Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys , Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys , Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys , Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys , Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys , Comprehensive nuclear materials 4 04 radiation effects in nickel based alloys ,
Trang 1R M Boothby
National Nuclear Laboratory, Harwell, Oxfordshire, UK
ß 2012 Elsevier Ltd All rights reserved.
Abbreviations
AGR Advanced gas-cooled reactor
DFR Dounreay Fast Reactor
EBR-II Experimental Breeder Reactor-II
EDX Energy dispersive X-ray
HVEM High-voltage electron microscope
N/2 dpa calculated according to half-Nelson
model
NRT dpa calculated according to Norget,
Robinson, and Torrens model
STA Solution treated and aged
TEM Transmission electron microscope
UTS Ultimate tensile strength
VEC Variable energy cyclotron
4.04.1 Introduction
Research into the effects of irradiation on
nickel-based alloys peaked during the fast reactor
develop-ment programs carried out in the 1970s and 1980s
Interest in these materials focused on their high
resis-tance to radiation-induced void swelling compared to
austenitic steels, though a perceived susceptibility to
irradiation embrittlement limited their application tosome extent Nevertheless, the Nimonic alloy PE16was successfully used for fuel element cladding andsubassembly wrappers in the United Kingdom, andInconel 706 was utilized for cladding in France Both
of these materials are precipitation hardened andconsequently have high creep strength, and muchresearch and development of alternative alloys wasdirected toward maintaining swelling resistance andcreep strength while aiming to alleviate, or at leastunderstand, irradiation embrittlement effects Therehas been some revival of interest in nickel-basedalloys for nuclear applications, and various aspects ofradiation damage in such materials have recently beenreviewed by Rowcliffe et al.1in the context of Gener-ation IV reactors, and by Angeliu et al.2in consider-ation of their use for the pressure vessel of thePrometheus space reactor Nickel-based alloys arealso candidate structural materials for molten saltreactors, for which resistance to corrosion by moltenfluoride salts and high-temperature creep strengthare prime requirements, though intergranular attack
by the fission product tellurium and irradiationembrittlement due to helium production are poten-tially limiting factors for this application.3
This chapter focuses on the void swelling ior, irradiation creep, microstructural stability, andirradiation embrittlement of precipitation-hardenednickel-based alloys Fundamental to all of theseeffects are the basic processes of damage production
behav-123
Trang 2by the creation of vacancies and interstitial atoms
in displacement cascades, and the ways in which
these point defects migrate and interact with, causing
the redistribution of, solute atoms Detailed
discus-sions of damage processes and radiation-induced
segregation are beyond the scope of this chapter
but these topics will be introduced where necessary,
particularly in relation to void swelling models
More detailed reviews are given in Chapter 1.01,
Fundamental Properties of Defects in Metals;
Chapter 1.03, Radiation-Induced Effects on
Microstructure;Chapter1.11, Primary Radiation
Damage Formation; Chapter 1.12, Atomic-Level
Level Dislocation Dynamics in Irradiated Metals
andChapter1.18, Radiation-Induced Segregation
Typical compositions of nickel-based alloys and
some precipitation-hardened steels, which are
con-sidered in this chapter, are shown inTable 1 Alloy
compositions are generally given in weight percent
throughout this chapter unless stated otherwise
Precipitation-hardened alloys may be utilized in a
number of different heat-treated conditions, which
are generally abbreviated here as ST (solution
trea-ted), STA (solution treated and aged), and OA
(over-aged) Further information on the material properties
of nickel alloys is given in Chapter 2.08, Nickel
Alloys: Properties and Characteristics
Neutron fluences are generally given for
E > 0.1 MeV unless indicated otherwise Atomic
dis-placement doses (dpa) are generally given in NRT
(Fe) units, although the half-Nelson (N/2) model was
widely used particularly in the United Kingdom inthe 1970s6 The exact relationship between theseunits will vary depending on the neutron spectrum(which may differ, not only from one reactor toanother, but also depending on location within areactor), but approximate conversion factors for fastreactor core irradiations are
1026n m2ðE > 0:1MeVÞ
¼ 5dpa NRT Feð Þ ¼ 6:25dpa N=2ð Þ
4.04.2 Void Swelling
4.04.2.1 Compositional Dependence ofVoid Swelling
Nimonic PE16 was first identified as a low-swellingalloy in the early 1970s Void swelling data derivedfrom density measurements on fuel pin cladding mate-rials from the Dounreay Fast Reactor (DFR) werereported by Bramman et al.7and were complemented
by electron microscope examinations described byCawthorne et al.8Swelling in STA PE16 was found to
be lower than in heat-treated austenitic steels andcomparable to cold-worked steels Comparison ofdata for PE16 and FV548 (a Nb-stabilized austeniticsteel) irradiated under identical conditions in DFR to
a peak neutron fluence of6 1026
n m2indicatedthat the lower swelling of PE16 was due to smallervoid concentrations at irradiation temperatures up
to 550C and reduced void sizes at higherTable 1 Nominal compositions (wt%) of commercial and developmental nickel-based alloys
aComposition indicated by Yanget al 4
bComposition indicated by Toloczkoet al 5
Trang 3temperatures At around the same time, Hudson et al.9
compared the swelling behavior of PE16, type 316
steel, and pure nickel, using 20 MeV C2+ion
irradia-tions in the Harwell VEC (variable energy cyclotron)
The materials were implanted with 10 appm (atomic
parts per million) of helium prior to ion bombardment
to peak displacement doses>200 dpa (N/2) at 525C.
Void swelling in 316 steel and nickel exceeded 10% at
the highest doses examined, compared to0.5% in
PE16 Void nucleation appeared to occur earlier
in nickel (at 0.1 dpa) than in PE16 or type 316
(2 dpa), but the peak void concentration was higher
by a factor of about 10 in the austenitic steel than in
nickel or PE16
Hudson et al.9 originally attributed the swelling
resistance of PE16 to the presence of the coherent,
ordered face-centered cubic, Ni3(Al,Ti) g0
precipi-tates, which were thought either to trap vacancies and
interstitials at their surface, thereby enhancing
point-defect recombination, or to inhibit the climb of
dis-locations, thereby preventing them from acting as
preferential sinks for interstitial atoms In support of
the first of these two suggested mechanisms, Bullough
and Perrin10 argued that the surface of a coherent
precipitate would be a more effective trapping site
than an incoherent one where the identity of the point
defects would immediately be lost (and where, as a
consequence, void nucleation was likely to occur) The
efficiency of point defect trapping would be expected
to be greater the higher the total surface area of the g0
precipitates, that is, to be inversely proportional to
the precipitate size at constant volume fraction On
the other hand, the second mechanism proposed by
Hudson et al should be most effective at an
intermedi-ate particle size where dislocation pinning is strongest
Support for the latter process was provided by Williams
and Fisher11 from HVEM (high-voltage electron
microscope) irradiations of PE16 at a damage rate of
about 102dpa s1at 600C, where the swelling rate
was higher at small (3 nm) and large (70 nm) g0particle
diameters than at intermediate sizes of about 20 nm
However, it is now considered that any effect
that the g0 precipitates may have on the swelling
resistance of Nimonic PE16 is secondary to that of
the matrix composition The generally low-swelling
behavior of Ni-based alloys compared to austenitic
steels was shown by Johnston et al.12following
bom-bardment with 5 MeV Ni2+ions at 625C The
dam-age rate in these experiments was 102dpa s1and
the displacement dose was originally estimated as
140 dpa but this was subsequently revised by Bates
and Johnston13 to 116 dpa (based on displacement
energy Ed¼ 40 eV) In addition to hardened alloys, including PE16 and Inconel 706,this experiment included nonhardenable high-Nialloys, such as Inconel 600 and Hastelloy X, a range
precipitation-of commercial steels, and Fe–Cr–Ni ternary alloyscontaining 15% Cr and 15–35% Ni The alloys werepreimplanted with 15 appm helium prior to ion bom-bardment, and the irradiation temperature was chosen
as being close to the peak swelling temperature for irradiated austenitic steels The extent of void swellingwas determined by electron microscope examinations
ion-in low-swellion-ing alloys, but was estimated from height measurements (comparing the surfaces of irra-diated and nonirradiated regions) in high-swellingmaterials As illustrated inFigure 1, the results showednegligible swelling (<0.1%) in PE16, Inconel 706,Hastelloy X, and the Fe–15Cr–35Ni ternary alloy,low swelling (<1%) in other high-Ni alloys, but highswelling (generally>20%) in austenitic steels In com-mercial alloys containing 18% Cr, minimumswelling occurred at Ni contents of about 40–45%.Although void diameters generally appeared to besmaller in the Ni-based alloys than in austenitic steels,the main factor accounting for reduced swelling was amuch lower void concentration In the ternary alloys,reducing the Ni content from 35% to 30% resulted in
step-8 9
7 6
3
2 1
13 12 11 10 0
10
20 30 40 50 60
Nickel (wt%)
Commercial alloys Fe–15Cr–Ni alloys Commercial alloys:
Trang 4an increase in overall swelling from<0.1% to 12%,
although it was noted that the 35% Ni alloy showed
a localized swelling of 5% in a region close to a
grain boundary Additional experiments reported by
Johnston et al.12indicated that the peak swelling
tem-perature for PE16 irradiated with 5 MeV Ni2+ions was
675C, but even then, swelling at 116 dpa remained
below 0.2%
Swelling data for a wider range of pure Fe–Cr–Ni
austenitic alloys, with Cr contents up to 30% and
Ni up to 100%, following Ni ion bombardment to
116 dpa at 675C, were reported by Bates and
Johnston.13 These results showed a strong
depen-dence on both Cr and Ni, with the swelling
increas-ing with increasincreas-ing levels of Cr but beincreas-ing minimized
at Ni contents of about 45–60% Examination of the
dose dependence of swelling in ternary alloys
con-taining 15% Cr and 20–45% Ni showed that the
incubation dose required for the onset of swelling
increased with increasing Ni content Furthermore,
although high-swelling rates of the order of 1% per
dpa were attained in 20–35% Ni alloys, the swelling
rate of the 45% Ni alloy remained low even at doses
above 250 dpa
Following their earlier C2+ion irradiation
experi-ments, Hudson and coworkers moved to the use of
46.5 MeV Ni6+ ions to investigate void swelling
behavior This was considered preferable because
the recoil spectra of high-energy Ni ions provided
a better simulation of fast neutron damage, and
because carbon implantation encouraged the
forma-tion of carbides which acted as void nucleaforma-tion sites
A summary of some of the Ni ion irradiation work
carried out by the Harwell group was given by Makin
et al.14 No significant differences in the swelling
behavior of Nimonic PE16 were evident between
ST or aged conditions Peak swelling in Ni6+
ion-irradiated PE16 (preimplanted with 10 appm He)
occurred at 625C, where a swelling of1.5% was
recorded at 120 dpa (N/2) Void concentrations in
PE16 were reported to be lower by a factor of about
5 than in similarly irradiated type 316 and 321
aus-tenitic steels
A drawback of charged particle irradiation
experi-ments for evaluating void swelling is that the
evolu-tion of other microstructural features may differ
significantly from that during neutron irradiation
(see also Chapter 1.07, Radiation Damage Using
Ion Beams) In the case of Nimonic PE16, for
exam-ple, the precipitation and/or redistribution of the
g0 phase during long-term neutron exposure might
be expected to influence swelling behavior In order
to simulate swelling in a more appropriate structure, Bajaj et al.15examined the effect of 4 MeV
micro-Ni2+ion irradiation on PE16, which had been conditioned by exposure to neutrons in ExperimentalBreeder Reactor-II (EBR-II) Reactor-conditionedsamples had been exposed to neutron fluences inthe range of 3–6 1026
pre-n m2(E > 0.1 MeV) at peratures from 454 to 593C Swelling rates during
tem-Ni ion irradiations at 675C were higher by a factor
of about five in reactor-conditioned material than in anonconditioned sample The increased swelling ratewas attributed to changes in the matrix compositionresulting from an increased volume fraction of g0 inthe reactor-conditioned material
Early attempts to account for the effects of matrixcomposition on void swelling focused on the stability
of the austenite phase Harries16 suggested that theswelling behavior of austenitic steels and nickel-based alloys could be rationalized in terms of their
Ni and Cr equivalent contents (i.e., the relativeaustenite and ferrite stabilizing effects of their con-stituent elements), with the composition of high-swelling alloys then falling into the (gþ s) phasefield in the Fe–Cr–Ni ternary phase diagram Harriespostulated that the partitioning of solute elementsinto the sigma phase would have a detrimental effect
on the swelling resistance of austenite Watkin17took
a similar approach, but found that an improvedcorrelation could be obtained using the concept ofelectron vacancy numbers rather than Ni and Crequivalents The average electron vacancy number,
Nv, of the matrix is calculated from the atomic tions of its constituents, with allowance being madefor the precipitation of carbides and g0 (or g00, etc.),and has been widely used to predict the susceptibility
frac-of nickel-based alloys to the formation frac-of lic phases.18Nvwas calculated from:
intermetal-Nv¼ 0:66Ni þ 1:70Co þ 2:66Fe þ 3:66Mn
þ 4:66 Cr þ Moð ÞWatkin found that void swelling in a range of alloyswith Ni contents up to43%, which were irradiated
in DFR to a peak dose of 30 dpa at 600C, remainedlow for Nv below about 2.5 (corresponding to lowsusceptibility to s phase formation), but increasedapproximately linearly at higher Nv However, as wasclearly argued by Bates and Johnston,13correlationsbased on sigma-forming tendency could not accountfor the minimum in swelling observed at about 45%
Ni, since higher Ni contents should continue to bebeneficial
Trang 5A better understanding of the swelling behavior of
Fe- and Ni-based alloys resulted from a series of fast
neutron irradiation experiments which were carried
out in EBR-II in the early 1980s Irradiation
tem-peratures in these experiments ranged from about
400 to 650C Initial data for a range of commercial
alloys, including ferritic and austenitic steels, as well
as nickel-based alloys, were reported by Bates and
Powell19and Powell et al.,20with higher dose data (up
to a peak fluence (E > 0.1 MeV) of 25 1026n m2,
corresponding to 125 dpa) being reported by
Gelles21 and Garner and Gelles.22Swelling data for
Fe–Cr–Ni ternary alloys, irradiated in EBR-II to a
peak fluence of 22 1026
n m2 (110 dpa), werepresented by Garner and Brager.23 The extent of
void swelling in these experiments was determined
by density change measurements In general, alloys
with nickel contents in the range of 40–50%
exhib-ited the lowest swelling Swelling in commercial
nickel-based alloys was generally lower in ST than
in aged conditions, this being attributed to the
bene-ficial (though temporary) effect of minor elements
remaining in solution and being able to interact with
point defects19; subsequent precipitation during
irra-diation would be expected to reduce this benefit and
the resulting densification, though small, would also
effectively reduce the measured swelling Swelling
data for a number of ST alloys, which were irradiated
in the AA-1 rig in EBR-II, are shown in Figure 2;
data are shown for two withdrawals, at peak fluences
of 14.7 1026
n m2and 25.3 1026
n m2, with surements for Inconel 600 and Inconel 625 reported
mea-at both fluence levels, dmea-ata for Nimonic PE16 and
Inconel 706 at the lower level, and data for Incoloy
800 and Hastelloy X at the higher level The nickel
contents of the alloys range from about 34% in
Inco-loy 800 to 75% in Inconel 600 Swelling remained
relatively low in the three Inconel alloys and in PE16
However, both Incoloy 800 and Hastelloy X exhibited
high swelling at some temperatures, with swelling in
the latter reaching80% at 593C The reason for
such high swelling in neutron-irradiated Hastelloy
X (nickel content48%) is unclear, but it was noted
that densification up to 3% occurred at the lower
irradiation temperatures – indicating microstructural
instability and possibly signaling changes in the
com-position of the matrix which may have affected the
swelling behavior (Note that Hastelloy X was
identi-fied as a low-swelling alloy in the Ni2+ion irradiation
experiments described by Johnston et al.12)
Some data for different heat-treated conditions of
PE16 at the higher fluence level were reported by
Garner and Gelles,22and are compared for tions at 538C (more or less corresponding to thepeak swelling temperature for PE16 in the AA-1experiment) with lower fluence data from Batesand Powell19 in Figure 3 The heat-treated condi-tions indicated in Figure 3 are ST (ST 4 h at
irradia-1080C), A1 (ST and aged 16 h at 705C), A2 (STand aged 1 h at 890C plus 8 h at 750C), and OA(ST and aged 24 h at 840C) Note that the siliconcontent of the PE16 used in these experiments wasmuch lower at 0.01% than the level of0.2% typi-cally found in UK heats of the alloy Overall, the dataappear to show little effect of initial heat treatment
on the swelling of PE16, except that the OA tion exhibited the most swelling (5.2%) at the higherfluence
condi-Although it is clear that the swelling behavior ofaustenitic alloys is largely dependent on nickel con-tent, there is ample evidence to show that minor soluteadditions can have significant effects Much of thework on minor solutes has focused on steels similar
to type 316, but some data are available for highernickel alloys For example, Mazey and Hanks24 used46.5 MeV Ni6+ion irradiations to examine the effects
of Si, Ti, and Al additions on the swelling response ofmodel alloys with base compositions approximatingthat of the matrix phase in PE16 Solute additions
of 0.25% Si or 1.2% Ti reduced swelling, but theaddition of 1.2% Al (in the absence of Si or Ti)markedly increased it The beneficial effect of Si wasbelieved to arise from its high diffusivity in solution(this is discussed further inSection 4.04.2.2), whereasthat of Ti appeared to be related to the formation of Zphase (hexagonal-structured Ni3Ti) The addition of
Al resulted in an increase in the concentration ofvoids, the surfaces of which were coated in a thinlayer of the g0phase (Ni3Al) A beneficial effect of Si
on the swelling response of modified Incoloy DS alloysunder Ni6+ion irradiation was also reported by Mazey
et al.25However, it should be noted that high Si tents can give rise to the formation of radiation-induced phases which are enriched with Ni and Si,such as the Ni3Si form of g0and the silicide G-phase(M6Ni16Si7, where M is usually Ti, Nb, or Mn).G-phase particles are generally found in associationwith large voids and their formation may thereforegive rise to an increase in the swelling rate.26,27Swelling data derived from density measurementsfor neutron irradiated, modified Incoloy DS alloys,with Si contents ranging from 0.19 to 2.05% (com-pared to a specified level of 1.9–2.6% in the commer-cial alloy), are compared with data for a ‘PE16 matrix
Trang 6con-alloy’ and Nimonic PE16 inFigure 4 The materials
were all in ST condition apart from PE16 which was
in an STA condition (aged 4 h at 750C) The alloys
were irradiated in the UK-1 rig in EBR-II to fluences
in the range of 9–16 1026
n m2 (E > 0.1 MeV) attemperatures of 390–640C These data are pre-
viously unpublished except those for STA PE16
(heat DAA 766) which were reported by Boothby.28
Swelling in the modified Incoloy DS alloys generally
decreased with increasing Si content The 0.19% Si
alloy exhibited high swelling at all temperatures withindications of swelling peaks at about 440 and 640C.Increased Si levels tended to suppress the high tem-perature swelling peak and reduce the magnitude ofswelling at lower temperatures The PE16 matrixalloy containing 0.24% Si exhibited a high tempera-ture swelling peak but moderate swelling below
550C, suggesting a beneficial effect of Mo (thisbeing the main compositional difference between thePE16 matrix alloy and the modified Incoloy DS alloys)
−0.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0
Temperature (°C)
0 5 10 15
Temperature (°C)
0 5 10 15 20
25
In 600
In 625
In 800 Hast X
Trang 7at lower temperatures However, swelling in the PE16matrix alloy remained significantly higher at all tem-peratures than in STA Nimonic PE16 (containing0.15% Si), indicating a significant benefit of the g0forming elements Al and Ti.
4.04.2.2 Void-Swelling ModelsPoint defects created by atomic displacements arelost either through mutual recombination or bymigration to sinks Void swelling requires a mobilepopulation of excess vacancies and can only occurover a limited temperature range, typically 350–
700C in neutron-irradiated steels and nickel-basedalloys Rapid diffusion at higher temperatures reducesthe concentration of radiation-induced vacancies tonear thermal equilibrium levels Recombination dom-inates at lower temperatures, where reduced vacancymobility prevents the formation of voids as the neces-sary counter-migration of matrix atoms cannot occur
In the swelling regime, an increased bias for tials over vacancies at dislocation sinks gives rise to thesurplus vacancies which agglomerate to form voids.The flux of point defects to sinks, including voidsurfaces, dislocations, and grain boundaries, results inthe segregation of particular solute atoms at the sinksand the depletion of others In austenitic steels andnickel-based alloys, it is generally found that nickelsegregates at the point defect sinks This is generallyattributed to the inverse Kirkendall effect described
intersti-by Marwick,29 whereby faster diffusing solutes such
as Cr move in the opposite direction to the vacancyflux and are depleted at the sink, and slower diffusingsolutes such as Ni are enriched One of the earliestobservations of nickel segregation at void surfacesdue to the inverse Kirkendall effect was made byMarwick et al.30 in an alloy with a composition cor-responding to that of the matrix phase in NimonicPE16 (For more detailed discussions on radiation-induced segregation effects, see the reviews ofWiedersich and Lam,31and Rehn and Okamoto.32)Venker and Ehrlich33recognized that differences
in the partial diffusion coefficients of alloy ents might account for the effects of composition onswelling Any effect of this kind would generally beexpected to be more significant the larger are thedifferences between the partial diffusion coefficients
constitu-of the alloy components Garner and Wolfer34ined Venker and Ehrlich’s conjecture and concludedthat the addition of even small amounts of a fast-diffusing solute such as silicon to austenitic alloyswould greatly increase the effective vacancy diffusion
Figure 4 Void swelling data derived from density
measurements for Nimonic PE16, a PE16 matrix alloy,
and modified Incoloy DS alloys, irradiated in the UK-1 rig
in Experimental Breeder Reactor-II Unpublished data from
Boothby, R M.; Cattle, G C Void Swelling in EBR-2
Irradiated Nimonic PE16 and Incoloy DS; FPSG/P(90)10,
with permission from AEA Technology Plc.
Figure 3 Effect of heat treatment on void swelling of
Nimonic PE16 irradiated in Experimental Breeder Reactor-II
at 538C Adapted from Bates, J F.; Powell, R W J Nucl.
Mater.1981 , 102, 200–213; Garner, F A.; Gelles, D S.
In Effects of Radiation on Materials: 14th International
Symposium; Packan, N H., Stoller, R E., Kumar, A S.,
Eds.; American Society for Testing and Materials:
Philadelphia, PA, 1990; Vol II, pp 673–683, ASTM
STP 1046.
Trang 8coefficient (i.e., would enhance the diffusion rate for
all matrix elements) The overall effect is analogous to
an increase in temperature – resulting in an effective
decrease in the vacancy supersaturation and hence a
reduction in the void nucleation rate This
mecha-nism is generally accepted as the explanation for the
beneficial effect of silicon in reducing swelling in
austenitic steels and nickel-based alloys Although
this relies on the diffusion of silicon via vacancy
ex-change, silicon is also generally observed to segregate
to point defect sinks and since it is an undersized
solute, this is believed to occur by the migration of
interstitial–solute complexes There is, however, no
reason to suppose that both diffusion mechanisms
cannot operate simultaneously
Garner and Wolfer34 originally considered that
since nickel diffuses relatively slowly in austenitic
alloys, an increase in nickel content would have the
opposite effect to silicon However, a later assessment
made by Esmailzadeh and Kumar,35 based on
diffu-sion data reported by Rothman et al.,36indicated that
the void nucleation rate in Fe–15Cr–Ni alloys would
decrease with an increase in nickel content from 20 to
45% This result is obtained because, although nickel
remains the slowest diffusing species, the effective
vacancy diffusion coefficient of the system is
calcu-lated to increase at the higher nickel content
Esmail-zadeh and Kumar’s calculations also confirmed
the beneficial effect of silicon, with the addition of
1% Si predicted to be as effective in suppressing
void nucleation as increasing the nickel content
from 20 to 45% Effects at nickel contents above
45% could not be examined due to a lack of
appro-priate diffusion data
As well as affecting the nucleation of voids,
differ-ences in the diffusion rates of the various solutes
might also be expected to influence void growth
Simplistically, this can be thought of as being partly
due to the segregation of slower diffusing solutes
reducing the rate of vacancy migration in the vicinity
of the voids However, a further consequence of such
nonequilibrium solute segregation was identified by
Marwick,29 who realized that it would give rise to
an additional vacancy flux which would oppose the
radiation-induced flux to the sink As discussed by
Marwick, this additional flux (the Kirkendall flux)
may itself be an important factor in limiting void
growth, since it will reduce the probability of vacancy
annihilation at sinks and increase the likelihood of
point defect recombination
The effect of nickel content on void swelling was
considered further in a model developed by Wolfer
and coworkers.37,38The model examined the sitional dependence of the void bias and focused onthe effects of nickel segregation at void surfaces.Wolfer’s model indicated that the compositional gra-dients produced by radiation-induced segregationgive rise to additional drift forces which affect thepoint defect fluxes and thereby modify the bias terms.These additional drift forces arise from the effects ofcomposition on point defect formation and migrationenergies, on the lattice parameter and the elastic mod-uli, and from the Kirkendall flux Wolfer’s calculationsfor binary Fe–Ni alloys indicated that the effect of theKirkendall flux is small for interstitials but significantfor vacancies Nevertheless, it was considered that theoverall effect of compositional gradients on the biasterms is likely to be greater for interstitials than forvacancies due to other factors, particularly the effect ofvariations in the elastic moduli As noted by Garnerand Wolfer,39an increase in the shear modulus in thesegregated regions around voids would reduce the biasfor interstitials and therefore help to stabilize voids It
compo-is difficult to predict the significance of thcompo-is effect incomplex alloys, however, since depletion of Cr in thesegregated region will tend to reduce the shear modu-lus, whereas enrichment of Ni in high-Ni alloys willtend to increase it.38 A more significant result of themodel with regard to the effect of nickel on swelling isthat there is a reversal in the sign of the Kirkendallforce for vacancies in Fe–Ni alloys at35% Ni Belowthis level, vacancies are predicted to be attracted intoregions of higher Ni concentration, but above it,the opposite occurs Wolfer et al considered that thiseffect may account for the dependence of swelling on
Ni content in austenitic alloys containing less than35% Ni
A generalized description of the swelling behavior
of austenitic alloys, which was consistent with themodel developed by Wolfer et al., was put forward
by Garner40 (see also Chapter 4.02, RadiationDamage in Austenitic Steels) Garner’s ideas werelargely based on the results of the EBR-II irradiationexperiments and the earlier ion bombardment work
of Johnston et al., both of which showed a strongdependence of swelling on nickel content It wasconsidered that swelling was characterized by a tran-sient period followed by a regime in which theswelling rate became constant In neutron-irradiatedalloys, the swelling rate in the posttransient regimewas generally found to be1% per dpa In swelling-resistant alloys, however, it was argued that such highswelling rates might not be observed owing to ex-tended transient periods The duration of the
Trang 9transient regime was shown to be dependent on alloy
composition and could extend for many tens of dpa in
low-swelling materials The duration of the transient
regime was implicitly linked to the completion of
void nucleation but, at the time these ideas were
put forward, relatively few measurements of void
concentrations were available, as swelling data were
mainly derived from dimensional or density changes
Factors that were proposed to account for the
influence of nickel on the void nucleation rate
in-cluded the effect on vacancy diffusivity described by
Esmailzadeh and Kumar35; a possible correlation with
the development of fine scale compositional
fluctua-tions by a spinodal-like decomposition process
(observed by Dodd et al.41 in ion-irradiated ternary
Fe–Cr–Ni alloys); and an effect of nickel on the
minimum critical radius for the formation of stable
voids.42Voids are unstable below a critical size, and
will generally shrink unless stabilized by gas atoms;
the minimum stable void radius is dependent on a
number of factors, including temperature and defect
bias, and Coghlan and Garner suggested that the
compositional dependence of the vacancy diffusivity
would also affect this critical size In other words, it
was considered that the transition from gas bubble to
void would require a larger bubble size in
high-nickel alloys, particularly at relatively high
tempera-tures in the swelling regime where void nucleation
becomes increasingly difficult Hoyt and Garner43
subsequently argued that the minimum critical void
radius concept might account for the minimum in
swelling found at the intermediate nickel contents,
provided that a compositional-dependent bias factor
for dislocations was also incorporated into the model
The compositional dependence of the bias factor
arises from solute segregation, which reduces the
strain energy of dislocations and decreases the ratio
of the bias for interstitials compared to vacancies
It is of interest that early evidence for the
opera-tion of the bubble to void transiopera-tion was obtained by
Mazey and Nelson,44who implanted Nimonic PE16
(STA condition) and a PE16 matrix alloy (ST
condi-tion) with 1000 appm He to produce a high density
of gas bubbles before subsequent irradiation with
46.5 MeV Ni6+ ions The PE16 matrix alloy used
in this particular experiment was a low Si variant
(<0.02 wt%) which was known to exhibit relatively
high swelling The mean bubble size following
helium implantation at 625C was higher by a factor
of about two in the matrix alloy (11 nm diameter)
than in the commercial PE16 alloy (5 nm diameter)
Examination of the alloys following subsequent
irradiation also at 625C revealed high swelling(12% at 60 dpa) with a uniform distribution of largevoids but no remaining helium bubbles in the matrixalloy, and low swelling (1% at 60 dpa) with abimodal distribution of bubbles plus voids in thestandard PE16 alloy (see Figure 5) These resultswere interpreted as providing evidence for the con-cept of a critical stable void size, with only a smallfraction of bubbles in the commercial PE16 alloy,but all of the bubbles in the matrix alloy, beingsufficiently large to grow as voids Although notspecifically discussed by Mazey and Nelson, thecompositional differences between the two alloyssuggest that the presence of Si and/or the g0formingsolutes Al plus Ti may help to reduce void nucleation
in PE16
The belief advanced by Garner,40that sluggish voidnucleation generally accounted for low swelling innickel-based alloys, persisted for some time However,data reported by Muroga et al.45,46largely overturnedthis view Muroga et al carried out microstructuralexaminations of a series of EBR-II-irradiatedFe–15Cr–Ni ternary alloys with Ni contents rangingfrom 15 to 75 wt%, and of archived samples of similaralloys from the heavy-ion bombardment experiments
of Johnston et al.12Examination of alloys irradiated inEBR-II at 510C showed that the saturation void con-centration was dependent on nickel content and wasminimized at35–45% Ni, but revealed that there was
no increase in void numbers in any of the materialsabove a fluence of 2.6 1026
n m2(E > 0.1 MeV) (seeFigure 6) Alloys containing 19% and 30% Ni exhib-ited high swelling rates at higher fluences, but swellingremained low in higher nickel alloys Similar effectswere found in the ion-bombarded samples, where, forexample, it was shown that there was no significantchange in the void concentration in Fe–15Cr–45Ni
at doses above 50 dpa in irradiations at 675C, yet amarked increase in swelling rate occurred above
120 dpa Thus, contrary to earlier ideas, these gations clearly demonstrated that the onset of a highswelling rate was not related to the cessation of voidnucleation It follows that the transition to a high rate ofswelling must be due to an increase in the growth rate
investi-of existing voids
Muroga et al.45,46observed that the total tion density in the irradiated Fe–15Cr–Ni alloys wasonly weakly dependent on nickel content This sug-gested that at the intermediate nickel levels, wherethe void concentration was low, dislocations wereweak sinks (for both vacancies and interstitials)relative to voids In addition, it was observed that
Trang 10disloca-dislocation loops persisted to higher doses at the
intermediate nickel contents, indicating a lower
growth rate for the loops – again implying an effect
of nickel on dislocation sink strength Based on these
observations, Muroga et al suggested that a reduced
dislocation bias for interstitials at the
intermedi-ate nickel contents might explain the influence of
nickel on the early stages of void development An
additional factor was required to account for the
eventual transition to a high swelling rate
Microche-mical data presented by Muroga et al.46 suggested
that this transition was related to the depletion of
nickel in the matrix owing to its enrichment at void
surfaces
A complete description which incorporates all of
the composition-dependent factors which affect the
nucleation and growth of voids is lacking However,
there is a general consensus that the major influence
of alloy composition arises through its effects on the
effective vacancy diffusivity and on segregation
aris-ing from the inverse Kirkendall effect A correlation
between the magnitude of void swelling and
radia-tion-induced segregation was shown for Fe–Cr–Ni
ternary alloys by Allen et al.48 The compositionaldependence of radiation-induced segregation wasdetermined using a model based on the earlier work
of Marwick,29 which incorporates both the vacancyflux to the voids and the back-diffusion of vacanciesdue to the solute gradients set up by the inverseKirkendall effect Vacancy diffusivities for variousalloy compositions were determined by the measure-ments of grain boundary segregation in proton-irradiated samples Swelling data for ion andneutron-irradiated alloys were then compared withthe expected swelling propensity defined by the ratio
of the forward to back diffusion terms calculated at theappropriate irradiation temperature The materialsfor which vacancy diffusivity data were determinedincluded Fe-based alloys containing 16–24% Cr and9–24% Ni, and Ni-based alloys containing 18% Crand either zero or 9% Fe This work did not specifi-cally examine 40–50% Ni alloys corresponding to thehighest swelling resistance, though the results indi-cated that swelling generally decreased with increas-ing levels of nickel enrichment and chromiumdepletion at void surfaces
20 16 12 8 4 0
0
0 10 20 30 40
Cavity diameter, d (nm)
50 60 70 80 90 100 110 120 130 4
8 12 16 0 4 8 12 16
Figure 5 Histograms showing size distributions of bubbles/voids in (a) solution treated and aged Nimonic PE16 and (b) solution treated PE16 matrix alloy, irradiated with Ni6þions at 625C to damage levels of 30 and 60 dpa following implantation with 1000 appm He (producing 0.2 dpa) at the same temperature Reproduced from Mazey, D J.;
Nelson, R S J Nucl Mater.1979, 85–86, 671–675.
Trang 114.04.2.3 Swelling Behavior of
Neutron-Irradiated Nimonic PE16
Brown et al.49 compared the swelling behavior of
STA Nimonic PE16 and two cold-worked austenitic
steels (M316 and Nb-stabilized FV548) which were
irradiated in DFR as fuel pin cladding Two PE16
clad pins were examined, which were irradiated to
burn-ups of 6.1% and 21.6% of heavy atoms,
corresponding to peak damage levels of about 17
and 80 dpa, respectively Void concentrations and
swelling were lower in PE16 than in the austenitic
steels Swelling data, void concentrations, and void
diameters for the two PE16 pins examined by Brown
et al are shown inFigure 7 Note that Brown et al.49
only showed trend lines for void concentration and
void size in the less highly irradiated pin and
com-pared the swelling tendencies of the two pins; the
individual data points were not plotted and those
shown inFigure 7are previously unpublished data
obtained by Sharpe Brown et al stated that the void
concentration in PE16 decreased with increasing
irradiation temperature but did not alter greatly
with an increasing dose above17 dpa It should be
noted, however, that swelling measurements for the
higher burn-up pin were restricted to temperatures
below 525C, so that a direct comparison of voidconcentrations in the two pins cannot be made athigher temperatures Although there were fewervoids in PE16 than in the two steels, the voids
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0
Temperature (°C)
DFR ~ 17 dpa DFR ~ 80 dpa
DFR ~ 17 dpa DFR ~ 80 dpa
0 10 20 30 40 50 60 70 80 90 100
in Fast Reactor Irradiated Commercial High Nickel Alloy; DFMC/P(82)27, with permission from AEA Technology Plc.
Figure 6 Fluence dependence of swelling and void
density of Fe–15Cr–Ni alloys irradiated in Experimental
Breeder Reactor-II at 510C Swelling data obtained by
immersion density measurements by Garner and Kumar47
are also shown Reproduced from Muroga, T.; Garner, F A.;
Ohnuki, S J Nucl Mater.1991, 179–181, 546–549.
Trang 12appeared to be homogeneously distributed and to have
developed during the early stages of irradiation; once
nucleated, the growth rate of voids in PE16 remained
low These observations are clearly contrary to early
models which suggested that low swelling rates result
from incomplete void nucleation and extended
tran-sient regimes Rather, in agreement with the more
recent observations of Muroga et al.,45,46 it appears
that the swelling resistance of PE16 is due to a
combi-nation of a comparatively low saturation void
concen-tration, which is reached at a relatively low
displacement dose, and a low void growth rate There
does not appear to be any evidence of an accelerated
swelling rate in PE16 once void nucleation is complete
Additional data on void concentrations in
neutron-irradiated PE16 are available from Cawthorne et al.,8
Sklad et al.,50 and Boothby.28 The results presented
by Cawthorne et al for PE16 fuel pin cladding
irra-diated in DFR to a peak fluence of 5.6 1026
n m2(28 dpa) differ from those shown in Figure 7 in
that, although void number densities are similar for
irradiations at 380–520C, void concentrations are
about an order of magnitude higher at 350C and
600–630C Such discrepancies might arise from
uncertainty and/or variability in irradiation
tempera-tures Another possibility is that void nucleation was
incomplete at the higher irradiation temperatures in
the lower burn-up pin examined by Brown et al Data
from Sklad et al show an increase in void numbers in
unstressed PE16 specimens irradiated in EBR-II at
500C from an average (for two differently heat
trea-ted conditions) of about 4 1019
to 1.2 1020
m3with increasing fluence from 1.2 1026
to4.0 1026
n m2 (E > 0.1 MeV), that is, from 6 to
20 dpa In this case, the void concentration and overall
swelling of0.2% at 20 dpa remain below the levels
shown in Figure 7 for the DFR-irradiated pin
at 17 dpa; this may reflect the effect of stress on
swelling for fuel pin cladding
Void swelling data determined from Transmission
electron microscope (TEM) examinations of three
heats of PE16 which were irradiated in the UK-1
rig in EBR-II are shown inFigure 8, which includes
previously unpublished results for the low boron
(4 ppm) heat Z184 as well as data for heats DAA766
and Z260D (with 18 and 70 ppm boron, respectively)
which were reported by Boothby.28 Data are shown
for all three heats in the STA condition (ST 1020C
and aged 4 h at 750C) and for DAA766 in the OA
condition (a multistage heat treatment that included
aging at 900C, slow cooling to 750C, and then
aging for 16 h at that temperature, resulting in the
precipitation of TiC and an overaged g0 structure).Swelling data derived from the density measure-ments of STA PE16 heat DAA 766 from the sameexperiment are shown inFigure 4 An example of the
0.0 2.0 4.0 6.0 8.0 10.0
Temperature (°C)
0 5 10 15
STA DAA766
OA DAA766 STA Z260D STA Z184
STA DAA766
OA DAA766 STA Z260D STA Z184
in Experimental Breeder Reactor-II Adapted from Boothby,
R M J Nucl Mater.1996, 230, 148–157; Unpublished data for Boothby, R M The Microstructure of EBR-II Irradiated Nimonic PE16; AEA TRS 2002 (FPSG/P(90)23), with permission from AEA Technology Plc.
Trang 13void distribution in the OA condition is shown in
Figure 9 Note that the voids in neutron-irradiated
PE16 tend to be cuboidal and that enhanced growth
of voids attached to TiC precipitates (located at the
site of a prior grain boundary) has occurred
Neutron fluences and irradiation temperatures
in the UK-1 experiment were similar to those for the
first withdrawal of the AA-1 rig for which data is
shown in Figure 2 Void concentrations for heats
DAA766 and Z260D shown inFigure 8appear to be
less temperature-dependent than for the fuel pin
clad-ding data shown inFigure 7 Void numbers are
gener-ally lower than in the cladding at temperatures
up to 550C, but are intermediate between the
results of Brown et al.49and Cawthorne et al.8for
irra-diations at 600C Void concentrations for PE16
irradiated to fast neutron fluences (E > 0.1 MeV) of
9.4–12.3 1026
n m2at 477–513C in the UK-1
ex-periment were very similar to those determined by
Sklad et al.50 for 4.0 1026
n m2at 500C The lowboron heat Z184 showed atypical behavior, with a very
high concentration of small voids and low swelling at
438C, but high swelling owing to increased void sizes
at normal void concentrations at temperatures above
513C It is probable that the effect of boron on swelling
is related to the formation of boron–vacancy complexes,
which can give rise to the nonequilibrium segregation
of boron in the presence of quenched-in thermal
vacan-cies as well as to radiation-induced effects.51
Some variability in the swelling response of
Nimonic PE16 in PFR (Prototype Fast Reactor)
components was reported by Brown and Linekar.52
Increased swelling in PE16 subassembly and guidetube wrappers in PFR compared to expectationsbased on the performance of DFR pin claddingappeared to be related to temperature fluctuations,particularly at temperatures below 400C during theearly operation of PFR Void concentrations werereported to be higher in the PFR components, and
it was suggested (by Cawthorne, unpublished data)that this may have been due to the release of vacan-cies from vacancy loops which had formed duringlower temperature excursions In fact, the void con-centration reported by Cawthorne et al.8for DFR pincladding irradiated at 350C was higher than thehighest value reported for the PFR components by
a factor of about 3, but this comparison was not made
by Brown and Linekar There were also indications ofheat-to-heat variability and effects of the fabricationroute on the swelling of PE16 wrappers in PFR.Nevertheless, swelling of PE16 wrappers, althoughhigher than expected, remained low in absolute termsand did not give rise to any operational problems.Although PE16 was originally selected as the ref-erence wrapper material for PFR and as an alterna-tive to cold-worked M316 steel for fuel pin cladding,PE16 was favored as a cladding material with 12%Crferritic–martensitic steel wrappers in subsequentsubassembly designs.53The 12%Cr steel was chosen
as a wrapper material because of its superior swellingresistance, but its use was limited to relatively lowtemperatures owing to inadequate strength at thehigher operating temperatures experienced by pincladding Design calculations for PE16 fuel pin clad-ding made by Cole54 indicated that cladding hoopstresses, which arise from the internal pressure fromthe gaseous fission products released from the fuel,were much lower than the yield stress of the materialand were generally expected to remain below about
70 MPa In addition, the void swelling and irradiationcreep behavior of PE16 were considered to be wellmatched to the fuel swelling, so that fuel–clad inter-action stresses also remain low Fuel pins with PE16cladding successfully attained high burn-ups in PFR,with some 3500 pins exceeding dose levels of 100 dpaand 265 pins reaching maximum doses of 155 dpa.55Very few failures of PE16 clad pins were recorded –three failures occurred in pins which had reachedburn-ups over 17 at.%, with one failure at 11.3 at.%burn-up which was believed to have resulted from
a fabrication defect.56 In addition to the four PE16cladding failures in PFR, Plitz et al.57 recorded 14failures in austenitic steel cladding, all at lower burn-ups than in PE16 The failures in PE16 cladding were
200 nm Figure 9 Void structure in PE16 (OA condition)
irradiated in Experimental Breeder Reactor-II to 58 dpa at
513C Reproduced from Boothby, R M J Nucl.
Mater.1996, 230, 148–157.
Trang 14regarded as benign and permitted continued
opera-tion, with no significant loss of fuel into the primary
circuit coolant A peak burn-up of 23.2 at.%,
corresponding to a peak dose in the PE16 cladding
of 144 dpa, was achieved in PFR in an experimental
fuel cluster Postirradiation examinations of pins
from this cluster and a high burn-up subassembly
(18.9 at.%, with a peak cladding dose of 148 dpa)
were carried out by Naganuma et al.58 Maximum
diametral strains of less than 1% were measured,
attributable to the combined effects of void swelling,
creep deformation arising from internal gas pressure
in the pins, and small contributions from mechanical
interactions between the fuel and cladding in the
lower part of the pins
4.04.3 Irradiation Creep
A detailed discussion of irradiation creep
mechan-isms is beyond the scope of this chapter, which will
instead concentrate on experimental data which
enable comparisons to be made between
nickel-based alloys and austenitic steels However, some
insight into irradiation creep mechanisms is given
inSection 4.04.4.1, where the effect of stress on the
evolution of dislocation structures is described
Irra-diation creep mechanisms are discussed more fully
inChapter 1.04, Effect of Radiation on Strength
and Ductility of Metals and Alloys Several reviews
of irradiation creep data are available in the literature,
for example, by Harries,59 Ehrlich,60 and Garner,61
and although these have tended to focus on austenitic
steels, the behavior of nickel-based alloys generally
appears to be similar
Different types of test specimen, including
pres-surized tubes and helical springs, have been used to
measure irradiation creep strains The data are
therefore generally converted to effective straine
and effective stress s values, using the Soderberg
formalism60:
e=s ¼ e=s ¼ g=3t ¼ 4eH=3sH
where e, g, and eH are tensile, surface shear and
hoop strains; and s, t, and sH are tensile, surface
shear and hoop stresses, respectively
Irradiation creep experiments carried out in DFR
used helical spring specimens, which were loaded in
tension and periodically removed for measurements
DFR data for austenitic steels and Nimonic PE16
were reviewed by Mosedale et al.62 and Harries,59
and results for PE16 were reported in full by
Lewthwaite and Mosedale.63 Average irradiationtemperatures for PE16 specimens ranged fromabout 280 to 340C, with displacement doses up to
a maximum of 13 dpa (N/2) For austenitic steels,the irradiation creep strain was found to be linearlydependent on the applied stress and the displacementdose, comprising transient and steady-state compo-nents as follows:
g ¼ At þ Bdtwhere d is the displacement dose and A and B arematerial-dependent creep coefficients For PE16 in
a STA condition (1 h at 1080C plus 16 h at 700C),creep at dose rates of 5 107dpa (N/2) s1wascharacterized by an initial period of low strain and anincreased creep rate at higher displacement doses.Mosedale et al.62described the g=t versus dpa creepcurve for STA PE16 as parabolic, though the maxi-mum observed creep rate was similar to that in aus-tenitic steels and Harries59 represented the creepstrain above a threshold dose of 8 dpa (N/2) by
g ¼ 4:3 106tðd 8Þwhere t is in MPa; converting to effective strain/stress values and to NRT units of displacement dose(assuming 1 dpa (N/2)¼ 0.8 dpa (NRT-Fe)) wouldreduce the creep coefficient by a factor of 2.4 Datapresented by Lewthwaite and Mosedale63 showedthat ST PE16 behaved similarly to the STA condi-tion, though OA conditions exhibited higher creepstrains due to a combination of increased creep ratesand low threshold doses (around 1 dpa) An apparentdose-rate dependency was observed, with steady-state creep coefficients for STA and OA PE16increased by factors of 2 at lower damage rates of
0.5–1.5 107dpa (N/2) s1 and threshold dosesreduced to 0.5 dpa or less A similar effect ofdose rate on the creep strain per dpa was alsoreported for austenitic steels.64 Steady-state creepcoefficients (MPa1dpa1) and creep strain rates(MPa1s1) for PE16 as a function of dose rate arecompared with data for cold-worked steels M316 andFV548 inFigure 10 The data plotted inFigure 10are derived from the results of Lewthwaite and Mose-dale63,64 but are converted to effective strain/stressvalues and NRT(Fe) dpa units to enable comparisonwith other published data It is evident that the irra-diation creep behavior of STA and OA (24 h at
800C) PE16 is similar to that of the austenitic steels.Creep rates at higher dose rates are generally lowerthan would be indicated from the linear extrapolation
of low dose rate data Lewthwaite and Mosedale63