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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�
Atomic displacements in low temperature irradiated chromium crystals
M.
Biget,
F. Maury, P.Vajda,
A. Lucasson (*) and P. LucassonBât. 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
lesmécanismes 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 bcccrystals,
andcheck whether this surface would
depend
on theparticular
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]
aswell 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 thatpredicted
by the compu- tations on iron[8],
the ratioTd’ 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 whichmight
account, at leastpartly,
for the differences in the stage 1 recovery spectrum, observed in different bcc metals : it may directly influence the relativepopulations
of the various substages. Moreover, itmay be
indirectly
related to the stage 1 recovery spectrum by the fact that, like the interaction between interstitial and vacancyspecific
to each Frenkelpair configuration,
itoriginates
from the interatomicpotential particular
to each metal. Very little isknown about low temperature irradiated chromium.
To our knowledge the only
existing
data have been obtained in our group [9] onpolycrystalline specimens.
A
single-step displacement probability
function P(T)with a
unique
threshold at 28 ± 1 eV could account for the defectproduction
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, forexample),
it was notpossible
to determine exactlythe end of stage 1 since no long range
migration
wasevident below 60 K.
2. Expérimental. - The
specimens
wereprepared
from a zone-refined chromium bar obtained
by
thecourtesy of J.
Bigot (CECM-Vitry,
France)[10].
Several
grains
with their axesparallel
to ( 111 ) and (110) were detected by a systematic X-ray explo-ration of the bar and then cut out of it. The
slicing
wasperformed
with agoniometric
adaptor described in reference [11]. The final thickness was achieved bymechanical
polishing,
followed byelectropolishing
in a mixture of 95 %
CH3COOH
+ 5 % HCI04. NoArticle published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01979004003029300
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
isgiven by
theresistivity
ratio A (see Table I), the main
impurities being
Fe (10
ppm)
and N (10ppm) (cf.
Ref.[10]).
As can be seen, the thickness of the
samples
ishighly
non uniform, thesamples being
thinner at bothends
(xi, x2)
than in their middle(xm).
Since the very ends of thesamples
are not irradiated, this will leadto 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 thesample
holder (a copper foil of 50 gm covered withsuperconducting
soft solder) was irradiated, thus
resulting
in an extraheating
of thesample.
The irradiation temperaturewas controlled in a first series of irradiations by
measuring
the resistance of the irradiated poly-crystalline sample
(its mean temperatureduring
the irradiations,Ti,
waskept
around 9 K) and in asecond series of irradiations
(performed
at a lowertemperature)
bymeasuring
theresistance
of the (111)sample
(its mean temperature T; was kept between 6and 7 K). Note that the weak
points
at the ends of thesamples
may be another cause of extraheating.
Experience proved
(cf. section 4) that,during
thefirst series of irradiations,
samples
(100) B and (110) Awere irradiated at a
higher
temperature thansamples
(100) A and (110 B).The
annealing
studies wereperformed in
situby heating
the entiresample
chamber andmonitoring
the temperature by means of a
platinum
resistor. Allresistivity
measurements were made at 4.2 K with asensitivity
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 ofoverheating).
The firstthing
to note is that the pro- duction rate remained constant (within the measuringsensitivity),
with the incident electron fluence, even atthe lowest electron energies. This means that the sub-
threshold defects play a
negligible
role in the totaldamage
production. Moreover, - 85 % of the defectsrecovered below 40 K after irradiation at 0.5 MeV ; this percentage decreased to - 60 % after
irradiating
at 0.75 MeV : these numbers are
quite
comparableto what is usually obtained in other metals when no
subthreshold damage is observed
(see
e.g. Ref.[2]).
The
experimental production
rates areplotted
infigure
1 for the foursamples
(100) A, (100) B, (110) Band (111), as a function of the electron energy. The
production
curve measured for thepolycrystalline
sample reproduced closely that obtained before [9]and is not
given
here. Theuncertainty
due to theelectrical measurements lies between 1 and 2 %.
Most of the
uncertainty
on theexperimental points
comes from
possible
variations of the electron beamprofile
in conjunction with the thickness inhomo-geneity
of thesamples,
and from uncontrolledoverheating (particularly
for the (111)sample).
3.2 DATA ANALYSIS. - Since the radiation-induced
resistivity
may be underestimated(by
an amountwhich may vary from one sample to the other) due to
a wrong evaluation of the
shape
factor for the irradia- ted part of thesample,
it would bemeaningless
to tryto determine the exact
shape
of the threshold energy surface, and even to try to determine the relâtiveopening
of the lenses(regions
of low threshold ener-gies
around the maincrystallographic
directions) in aclassical
geometrical
model. Therefore, we adopted athreshold 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 squarepotential
wells with radii of 22°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.
296
and 240
respectively.
Outside of these100 )
and ( 111 ) lenses, the threshold energy wasarbitrarily
fixed at 95 eV (which
corresponds
to an incidentelectron 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 notsupposed
to be asvalid 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>
andT¿lll>, plus
a norma-lization factor for each
production
curve which should beequal
to the Frenkelpair resistivity,
pF - if the radiation-inducedresistivity
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 infigure
1 with 3 sets of parameters :The calculated curves have been normalized to the
experimental
ones in the medium energy range where the model issupposed
to be still valid (not too manymultiple displacements)
and the corrections for energy loss and beamstraggling
are not tooimportant.
We can see that
Td"’>
= 29 eV leads toproduction
rates
definitely
smaller than theexperimental
ones atlow
energies
for the (100) samples; in the same wayTd "’ >
= 27 eV leads, for the (111) sample and atlow
energies,
toproduction
ratessystematically larger
than the measured ones.The best fit is obtained with
Td’00> =
27.5 ± 1 eVand
Td"’> =
28.5 ± 1 eV. These two values arenearly
equal,
as in the case of W [6]. This result will not depend much on the assumed threshold energy surface, but thegeneral shape
of the curves willdepend
on it. The agreement between theexperimental
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 sowidely spread
that - in thedirections of easy
displacement
- it covers the wholeof the
corresponding
lens ; thustaking
a mean valueof the threshold energy for the whole lens will be a
good
approximation.
Theapproximation
should notbe
quite
as good for the (110) sample.At high energies the equality of the two thre-
sholds
Td’00>
andT¿lll>
(which means that the crystal is fairlyisotropic)
is a very favourable case,allowing mutual
compensations
whenmultiple displa-
cements take place.
The obtained value for PF lies between 25 and 39 gÇl cm/at
%
F.P., the mostlikely 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 adisplacement probability
functionwith PF = 40 gfl cm/at %,
fitted well the
experimental production
rates in theenergy range 0.5-1.1 MeV. The
quantity
0.6 represents the fraction of the total solidangle
(4 7r) which is open to atomicdisplacements
in the medium energy range ; it corresponds, in the present model, to the totalopening
of thé ( 100 ) and ( lll ) lenses, whichamounts 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 thresholdsTa loo>
andTd"’>
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 theenergies
0.525 MeV(Fig.
2),0.75 MeV
(Fig.
3) and 0.5 MeV(Fig.
4) and afterone run of the second series of irradiations
(6
K ii
7 K) at 0.5 MeV(triangles
inFig.
4).Only
the curvescorresponding
to the (100) and (111) samples have been drawn on thefigures,
the curvesFig. 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.
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 ’" 16and at 21 K but with an
asymmetric
structure at least for the second one; the existence of at least threesubstages 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 definedstructure as can be seen on
figure
2, which suggests that it alreadybelongs
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
thefirst one has been
partially
suppressed in a number ofcases due to too
high
an irradiation temperature (seefor
example figure
4).Comparing figures
3 and 4, itappears clearly that the relative
amplitudes
of both substages increase with the incident electron energy whatever thesample
orientation may be. Thisimplies
that the
corresponding
defects are created with athreshold energy
slightly higher
than the minimumone. Moreover, the
substage
at 21 K, which islarger
at low
energies (Fig.
4, A) for the (111)sample
(inspite
of ahigher
irradiation temperature) and, athigh energies (Fig.
3), for the (100) sample, can be attributedto Frenkel
pairs
created viadisplacements taking
place near the ( lll ) direction.Nothing
definitecan be said of the first substage, since its relative
amplitude
ishighly 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 frompairs produced
in thé ( 100 ) direction.In many respects
(energy dependence,
orientationdependence
of the second substage), the recovery between 10 and 25 K in Cr appears similar to that in W, which takes place inroughly
the same tempera-ture range (8-20 K) [6]. As in W, the peak correspon-
ding
to thepairs
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
temperatureside).
Let us note that if theanalogy
stands on real
physical grounds,
an internal frictionrelaxation
peak
should be observed in Cr as it has been observed in W [14, 15] and Mo [16], which would annealduring
substage I2, dislocationpinning taking place
in the same temperature range.As concerns the first substage, it seems (see
Fig.
4and
Fig.
3) to shift towards thehigher
temperatures whenincreasing
the energy. Mostlikely
this shift is the mere result of thehigher
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 lowenergies
for all orientations and thus it should correspond to
defects produced with the lowest threshold
energies.
298
At least four substages must be
distinguished
in thattemperature 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 thisassumption).
An even morecomplex
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 athigh energies
for the (111) orientation wouldcorrespond
to Frenkelpairs
created in the ( 100 )direction.
- The 28.5 K and 33 K
peaks
which exhibit thesame orientation
dependence (they
are larger at lowenergies
for the (111)sample
and athigh energies
forthe (100)
samples)
would correspond to Frenkelpairs
created in the ( 111 ) direction.
- The 36 K peak is a candidate for free interstitial
migration
like the 47 Kpeak
of molybdenum [17, 18, 19] or the 115 Kpeak
of iron [4]. However, no indi- cation exists at the moment to confirm or to invalidate this.4.2.3
Comparison
with calculations. - Table IIgives
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 dependenton 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
createdin
the
100 > directionSample orientation and mean thickness
5. Conclusion. - A
simple geometrical
model inwhich the threshold energy is assumed to be approxi- mately constant around a few directions of low indices
(here
100 ) and (111))
has been found toreproduce surprisingly
well theexperimental
results.The mean threshold
energies
around the ( 100 ) and ( 111 ) directions which are determined in this model are foundpractically equal.
In that respect, chromium behaves like tungsten.An
interpretation
has beengiven
of the mainrecovery 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 ofpairs
produced in thé ( 100 ) and ( 111 ) directions (and,in that respect, can be compared to substage ID of iron). Further
experiments
arerequired
toidentify
the long range interstitialmigration.
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.
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Aspects of Radiation Damage in Metals, Gatlinburg,
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[13] DAUSINGER, F., Thesis, Stuttgart (1976).
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[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.
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