samples

are not irradiated, this will lead

to an underestimate of the radiation-induced

resistivity

calculated from the measured resistance.

On the other hand, the length of the (111) sample (4 mm) was shorter than the total irradiated

length

(5 mm) ; in consequence, part of the

sample

holder (a copper foil of 50 gm covered with

superconducting

soft solder) was irradiated, thus

resulting

in an extra

heating

of the

sample.

The irradiation temperature

was controlled in a first series of irradiations by

measuring

the resistance of the irradiated poly-

crystalline sample

(its mean temperature

during

the irradiations,

Ti,

was

kept

around 9 K) and in a

second series of irradiations

(performed

at a lower

temperature)

by

measuring

the

resistance

of the (111)

sample

(its mean temperature T; was kept between 6

and 7 K). Note that the weak

points

at the ends of the

samples

may be another cause of extra

heating.

Experience proved

(cf. section 4) that,

during

the

first series of irradiations,

samples

(100) B and (110) A

were irradiated at a

higher

temperature than

samples

(100) A and (110 B).

The

annealing

studies were

performed in

situ

by heating

the entire

sample

chamber and

monitoring

the temperature by means of a

platinum

resistor. All

resistivity

measurements were made at 4.2 K with a

sensitivity

of 1 x 10- 11 Q cm.

3. Defect production. - 3. 1 EXPERIMENTAL RE- SULTS. - Two series of irradiations were

performed

in the energy range 0.48-1.7 MeV. The results of the second one only will be presented here since a fraction

of the defects was lost

during

the first run (because of

overheating).

The first

thing

to note is that the pro- duction rate remained constant (within the measuring

sensitivity),

with the incident electron fluence, even at

the lowest electron energies. This means that the sub-

threshold defects play a

negligible

role in the total

damage

production. Moreover, - 85 % of the defects

recovered below 40 K after irradiation at 0.5 MeV ; this percentage decreased to - 60 % after

irradiating

at 0.75 MeV : these numbers are

quite

comparable

to what is usually obtained in other metals when no

subthreshold damage is observed

(see

e.g. Ref.

[2]).

The

experimental production

rates are

plotted

in

figure

1 for the four

samples

(100) A, (100) B, (110) B

and (111), as a function of the electron energy. The

production

curve measured for the

polycrystalline

sample reproduced closely that obtained before [9]

and is not

given

here. The

uncertainty

due to the

electrical measurements lies between 1 and 2 %.

Most of the

uncertainty

on the

experimental points

comes from

possible

variations of the electron beam

profile

in conjunction with the thickness inhomo-

geneity

of the

samples,

and from uncontrolled

overheating (particularly

for the (111)

sample).

3.2 DATA ANALYSIS. - Since the radiation-induced

resistivity

may be underestimated

(by

an amount

which may vary from one sample to the other) due to

a wrong evaluation of the

shape

factor for the irradia- ted part of the

sample,

it would be

meaningless

to try

to determine the exact

shape

of the threshold energy surface, and even to try to determine the relâtive

opening

of the lenses

(regions

of low threshold ener-

gies

around the main

crystallographic

directions) in a

classical

geometrical

model. Therefore, we adopted a

threshold energy surface which has been

directly

deduced from the results of

Erginsoy et

al.

[8]

on iron,

the same that we had used for Mo [3].

Two

regions

of low threshold energy were consi- dered around the ( 100 ) and 111 ) directions, and treated like square

potential

wells with radii of 22°

(4)

Fig. 1. - Induced resistivity change rates as a function of the incident electron energy for four samples ; the crosses are the experimental points, the curves are calculated with :

The PF values used for normalization are indicated on the figure.

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296

and 240

respectively.

Outside of these

100 )

and ( 111 ) lenses, the threshold energy was

arbitrarily

fixed at 95 eV (which

corresponds

to an incident

electron energy of 1.1 MeV). The exact value of this parameter is of little

importance,

since it will influence the calculated production curves only at high energies where, in any case, the model is not

supposed

to be as

valid because of the occurrence of

multiple displa-

cements. Thus we remain with two parameters

only,

which are the threshold

energies

in thé ( 100 ) and 111 > directions,

T¿100>

and

T¿lll>, plus

a norma-

lization factor for each

production

curve which should be

equal

to the Frenkel

pair resistivity,

pF - if the radiation-induced

resistivity

has been estimated cor-

rectly - or less than PF - if it has been underestimated

(cf. section 2).

The calculation of the

displacement

cross-sections with this model has been described in detail in refe-

rences [3] and [4].

The calculated

production

curves are drawn in

figure

1 with 3 sets of parameters :

The calculated curves have been normalized to the

experimental

ones in the medium energy range where the model is

supposed

to be still valid (not too many

multiple displacements)

and the corrections for energy loss and beam

straggling

are not too

important.

We can see that

Td"’>

= 29 eV leads to

production

rates

definitely

smaller than the

experimental

ones at

low

energies

for the (100) samples; in the same way

Td "’ >

= 27 eV leads, for the (111) sample and at

low

energies,

to

production

rates

systematically larger

than the measured ones.

The best fit is obtained with

Td’00> =

27.5 ± 1 eV

and

Td"’> =

28.5 ± 1 eV. These two values are

nearly

equal,

as in the case of W [6]. This result will not depend much on the assumed threshold energy surface, but the

general shape

of the curves will

depend

on it. The agreement between the

experimental

and calculated data is

surprisingly

good,

especially

for the (100) samples : it is to be noted that the calcu- lation reproduces even the difference in the shape of

the

production

curves for the two (100)

samples

between - 0.5 and 0.7 MeV, as a consequence of their different mean thicknesses.

One may wonder why so crude a model leads to such a good fit. We see two reasons for that : - at low

energies,

the beam is so

widely spread

that - in the

directions of easy

displacement

- it covers the whole

of the

corresponding

lens ; thus

taking

a mean value

of the threshold energy for the whole lens will be a

good

approximation.

The

approximation

should not

be

quite

as good for the (110) sample.

At high energies the equality of the two thre-

sholds

Td’00>

and

T¿lll>

(which means that the crystal is fairly

isotropic)

is a very favourable case,

allowing mutual

compensations

when

multiple displa-

cements take place.

The obtained value for PF lies between 25 and 39 gÇl cm/at

%

F.P., the most

likely being

- 37 gn cm/at %. Of course, this value will

depend

much on the threshold energy surface and will decrease if one increases the size of the low-threshold energy

regions.

These conclusions are in good agreement with the

polycrystalline

results. There, we had found that a

displacement probability

function

with PF = 40 gfl cm/at %,

fitted well the

experimental production

rates in the

energy range 0.5-1.1 MeV. The

quantity

0.6 represents the fraction of the total solid

angle

(4 7r) which is open to atomic

displacements

in the medium energy range ; it corresponds, in the present model, to the total

opening

of thé ( 100 ) and ( lll ) lenses, which

amounts to 0.55 x 4 TE in our model. Thus, this first step of the P(T ) function must include both 100 ) and ( 111 )

displacements,

contrary to the case of Mo [3, 12] for example, for which the two thresholds

Ta loo>

and

Td"’>

stood much more apart.

4. Recovery. - 4. 1 EXPERIMENTAL RESULTS. -

Isochronal anneals (At = 10 min.) were

performed

after

three runs of the first series of irradiations

(7§ -

9 K) at the

energies

0.525 MeV

(Fig.

2),

0.75 MeV

(Fig.

3) and 0.5 MeV

(Fig.

4) and after

one run of the second series of irradiations

(6

K ii

7 K) at 0.5 MeV

(triangles

in

Fig.

4).

Only

the curves

corresponding

to the (100) and (111) samples have been drawn on the

figures,

the curves

Fig. 2. - Isochronal recovery spectra (At = 10 min.) for the two orientations (111) and (100) (0 : sample (100) A, + : sample (100) B) after an irradiation at 0.525 MeV ; the curves have been normalized to the radiation-induced resistivity recovery between 8 and 40 K.

(6)

Fig. 3. - Isochronal recovery spectra (AI = 10 min.) for the two orientations (III) and (100) (0 : sample (100) A, + : sample (100) B) after an irradiation at 0.75 MeV ; the curves have been normalized to the radiation-induced resistivity recovery between 8 and 40 K.

Fig. 4. - Isochronal recovery spectra (At = 10 min.) for the two

orientations (111) and (100) (0 and t::. : sample (100) A, + : sample (100) B) after two different irradiations at 0.5 MeV. The triangles

refer to the second irradiation. The curves have been normalized to the radiation-induced resistivity recovery between 8 and 40 K.

obtained with the (110) samples being intermediate.

The temperature interval was OT = 1.5 K,

allowing

the observation of more details than in the poly- crystalline

experiment.

The same peaks appear at ’" 16

and at 21 K but with an

asymmetric

structure at least for the second one; the existence of at least three

substages has to be assumed in the temperature range 26-35 K if one compares the recovery curves of the different orientations.

The recovery between 40 and 60 K has been studied

only

after the 0.525 MeV run. It is rather constant and small in that range,

exhibiting

no well defined

structure as can be seen on

figure

2, which suggests that it already

belongs

to stage II.

4.2 DISCUSSION. - 4. 2.1 Recovery between 10 and 25 K. - This temperature range contains two main

substages centred at - 16 and 21 K,

although

the

first one has been

partially

suppressed in a number of

cases due to too

high

an irradiation temperature (see

for

example figure

4).

Comparing figures

3 and 4, it

appears clearly that the relative

amplitudes

of both substages increase with the incident electron energy whatever the

sample

orientation may be. This

implies

that the

corresponding

defects are created with a

threshold energy

slightly higher

than the minimum

one. Moreover, the

substage

at 21 K, which is

larger

at low

energies (Fig.

4, A) for the (111)

sample

(in

spite

of a

higher

irradiation temperature) and, at

high energies (Fig.

3), for the (100) sample, can be attributed

to Frenkel

pairs

created via

displacements taking

place near the ( lll ) direction.

Nothing

definite

can be said of the first substage, since its relative

amplitude

is

highly dependent

on the irradiation temperature. At low energy, and for the only irra-

diation

performed

well below 10 K

(Fig.

4, A) it is larger for the (100)

sample

and almost invisible in the

(111)

sample ;

this suggests that it could stem from

pairs produced

in thé ( 100 ) direction.

In many respects

(energy dependence,

orientation

dependence

of the second substage), the recovery between 10 and 25 K in Cr appears similar to that in W, which takes place in

roughly

the same tempera-

ture range (8-20 K) [6]. As in W, the peak correspon-

ding

to the

pairs

created in thé ( l ll ) direction

(substage I2)

has a complex structure

(in

both cases,

W [13] and Cr, a bump is clearly visible on the

high

temperature

side).

Let us note that if the

analogy

stands on real

physical grounds,

an internal friction

relaxation

peak

should be observed in Cr as it has been observed in W [14, 15] and Mo [16], which would anneal

during

substage I2, dislocation

pinning taking place

in the same temperature range.

As concerns the first substage, it seems (see

Fig.

4

and

Fig.

3) to shift towards the

higher

temperatures when

increasing

the energy. Most

likely

this shift is the mere result of the

higher

temperature of the 0.75 MeV irradiation, which suppresses the low temperature part of the peak.

4.2.2 Recovery between 25 and 40 K. - This is the most

important

part of the recovery at low

energies

for all orientations and thus it should correspond to

defects produced with the lowest threshold

energies.

(7)

298

At least four substages must be

distinguished

in that

temperature range, centred at - 28.5 K, 31 K, 33 K and 36 K (the curves of

figures

2, 3 and 4 have been drawn on this

assumption).

An even more

complex

structure is not excluded.

A tentative attribution of these

peaks

is the follo-

wing :

- The 31 K peak whose relative

amplitude

is’

maximum at low

energies

for the (100) orientation and at

high energies

for the (111) orientation would

correspond

to Frenkel

pairs

created in the ( 100 )

direction.

- The 28.5 K and 33 K

peaks

which exhibit the

same orientation

dependence (they

are larger at low

energies

for the (111)

sample

and at

high energies

for

the (100)

samples)

would correspond to Frenkel

pairs

created in the ( 111 ) direction.

- The 36 K peak is a candidate for free interstitial

migration

like the 47 K

peak

of molybdenum [17, 18, 19] or the 115 K

peak

of iron [4]. However, no indi- cation exists at the moment to confirm or to invalidate this.

4.2.3

Comparison

with calculations. - Table II

gives

the calculated percentage of defects created in the

( 100 ) direction as a function of the electron energy and sample orientation. The calculations have been

performed

with the two sets of parameters :

(The

percentage of defects created in thc ( 111 )

direction is the mere complement to 100 % of that

listed).

The

figures

obtained are seen to be rather dependent

on the exact values of the parameters (at least for the low

energies).

In any case, they are consistent with the

.previous

attributions.

Table II. - Calculated percentages of

defects

created

in

the

100 > direction

Sample orientation and mean thickness

5. Conclusion. - A

simple geometrical

model in

which the threshold energy is assumed to be approxi- mately constant around a few directions of low indices

(here

100 ) and (111

))

has been found to

reproduce surprisingly

well the

experimental

results.

The mean threshold

energies

around the ( 100 ) and ( 111 ) directions which are determined in this model are found

practically equal.

In that respect, chromium behaves like tungsten.

An

interpretation

has been

given

of the main

recovery substages below 40 K. Although a confir-

mation is needed as concerns the first recovery

substage centred around 15 K, the low temperature part of the recovery (below 25 K) appears to be very similar to W, i.e. the defects which anneal at the lowest temperature are those which are produced with

a

relatively high

threshold energy. Moreover, as for W, the recovery in the temperature range 25-40 K is due to the simultaneous recombination of

pairs

produced in thé ( 100 ) and ( 111 ) directions (and,

in that respect, can be compared to substage ID of iron). Further

experiments

are

required

to

identify

the long range interstitial

migration.

References [1] BIGET, M., Thesis, Orsay (1978).

[2] BIGET, M., VAJDA, P., LUCASSON, A. and LUCASSON, P., Radiat.

Eff. 21 (1974) 229.

[3] MAURY, F., VAJDA, P., BIGET, M., LUCASSON, A. and LUCAS- SON, P., Radiat. Eff. 25 (1975) 175.

[4] MAURY, F., BIGET, M., VAJDA, P., LUCASSON, A. and LUCAS- SON, P., Phys. Rev. B 14 (1976) 5303.

[5] BIGET, M., MAURY, F., VAJDA, P., LUCASSON, A. and LUCAS- SON, P., Phys. Rev., to be published in 1978.

[6] MAURY, F., BIGET, M., VAJDA, P., LUCASSON, A. and LUCAS- SON, P., Radiat. Eff. 38 (1978) 53.

[7] LOMER, J. N. and PEPPER, M., Philos. Mag. 16 (1967) 1119.

[8] ERGINSOY, C., VINEYARD, G. H. and ENGLERT, A., Phys.

Rev. A 133 (1964) 595.

[9] BIGET, M., VAJDA, P., MAURY, F., LUCASSON, A. and LUCAS- SON, P., Proc. of the Int. Conf. on the Fundamental

Aspects of Radiation Damage in Metals, Gatlinburg,

USERDA Conf.-751006, 66 (1975).

[10] BIGOT, J., Ann. Chim. 5 (1970) 397.

[11] BIGET, M. and VAJDA, P., J. Phys. E. Sci. Instrum. 6 (1973)

968.

[12] RIZK, R., VAJDA, P., LUCASSON, A. and LUCASSON, P., Phys.

Status Solidi (a) 18 (1973) 241.

[13] DAUSINGER, F., Thesis, Stuttgart (1976).

[14] OKUDA, S. and MIZUBAYASHI, H., Phys. Rev. Lett. 34 (1975) 815.

[15] OKUDA, S. and MIZUBAYASHI, H., Phys. Rev. B 13 (1976) 4207.

[16] MIZUBAYASHI, H. and OKUDA, S., Radiat. Eff. 33 (1977) 221.

[17] RIZK, R., VAJDA, P., MAURY, F., LUCASSON, A. and LUCAS- SON, P., Phys. Status Solidi (a) 14 (1972) 135.

[18] COLTMAN, R. R., KLABUNDE, C. E. and REDMAN, J. K., Proc.

of the Int. Conf. on Fundamental Aspects of Radiation

Damage in Metals, Gatlinburg. USERDA Conf.-751006, 445 (1975).

[19] ANTESBERGER, G. and SONNENBERG, K., J. Nucl. Mater. 69 and 70 (1978) 698.

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