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Structure of cation interstitial defects in
nonstoichiometric rutile
L.A. Bursill, M.G. Blanchin
To cite this version:
L.A. Bursill, M.G. Blanchin. Structure of cation interstitial defects in nonstoichiometric rutile. Journal
de Physique Lettres, Edp sciences, 1983, 44 (4), pp.165-170. �10.1051/jphyslet:01983004404016500�.
�jpa-00232175�
Structure of
cation interstitial defects
in
nonstoichiometric
rutile
L. A. Bursill(*)
and M. G. BlanchinDépartement de Physique des Matériaux (**), Université Claude Bernard, Lyon
I, 43, Boulevard
du 11 Novembre 1918, 69622 Villeurbanne Cedex, France(Re~u le 16 aofit 1982, revise le 14 decembre, accepte le 3 janvier 1983)
Résumé. - On
présente
ici de nouveaux modèles de défauts interstitiels pour accommoder la non-stoechiométrie du rutile peu réduitTiO2-x.
Ces défauts consistent en des arrangements linéaires, lelong
de directions [100] ou [010], depaires
de cations trivalents situés au centre d’octaèdresd’oxygène
ayant une face en commun. On décrit ensuite les mécanismes de diffusion permettant
l’aggrégation
de tels défauts pour donner naissance à despaires
de plans de « cisaillementcristallographique
», ainsi que cela a été récemment observé enmicroscopie électronique
à haute résolution dans des cristauxTiO2-x
refroidis relativement lentementdepuis
la température de réduction de 1 050 °C. Des consi-dérations relatives àl’énergie électrostatique expliquent pourquoi
ces défauts ont uneénergie
deformation et de
migration beaucoup plus
basse que les défauts « ponctuels » traditionnels.Abstract. - New cation interstitial defect models are derived for substoichiometric rutile
TiO2-x.
These consist of linear arrangements,
along
[100] or[010], containing
two face-shared octahedralpairs
of trivalent cations. Diffusion mechanisms are describedwhereby
these mayreadily
aggregate to formpairs
ofcrystallographic
shearplanes,
as observed recentlyby high-resolution
electronmicroscopy, when
TiO2-x specimens
are cooledrelatively slowly
from 1 050 °C. Electrostatic argu-mentsexplain why
these defects have very much lower formation andmigration energies
than thetraditional «
point
defect » interstitial model. ClassificationPhysics Abstracts
61. 70B - 61. 70P - 61. 70Y
1. Introduction. - Considerable
uncertainty
remainsconcerning
the nature of the structural defectsresponsible
for thephase
Ti02-x (see
e.g. Akse and Whitehurst[1],
for a recent literaturesurvey).
Mostinterpretations
ofphysical
property
and resonancetechnique
measurements have been based upon models forpoint
defectequilibria
(see
e.g. Kofstad[2]).
Bursill and
Hyde [3] questioned
whether « classical »point
defects occurred in reduced rutilesince
TiO 1. 9 9 8 61
well annealed at 1 000 °C and thenslowly
cooled,
contained lamellaeof
crystal-lographic
shearplanes (CSP) coexisting
with a maze ofintersecting
{132} ~
0 2 2 ~
CSP. Thelatter was identified as the nonstoichiometric
phase TiO~-~.
However,
theinterpretation
of electricalconductivity
measurementsby
Baumard,
Panis andAnthony [4]
and ofquenching
experiments
followedby
electron diffraction contrast studies(Blanchin,
Faisant, Picard,
Ezzo and Fontaine[5])
suggested
that forTi0i 99~0-2.0000
theequilibrium phase existing
at 1 050 °C (*) Permanent Address : School of Physics,University
of Melbourne, Parkville, 3052, Victoria, Australia.(**) Associe au C.N.R.S.
L-166 JOURNAL DE PHYSIQUE - LETTRES
contains no CSP.
High-resolution
electronmicroscope
(HREM)
studies of a numberof Tio2
preparations
(0
x 0.0035),
reduced at 1 323 K andgiven
avariety
of thermomechanicalhistories,
showed newphenomena
(Blanchin,
Bursill,
Hutchison and Gai[6] ;
Bursill,
Blanchinand Smith
[7] ;
Smith,
Blanchin and Bursill[8]).
Thus CSP were notpresent,
even en miniature,in non-deformed
crystals quenched
from 1 323K,
but did appear,frequently
as veryclosely-spaced pairs,
in moreslowly
cooled or reduced and deformedspecimens.
HREM revealed bothlateral and
longitudinal
disorder within the structure of theCSP,
the details of which werestrong-ly dependent
uponcooling
histories.Many
of the HREMimages
showed «spot »
contrastswhich
suggest
the presence of small(
20 A
diameter)
defects. Recent electricalconductivity
studies over a wider range oftemperatures
(T),
and forrelatively high partial
pressures of oxygen(p02)
(Marucco,
Gautron and Lemasson[9],
Gautron,
Marucco and Lemasson[10])
suggest
that there are three domains within theTiO 2 - x phase,
where thepredominant
defects are assumed to be :I interstitial
Tit.,
prevailing
for T > 900 °C and forrelatively
lowpartial
pressures of oxygen; IIdoubly
ionized oxygen vacanciesV,5, prevailing
at lowertemperatures
and forincreasing
p02,
andIII another oxygen vacancy
defect, initially interpreted
as asingle
ionized oxygenV,6
(Marucco
et al.[9])
but later attributed to oxygen vacancies associated withcharge compensation
of alio-valentMe3+
impurities
(Gautron et
al.[10])
prevailing
for x0.000 16,
independent of p02
or T.
In this letter we
present
new models for cation interstitialdefects
which were derived in anattempt
to extend the structuralprinciples
of CS(previously
identified toapply throughout
most of thestoichiometry
rangeTi0l,sooo-Ti02,oo00) to
account for the structure of interstitial defects in non-stoichiometric rutile. New structure models for anion vacancy andimpurity
defects will bepresented
elsewhere(Bursill
andBlanchin,
inpreparation).
2. Derivation of interstitial structure. - 2 .1 TRADITIONAL CATION INTERSTITIAL STRUCTURE.
-Figure
ladepicts’the
[010]
boundedprojection
(2013 ~
yi)
of the rutile structure,using
the familiar octahedralrepresentation.
The 4
y1
boundedprojection
issymmetrically
equivalent.
(In
earlier work it was convenient to take thecorresponding [010]
section,
see BursillFig.
1. - Boundedprojection
(along
[100],
for - 4
xt)
of the structure of rutile,containing :
a)no defect ; b) traditional interstitial defect, i.e. additional Ti 3 + cations ; c) two
pairs
of octahedrally-coor-dinated Ti3 + cationssharing
faces; d), e) and f) show linear extensions of c) toproduce
more widely-separ-ated pairs of face-shared octahedra.and
Hyde
[3],
the use of[010]
in thepresent
workproved surprisingly
instructive.)
Rutile istetra-gonal
with cellparameters
a = 4.593 7A,
space groupP4/mnm
with Ti at000 ;
2 i i
and 0 atuuO;
l~uO; 2
u,2
+U, i 2 and 2
+u, 2 u, 2
with u = 0.305 3.Octahedrally
coordinated interstitialsites may be found at
~00; i02; 0~0; 0~
(see
Hurlen[11]).
Figure
lbdepicts
the classical model for the interstitial inrutile,
whereby
aTi3 +
cation isinserted
at(~00).
Note the formation of astring
of three face-sharedoctahedrally
coordinated cationsites,
separated by
2.3A,
Analysis
of the electrostatic valencies
(esv ;
seeMegaw [12],
for a discussion of thisconcept)
of the oxygenions
(labelled 01
and02
inFig. Ib)
associated with this modelgives -
2.00 for01
and - 2.5 for02.
The latterimplies
alarge
electrostatic energy for such a defect. Bursill andHyde [3]
showed that the CSP observed
by
electronmicroscopy
and diffractiontechniques throughout
most of the
stoichiometry
rangeTiOl,sooo-2.000o
allcontain,
as a common structuralprinciple,
pairs
of face-shared octahedra linkedby edge-
andcomer-sharing
in such a way thatthey
maybe
regarded
as coherentintergrowths
of elements of the corundum-like structure of e.g.Ti203’
with the rutile matrix. Our HREM observation thatpairs
of CSP occurredfrequently
inspecimens
relatively slowly-cooled
across theTi02-x phase boundary
suggest
that the interstitial defects may consist of twopairs
of face-shared octahedra and that these thenaggregate
in order topro-duce CSP. Thus
figure
2a shows the octahedral arrangement in a[010]
boundedprojection through
apair
of(121)
CSP. Note that cations in face-shared octahedral sites must have(formally
atleast) charge
+ 3 if the correctstoichiometry
(Ti2+, Ti~~ 2)
C~,-1
is to be obtained for the CSP. 2.2 ALTERNATIVE CATION INTERSTITIAL DEFECT STRUCTURE.- Figure
Ic shows that twopairs
of face-shared octahedra
may
bereadily
obtained fromfigure 1 b by shifting
one of the cations(arrowed) by
vector[~00].
Such ajump
isformally equivalent
to a cation Frenkel defect.However,
this
geometrical relationship
isonly
superficial.
In order to obtain apair
of CSPby aggregation
of the defects shown in
figure
Ic,
werequire
aTi3 +
cation in each of the face-shared sites. We therefore take as our basic interstitial defectfigure
Ic with fourTi3+
cations. Two of these occupy octahedral interstices and two substitute forTi4+
cations in normal cation sites. In additionFig. 2. - Bounded
projection
(along
[100],for - 4 x 4)
of the rutile structurecontaining :
a) apair
of (121)
crystallographic
shearplanes
(CSP); b) a pairof (253)
CSP; c) apair of (132)
CSP and d) apair
ofL-168 JOURNAL DE PHYSIQUE - LETTRES
one cation
site,
formerly occupied by
Ti4+,
is now empty.Altogether
we havereplaced
three normalTi4+
cationsby
fourTi3+ cations,
giving
no netchange
inpositive change
in thelattice,
compared
to the extra + 3charges
in the classical model. 2.3 ENERGETIC CONSIDERATIONS. - Thisnew defect model must
have,
at least inprinciple,
very much lower electrostaticcontributions,
at both short andlong-range,
to both its formation andmigration energies. Analysis
of the electrostatic valencies of the oxygen sites show twocrystallographically
distinct sites(labelled 0~
and0;
inFig. Ic),
with 120~
having
esv = 2013 1.833 and 6’0~ having
esv = - 2.333. The average esv is thus -2.0,
and weexpect
that ion relaxations and associatedpolarization
of the oxygen ions(rutile
has ahigh
dielectricconstant)
will allow the esv of all of the oxygen ions toapproach
close to - 2.0.Simplistic
electrostatic energycal-culations,
so farneglecting
ion relaxations andpolarization
effects,
using
a difference-sumtech-nique,
showed that the new model is lower in electrostatic energyby -
100eV,
despite
the factthat it contains four
Ti3 +
cationscompared
to one for the classical model(Bursill
andShen,
in
preparation).
More extensive calculations are in progress but it isalready
very clear that the new model is anextremely
efficient way, bothenergetically
andchemically
toincorporate
Ti3 +
cations into rutile.
3. Further consideration and discussion. - 3 .1 MOBILITY
AND AGGREGATION OF INTERSTITIAL DEFECTS. - A
pair
of(121)
CSP may bereadily
formed(Fig.
2a)
by
orderedaggregation
of the defects shown infigure
Ic,
provided
that the defects arereasonably
mobile.Assuming
ahomo-geneous distribution
of
such defects leads to the conclusion that CSP can form in the bulk ofa reduced
crystal
and
thus are not constrained to grow from the surface. Since thedisplacement
vector across a
pair
of CSP is R = 0[Modulo
1]
thismay occur without
necessarily creating
a
partial
dislocationloop (of
course, if dislocationsalready
exist,
as in deformedspecimens,
the defects may accrete to it and
produce
dissociation;
we return to elaborate the variouspossi-bilities in another
paper). Figures
3a,
b,
c indicate sequences ofcooperative
atomic diffusivejumps
required
formobility parallel
to[001], [100]
and[0~]
respectively.
Note that we assumesuch defects are created at the
crystal
surfaces,
following
loss of oxygen to the gasphase
onreduction of rutile. These
jumps
canalways
be carried out in such away
thattriple-face-sharing
of octahedra is avoided. Note that
essentially
Frenkel defects are involved but in addition weassume an
accompanying
electronicconductivity according
toTi 3 + --+> Ti4 +
+ e-. This lastFig. 3. - Arrows indicate
suggested
diffusion mechanisms for movement of Ti3 + interstitial defectsparallel
to a) [001] ; b)[010]
and c)[2 0 2].
Dotted arrows indicate more complex concerted atom movements required for bulk diffusion of M 3 + (e.g. Cr3 + orFe3 + )
interstitial defects.process has a low activation energy
( ~
0.40eV,
see Marucco et al.[9]).
Similar diffusivehops
allow CSP
splitting, subsequent
to theirformation,
toproduce arbitrary separations
(see
Bursillet al.
[13]).
3.2 LINEARLY EXTENDED INTERSTITIAL DEFECTS. - Our HREM
observations showed that the local orientation of the CSP
pairs
observed inrelatively
slowly-cooled
specimens
fall between(121)
and(143)
with mean orientation(132).
Figures
2b-d show thecorresponding
boundedprojections through pairs
of(253), (132)
and(143)
CSPrespectively.
Thisfigure immediately
suggests a furtherdevelopment
of the cation interstitialmodel,
depicted
infigures
Id,
e, f. Here successive[~00]
atomicjumps
lead to furtherseparation
of the face-sharedpairs, producing
linear defects
having
extentstarting
at 9.2A
andincreasing
to 13.8A,18.4
A
or 27.2A
respective-ly.
Orderly aggregation
of such defects leadsnaturally
topairs
ofhigher
index CSP.Further-more,
imperfect ordering
of any one type, or of a mixture of different types leadsnaturally
tolateral and
longitudinal
disorder within the CSP structure, as observedby
HREM. It should be noted that the linearstrings
ofdisplaced
octahedraconnecting
the face-sharedpairs
in these linear defects occur as elements of the(011)
antiphase boundary,
or microtwin lamellar structures,often observed in rutile
(see
Blanchin et al.[6] ;
Bursill andHyde
[3]).
The esv of thecorresponding
oxygens are - 2.0.
3.3 INTERSTITIAL DEFECTS IN DOPED SPECIMENS. - We note that CSP defects also occur in rutiles
doped
withFe3 +
orCr3 +.
The same interstitial defects models couldapply
here,
withTi3 +
substitutedby
Me3 +,
although
asyet
HREM has not been carried out to determine whether the CSPprecipitate
aspairs.
(In
such caseslong-range
diffusion mechanisms(dotted
inFig.
3),
are
required.)
Thus the kinetic behaviour ofdoped specimens
isexpected
to differ from that of the reducedbinary
system
Ti02-x.
3 . 4 LOCALIZATION OF ELECTRONS. - It has been convenient
so far to assume that Ti3 + ions
are
(formally)
attached to the face-shared octahedral sites. In fact electricalconductivity
mea-surementssuggest
(Marucco et
al.[9])
that at T > 800~C,
the effectivecharge
of interstitial cations isTi4 +,
implying complete
ionizationof Ti3 +
ions(Ti3 +
-~Ti4 +
+ e -,13
= 0.40eV)
with consequent delocalization of the electrons. Even at very low
temperatures
it is not certain that theTi3 +
ions will be located in face-shared octahedral sites. This appears to be the case forTi203,
and weregard
the shortest of the above linear defects as an element ofTi203
structure.However
crystallographic
studies of thephase
transitions ofTi407 [14,
15]
show that in thatphase
Ti3+ -Ti3+
pairing
occurs betweenedge-shared
octahedralsites,
withonly
one of eachface-shared octahedra
containing
aTi3 +
ion,
for temperatures below 125 K. At room tempe-rature and above all Ti ions have effectivecharge
3.5,
indicating virtually complete
delocalization of the electrons.Clearly
thespatial
extent of delocalization of electrons associated with small defects inTi02-x (x
0.0035),
and itstemperature
variation,
remains aninteresting problem,
requiring
furtherexperimental
and theoreticalstudy.
4. Conclusion. - It is
now necessary to seek further HREM evidence for the presence and interactions of cation interstitial defects described here.
Computer
simulations of HREMimages
(Bursill
andShen,
inpreparation)
show that it should bepossible
todirectly image,
andpositively
identify,
such smalldefects,
and theiraggregation,
under veryspecific imaging
conditions. In situ studies of theprecipitation
and dissolution ofCSP,
andcomplementary
HREMstudies,
havealready produced positive
results and are in the course ofpublication [13].
In another paper the structure of oxygen vacancy defects in nonstoichiometric rutile is examined
(Bursill
andBlanchin,
inpreparation).
It wasagain
foundpossible
tomodify
the classical model and derive a structure consistent with the common structural theme referred to above.Clearly
L-170 JOURNAL DE PHYSIQUE - LETTRES
the
principles
ofpoint
defectequilibria
used for theanalysis
of a wide range ofphysical
pro-perty
measurements(electrical conductivity,
thermogravimetry,
ionicconductivities,
internalfriction,
electron-spin-resonance,
etc...)
will need to becarefully
reassessed in thelight
of such models.Acknowledgments.
- L. A. Bursill isgrateful
toUniversity
ofLyon
for support of a visit toLyon
in 1982. The work was alsosupported by
theUniversity
of Melbourne.References
[1]
AKSE, J. R. and WHITEHURST, H. B., J.Phys.
Chem. Solids 39 (1978) 451.[2] KOFSTAD, P., Non
stoichiometry, diffusion
and electrical conductivity in binary metal oxides(Wiley-Interscience, New
York)
1972, p. 22 and 137.[3]
BURSILL, L. A. and HYDE, B. G., Prog. Solid State Chem. 7 (1972) 177.[4] BAUMARD, J. F., PANIS, D. and ANTHONY, A. M., J. Solid State Chem. 20 (1977) 43.
[5] BLANCHIN, M. G., FAISANT, P., PICARD, C., EZZO, M. and FONTAINE, G., Phys. Status Solidi (a) 60 (1980) 357.
[6] BLANCHIN, M. G., BURSILL, L. A., HUTCHISON, J. L. and GAI, P. L., J.
Physique Colloq.
42 (1981) C3-95.[7] BURSILL, L. A., BLANCHIN, M. G. and SMITH, D. J., Proc. R. Soc. Lond. A384 (1982) 135. [8] SMITH, D. J., BLANCHIN, M. G. and BURSILL, L. A., Micron 13 (1982) 245.
[9] MARUCCO, J. F., GAUTRON, J. and LEMASSON, P., J. Phys. Chem. Solids 42 (1981) 363.
[10] GAUTRON, J., MARUCCO, J. F. and LEMASSON, P., Mater. Res. Bull. 16 (1981) 515.
[11]
HURLEN, T., Acta Chem. Scand. 13 (1959) 365.[12]
MEGAW, H. D.,Crystal
structures : a workingapproach
(Saunders, New York) 1973, p. 39.[13]
BLANCHIN, M. G., BURSILL, L. A. and SMITH, D. J., Proc. Inter. Conf. defects in ioniccrystals,
Dublin(to be
published
in RadiationEffects),
1982.[14] MAREZIO, M., MCWHAN, D. B., DERNIER, P. D. and REMEIKA, J. P., J. Solid State Chem. 6 (1973)
213.