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Transcript of Observation of Oxygen Vacancy Filling under Water Vapor in Ceramic Proton Conductors in Situ with...
1
Q. Chen, F. El Gabaly, F. Aksoy Akgul, Z. Liu, B.S. Mun, S. Yamaguchi, A. Braun, Observation of oxygen vacancy 1
filling under water vapor in ceramic proton conductors in-situ with ambient pressure XPS; Chem. Mater., 2013, 25 2
(23), pp 4690–4696 http://pubs.acs.org/doi/abs/10.1021/cm401977p 3
in-situ observation of oxygen vacancy filling under water vapor 4
in ceramic proton conductors with resonant 5
ambient pressure XPS and impedance spectroscopy 6
7
Qianli Chen1,2, Farid El Gabaly3, Funda Aksoy Akgul 4,5, Zhi Liu4, 8
Bongjin Simon Mun6, Shu Yamaguchi7, Artur Braun1,* 9
10
1 Laboratory for High Performance Ceramics, Empa. Swiss Federal Laboratories for 11
Materials Science and Technology, CH-8600 Dübendorf, Switzerland 12
13
2 Department of Physics, ETH Zürich, Swiss Federal Institute of Technology 14
CH-8057 Zürich, Switzerland 15
3 Sandia National Laboratories, Livermore, California 94551, USA 16
4 Advanced Light Source, Lawrence Berkeley National Laboratory, 17
Berkeley, CA 94720, USA 18
5 Physics Department, Nigde University, 51240 Nigde, Turkey 19
6 Department of Physics and Photon Science, School of Physics and Chemistry, Ertl Cen-20
ter for Electrochemistry and Catalysis, Gwangju Institute of Science and Technology, 21
Gwangju 500-712, Republic of Korea 22
7 Department of Materials Engineering, University of Tokyo, 113-8656 Tokyo, Japan 23
2
Abstract 24
25
The interaction of metal oxides with their ambient environment at elevated temperatures 26
is of significant relevance for the functionality and operation of ceramic fuel cells, elec-27
trolyzers and gas sensors. Proton conductivity in metal oxides is a subtle transport pro-28
cess which is based on formation of oxygen vacancies by cation doping and substitution, 29
and oxygen vacancy filling upon hydration in water vapor atmosphere. We have investi-30
gated the conductivity and electronic structure of the BaCeY-oxide proton conductor un-31
der realistic operation conditions from 373 K to 593 K and water vapor pressures up to 32
200 mTorr in-situ by combining ambient pressure X-ray photoelectron spectroscopy and 33
electrochemical impedance spectroscopy. We provide element specific spectroscopic evi-34
dence that oxygen vacancies are filled by oxygen upon water exposure and partly oxidize 35
Ce3+ and Y2+ towards Ce4+ and Y3+. Moreover, the resonant valence band spectra of dry 36
and hydrated samples show that oxygen ligand holes in the proximity of the Y dopant are 37
by around 0.5 eV closer to the Fermi level than the corresponding hole states from Ce. 38
Both hole states become substantially depleted upon hydration, while the proton conduc-39
tivity sets on and increases systematically. Charge redistribution between lattice oxygen, 40
Ce, and Y when BCY is exposed to water vapor at ambient and high temperature, give us 41
insight in the complex mechanism for proton incorporation in BCY. 42
43
44
45
3
Introduction 46
47
Protons can be structural elements in molecules and in hydrates, for example, and also 48
ionic and electric charge carriers. In the former case they are localized, in the latter case 49
they are delocalized. The proton is in both cases an elusive element as far as its interac-50
tion with the host lattice or molecular environment is concerned. 51
Ceramic proton conductors are prospective solid electrolytes for intermediate temperature 52
solid oxide fuel cells (IT-SOFC [1-3]). For its functionality as proton conductor, the dy-53
namics is very important with respect to lowering proton transport activation energies. 54
Impedance spectroscopy, inelastic and quasi-elastic neutron scattering and Raman and in-55
frared vibrational spectroscopy are the analytical tools to address the dynamics of the pro-56
ton conductivity. For improving and optimizing proton conducting materials, detailed 57
knowledge on the chemical interaction of the proton with the elements in the host lattice 58
is necessary. For example, exposure of metals to hydrogen atmosphere can cause embrit-59
tlement of the metal, i.e. structural disintegration. In metal oxides, exposure to hydrogen 60
atmosphere can form hydroxyl groups, which constitute a very rigid and polar species 61
that may affect integrity of the oxide and influence on charge transfer. In compounds with 62
oxygen vacancies, the oxygen from ambient water vapor molecules may fill the vacan-63
cies, whereby the protons from the water molecules are incorporated to the host lattice 64
[4]. 65
In the present work we have substituted BaCeO3 to 20% with Y2O3 (BaCe0.8Y0.2O3-δ) in 66
order to form oxygen vacancies to be filled with oxygen from water vapor molecules. The 67
chemical interactions of protons with the host metal oxide are investigated by ambient 68
4
pressure XPS under dry and hydrated conditions, meanwhile the proton conductivity is 69
studied using electrochemical impedance spectroscopy. 70
71
72
73
Experimental 74
BaCe0.8Y0.2O3-δ (BCY20) was prepared by solid state synthesis from precursors mixed in 75
stoichiometric amounts and fired at 1473 K for 12 hours in air, then ground and calcined 76
again at 1473 K for 12 hours. The obtained powder was pressed to pellets of 1 mm thick-77
ness and 18 mm diameter at 10 kbar and sintered for 24 hours at 1673 K in air [5, 6]. 78
Phase purity of the BCY20 was confirmed with powder X-ray diffraction on the finally 79
obtained pellets (Figure S1 in Supporting Information). The sintered pellet was subject to 80
a water vapor saturated N2 flow at 670 K for 16h [5]. Temperature dependent X-ray dif-81
fraction measurements were made on the sintered sample from room temperature up to 82
923 K in steps of 50 K. X-ray diffractograms were measured in a Bragg–Brentano geom-83
etry using a PANalytical X’Pert PRO θ-2θ scan system with the X-ray wavelength of 84
1.5406 Å (Cu-Kα1). 85
Au electrodes were deposited on the proton conducting electrolyte by evaporation in vac-86
uum from crucibles heated by an electron beam, with a mask to control the shape of the 87
electrode [7]. A sample holder with spring-loaded probes (Figure 1), specifically de-88
signed for the combination of XPS and impedance spectroscopy in-situ and operando un-89
der realistic high temperature electrochemical conditions, was used to provide good elec-90
trical contact with the electrodes [8]. The ionic conductivity for BCY20 was measured by 91
5
electrochemical impedance spectroscopy (EIS) using a PCI4/750 Potentiostat (Gamry). 92
The impedance spectra were analyzed with ZView (Scribner Associates). 93
X-ray photoelectron spectra were recorded at the ambient pressure photoemission spec-94
trometer chamber at Beamline 9.3.2 at the Advanced Light Source in Berkeley, California 95
[9, 10]. We exposed the material to water vapor (100 mTorr) at ambient temperature 96
while at the same time recording XPS core level spectra and valence band (VB) spectra 97
in-situ. The temperature was increased step-by-step to 773 K under the water pressure of 98
100mTorr. Again, XPS core level and VB spectra were recorded in-situ with impedance 99
spectra. This approach warrants that we can assess the chemical state of the proton con-100
ductor surface under reaction conditions and also proton conducting operation conditions. 101
Core level spectra for Ba 4d, Y 3d, Ce 4d, and O 1s were recorded for ambient tempera-102
ture, 373 K and 573 K in vacuum, and 573 K with 100 mTorr and 200 mTorr water vapor 103
pressure, respectively. The temperature was measured with a 2-color pyrometer (Mikron 104
M90-H1). Ce 4p1/2 resonant XPS spectra were recorded in vacuum, and with the water 105
vapor pressures mentioned above; Y resonant XPS spectra were recorded with respect to 106
the Y 3p1/2 and 3p3/2 from 299 eV to 310 eV, respectively. 107
6
108
Figure 1: BCY20 pellet with two sputtered Au current collector terminals, clamped in 109
sample holder with 3-electrode configuration for in-situ/operando high-temperature XPS 110
and impedance spectroscopy. 111
112
113
114
115 Results and Discussions 116
Before we turn to the systematic changes in the proton conductor during hydration, we 117
have to investigate the constitution of the proton conductor material (BCY20 pellet) be-118
cause it has been exposed to ambient conditions after synthesis. We have thus subjected 119
the pellet to a controlled drying protocol and monitored this process with thermogravime-120
try and XPS (Supporting Information). After this drying procedure, we exposed the 121
BCY20 pellet to 100 mTorr water vapor at around 573 K, while still recording XPS spec-122
tra. 123
7
124
Proton conducting ceramics develop their ionic conductivity at elevated temperatures T > 125
500 K. A typical variation of the impedance spectra of hydrated BCY20 with temperature 126
ranging from 320 K to 820 K is shown in ref. [Q. Chen, J. Banyte, X. Zhang, J. P. Embs, 127
A. Braun; Proton Diffusivity in Spark Plasma Sintered BaCe0.8Y0.2O3-δ: in-situ combina-128
tion of quasi-elastic neutron scattering and impedance spectroscopy; Solid State Ionics; in 129
press, http://dx.doi.org/10.1016/j.ssi.2013.05.009]. Figure 2-a shows a representative set 130
of impedance spectra of hydrated BCY20, recorded during heating in the UHV chamber 131
while XPS spectra were taken. 132
The impedance spectra in Figure 2-a show the typical semicircles, the radii of which have 133
been determined by deconvolution and least square fitting (ZView, Scribner Associates). 134
The first semicircle at high frequencies originates from the bulk conductivity. Figure 2-b 135
shows hence the bulk conductivity. This conductivity increases with increasing tempera-136
ture homogeneously but not linear over the entire measured temperature range. Rather, 137
conductivity increases linear from 400 K to 450 K, increases then steep from 450 K to 138
550 K, and increases further with the similar slope to the temperatures region of 400 ~ 139
450 K. 140
141
8
142
Figure 2: 2-a: Representative set of impedance spectra of hydrated BCY20 pellet record-143
ed during heating in UHV. The inset shows magnified the high frequency semicircle from 144
the proton bulk conductivity. 2-b: Bulk proton conductivity of hydrated BCY20 as a 145
function of temperature, derived from impedance spectra set mentioned in 2-a. 2-c: Ex-146
cerpt of X-ray diffractograms from hydrated BCY20 recorded from 298 K to 973 K in air. 147
2-d: Variation of unit cell volume of hydrated BCY20 versus temperature, as derived 148
from X-ray diffractograms (2-c). 149
150
151
152
Naturally, the sample undergoes thermal expansion during annealing, which is reflected 153
by the change of the crystallographic unit cell volume (basically the thermal expansion) 154
as determined by high temperature X-ray diffraction in air (Figure 2-c). Note that the 155
9
BCY20 pellet has been saturated with water vapor by the same protocol as published in 156
[5]. The thermal expansion profile in Figure 2-d shows a similar behavior like the con-157
ductivity variation during annealing. We found recently [4] that a decrease of the thermal 158
expansion coefficient of BaZr0.9Y0.1O3-δ (BZY10) occurs at about the same temperature 159
of ~ 650 K where the quasi elastic neutron scattering shows an onset of lateral proton 160
mobility, revealing a correlation of proton conductivity and lattice spacing dynamics. 161
162
We begin with the systematic XPS study by heating the sample under exposure to water 163
vapor. Figure 3 shows three oxygen core level XPS spectra recorded when the sample 164
was dried in UHV, and then exposed to 100 mTorr and 200 mTorr water vapor pressure 165
at 592 K – 532 K. The spectrum recorded in dry condition in UHV (Figure 3-a) shows the 166
O-H peak at around 533 eV and the peak from structural oxygen near 529.5 eV. The two 167
peaks at 529 eV and 532.5 eV originate from structural oxygen Ox in the BCY20 perov-168
skite lattice and from hydroxyl groups (O-H) [12-15]. During exposure to 100 mTorr wa-169
ter vapor, the spectrum is shifted towards lower binding energy by about 0.3 eV, which 170
we have corrected for in Figure 3-b. This shift is likely due to increased electronic con-171
ductivity originating from the development of the space charge region through the grain 172
that influences strongly the inter-grain band-bending [8]. Concomitantly the O-H peak 173
height is increasing whereas the Ox peak intensity is decreasing. This observation sup-174
ports the suggestion that oxygen vacancies are filled and the concentration of protons in-175
creases and enhances the conductivity. During the injection of the water vapor into the 176
UHV chamber, the sample temperature decreased from 592 K to 545 K, an as of yet una-177
voidable technical side effect due to the heat capacity of water vapor. 178
10
179
In a further step, we increased the water pressure to 200 mTorr. The signature of water in 180
the gas phase comes up at around at 535.7 eV The spectrum shows two prominent and 181
well separated transitions at 528.5 eV and 532.5 eV, indicative to hydroxyl O-H and two 182
noticeably different structural oxygen ions. We believe these different oxygen ions could 183
be in proximity to Ce and to Y, respectively. An alternative interpretation could be that 184
these different structural oxygens are the well-known O1 and O2 oxygen ions in ortho-185
rhombic BCY [K.S. Knight, Solid State Ionics 2001, 145, 275–294.]. The exposure to 186
water vapor at this high temperature increases the electric conductivity of the BCY20 187
(Figure 2-b), which manifests in an additional shift of 0.4 eV to an overall shift of the 188
spectrum of 0.7 eV towards lower binding energies (Figure 3 shows the spectra (a) and (b) 189
after alignment on the energy axis). More noticeable is the redistribution of spectral 190
weight from the transition at 528.5 eV, originating from oxygen bound to Ce, toward the 191
corresponding transition originating from oxygen bound to Y, at 532.5 eV. This reveals 192
that the oxygen vacancies in BCY20 formed by substitution with Y are becoming filled, 193
and the corresponding states becoming more populated. 194
11
538 536 534 532 530 528 526 524
Ox (near Ce4+)OH(a) 592 K
UHV
O 1s
XPS
Inten
sity (b) 545 K
p(H2O)=100 mTorr
Ox (near Y3+ and Ce3+)
Ox (near Ce4+)
Binding Energy [eV]
H2O (gas)
(c) 532 K
p(H2O)=200 mTorr
0.4 eV
195
Figure 3: O 1s core level XPS for BCY20 at (592 K to 532 K, temperature changes due 196
to heat capacity of injected water vapor), in (a) UHV, and in water vapor with (b) p(H2O) 197
= 100 mTorr and (c) p(H2O) = 200 mTorr. Photon energy = 700 eV. The spectra are nor-198
malized and aligned by the structural Ox oxygen peak (near Ce4+). 199
200
A shift of 0.4 eV has been observed by Higuchi et al. [19] on 10% Y-substituted barium 201
cerate depending on whether the sample was heated in air or in hydrogen. This is consid-202
ered a sign of the thermal activation of protons, preceding the onset of lateral proton dif-203
fusivity which constitutes the proton conductivity. Since the protons draw electrons away 204
from oxygen, when one proton is shared by two oxygen ions, each oxygen ion should be 205
more negatively charged, and thus the O 1s core level is chemically shifted to lower bind-206
ing energy. To maintain charge balance, we expect that the yttrium delivers electrons 207
when it is getting oxidized. As we will see later, this is indeed observed. 208
12
209
The temperature ranges that we are considering here with XPS show also characteristic 210
changes in the thermogravimetry analyses. The mass of BCY20, as shown in Figure 4-b 211
is noticeably increasing in an air filled TGA chamber at around 300 K. Comparison with 212
literature [11] (Figure 4-a) shows that at such temperature surface water is being released, 213
as shown by mass spectrometry, notwithstanding that the actual weight of the sample is 214
increasing, possibly by hydroxylation. For BCY20, the slope of the derivative of the ob-215
served mass change (lower curve in Figure 4-b) is positive between 300 K and 400 K, 216
virtually zero from 450 K to 650 K, and negative for T > 800 K. 217
218
Figure 4: 4-a: TGA and mass spectrometry data of BaCe0.85Yb0.15O3 reproduced from lit-219
erature [11]; 4-b: and TGA mass change and derivative from hydrated BCY20 in synthet-220
ic air. 221
222
13
It is expected that exposure to water fills oxygen vacancies and thus oxidizes the BCY20. 223
One interesting question is: which vacancies are filled first, i.e. which vacancies are filled 224
more easily. In the course of this in-situ XPS experiment, the BCY20 always showed Ce 225
in a mixed state of Ce3+ and Ce4+. A change in the relative spectral weight is found in the 226
peak ratio at higher binding energies (labeled W‴ and X‴ in Figure 5a, following the no-227
tation in [16]) and lower binding energies (labeled A-C). W‴ and X‴ are signature peaks 228
for Ce4+; these are absent in Ce3+ [15]. This change of ratio in the spectra reveals that 229
Ce3+ is partially oxidized to Ce4+ upon adding water vapor. This picture is paralleled by 230
the evolution of Y3d core level spectra (Figure 5-b) under the same conditions. The in-231
tensities of the structures at 157.5 eV and 159.5 eV are increasing during supply of the 232
water vapor, whereas the structures at 156.5 eV and 158.5 eV are decreasing. 233
130 125 120 115 110 105 100 95 164 162 160 158 156 154
ABCX'''
200 mTorr H2O
100mTorr
XPS
Inten
sity
Binding Energy [eV]
UHV
W'''
(a) Ce 4d
UHV
(b) Y 3d 42% Y3+ Y(3-x)+
Y(3-x)+64% Y3+
p(H2O)=100 mTorr
Y(3-x)+107% Y3+
p(H2O)=200 mTorr
Binding Energy [eV] 234 235
Figure 5: Ce 4d (a) and Y 3d (b) core level XPS for BCY20 at ~530 K, dry and hydrated 236
condition, Ce and Y become oxidized upon addition of water. hν = 700 eV. 237
238
14
As stated in the Introduction, proton conductivity is a subtle process. Weak spectral sig-239
natures are a manifestation of that. High resolution soft X-rayX-ray absorption and emis-240
sion spectra [18] show three O 2p states which have been termed hydrogen structures and 241
considered direct evidence of O-H bonds in the bulk of Y-substituted SrCeO3. These so-242
called hydrogen structures have very small intensity [18]. 243
In order to enhance a potential spectroscopic contrast between Ce and Y, we have applied 244
the valence band XPS experiment in the resonant mode with varied photon energy. Fig-245
ure 6 shows the resonant XPS spectra in the Ce 4p→4d energy region. The valence band 246
consists of a mixed state between 4d1L (A) and 4d0 (B) configurations, in analogy to [17]. 247
L denotes the hole in the valence band, which is mainly composed of the O 2p state. The 248
valence band spectra show a remarkable difference between dry and hydrated state, 249
whereas at first glance a difference between on-resonance and off-resonance cannot be 250
made out. 251
10 8 6 4 2 0 -2 -4
UHV p(H2O)=100 mTorr
off-resonancehn = 223 eV
Inten
sity
Binding Energy [eV]
on-resonance (Ce 4p)hn = 232 eV
O 2p AB
252
Figure 6: On- and off-resonance XPS spectra for dry and hydrated BaCe0.8Y0.2O3-δ 253
measured at ~537 K with hν = 232 eV (Ce 4p 1/2) and 223 eV, respectively. The spectra 254
measured in water vapor are aligned to the spectrum obtained under UHV by shifting 0.6 255
15
eV to higher binding energy. The broad bump (blue) at 0 eV when hν = 232 eV is a sec-256
ond harmonic effect. 257
258
The leading peak A at around 5 eV in Figure 5 therefore represents the Ce3+ state and 259
peak B represents the Ce4+ state. The BCY20 dried in UHV shows in the resonant and 260
off-resonant mode two distinct peaks for Ce3+ and Ce4+ of equal heights, revealing that a 261
substantial amount of the Ce is in the Ce3+ valence at the probed region, i.e. the BCY20 262
surface in the dry condition. When water vapor is supplied at around 573 K, the spectral 263
weight of the leading Ce3+ state decreases by 50%. The spectral weight of the Ce4+ state 264
increases accordingly. A remarkable shoulder from Ce3+ spectral weight remains upon 265
hydration at this level, but the spectral differences are striking. The Ce3+ ions are likely 266
located on a sample surface or in an oxygen defect site. Water fills the oxygen defects 267
and consequently the spectral weight of Ce3+ decreases while the spectral weight of Ce4+ 268
increases. Moreover, for the hydrated BaCe0.8Y0.2O3-δ, the valence band shifts by 0.6 eV 269
to lower binding energy, suggesting higher conductivity due to hole doping induced by 270
hydration (Figure 6 shows the spectra after the aligning of the binding energy B.E. with 271
peak A and B). Slight shifts of the spectra on the energy axis have been observed for ex-272
ample in the VB and oxygen core level spectra on BaCe0.9Y0.1O3-δ (0.4 eV) depending on 273
whether the samples had been annealed in air or in hydrogen [19]. 274
A broad, low intensity peak with the FWHM of ~1 eV appears at 0 eV binding energy 275
when using hν = 232 eV (Ce resonant) as excitation energy, as shown in Figure 6. This 276
broad peak is a spectroscopic artifact and originates from the second order effect out of 277
16
the beamline grating, likewise in the Y resonance spectra (Figure 6). At the Ce resonance 278
energy, this second order effect can be significant. 279
The observation that we make on the cerium resonant VB spectra is paralleled by the yt-280
trium resonant VB spectra at 299 eV and 311 eV. Figure S6 shows a survey spectrum 281
from 200 eV to 350 eV, showing where Y and Ce resonance energies are located. 282
Figure 7 shows the Y-resonant VB spectra of the BCY20 recorded at the 3p3/2 and 3p1/2 283
resonant energies under dry and hydrated conditions at 585 K and 548 K, respectively. 284
We recall for the reader that the heat capacity of the water vapor had effect on the tem-285
perature at the sample when the water vapor was injected in the UHV chamber. Here, too, 286
the BCY20 has a double peak in the dry UHV condition. While we could assign the dou-287
ble peak to Ce3+ and Ce4+ in Figure 5, the origin of the double peak for the Y resonant 288
spectra is not immediately clear, because we anticipate no Y4+ state. We recall that the 289
valence band with respect to the Ce consists of a mixed state between 4d1L (A) and 4d0 290
(B) configurations, in analogy to [17]. Therefore, the leading peak in the Y-resonant 291
spectra at around 4.5 eV binding energy in Figure 6, should be assigned to a reduced Y 292
species such as Y(3-x)+, with x<1. Interesting to note is also that this peak has slightly 293
higher spectral weight than the neighboring conjugated Y3+ peak at around 6 eV. Upon 294
supplying water vapor, we again notice the shift of roughly 0.6 eV towards the Fermi en-295
ergy, suggesting hole doping. Hence, Ce and Y show qualitatively the identical electronic 296
response towards hydration, this is, a slight oxidation with hole doping from the O 2p 297
states. Moreover, it appears that we are unable to discriminate between Ce and Y, despite 298
the resonant excitation that we want to take advantage of. 299
17
14 12 10 8 6 4 2 0 14 12 10 8 6 4 2 0p(H2O)=100mTorr
XPS
Inten
sity
Binding Energy [eV]
UHV
(a)
(b)
p(H2O)=100mTorr
UHV
Binding Energy [eV] 300
Figure 7: Y 3p1/2 resonant XPS (photon energy = 311 eV) at 585 K and 548 K(a); and Y 301
3p3/2 resonant XPS (photon energy = 299 eV) at 585 K and at 544 K (b). The spectra 302
measured in water vapor are aligned to the spectrum obtained under UHV by shifting 0.6 303
eV to higher binding energy. 304
305
When we subtract the VB XPS spectra recorded under wet condition from those recorded 306
under dry condition, we obtain a difference spectrum which should contain the spectral 307
signature of the oxygen defects. Figure 8 shows these difference spectra in resonant con-308
dition for Y and Ce. The maxima of the pronounced difference peak at around 5 eV bind-309
ing energy are shifted by about 0.5 eV, revealing that the gap state of oxygen vacancies 310
next to Y is by 0.5 eV closer to the Fermi level than a gap state from an oxygen vacancy 311
next to Ce. 312
18
313
Figure 8: Difference spectra from Y and Ce resonant XPS measurements under dry and 314
wet condition show a chemical shift of 0.5 eV near the Fermi energy. 315
316
The temperature at which we study the BCY20 with VB XPS is the temperature where 317
we expect the water molecules to be split and their oxygen ions to fill oxygen vacancies 318
that were formed by the substitution with yttrium, which we have sketched in Figure 8. 319
This scenario is indeed confirmed by the change of our spectra upon hydration. Ce3+ is on 320
a sample surface or in an oxygen defect site. The oxygen from the water molecules fills 321
the oxygen defects and consequently the spectral weight of Ce3+ decreases while the Ce4+ 322
spectral weight increases. Note while we here discuss the behavior of cerium, the oxygen 323
vacancies should be actually concentrated at around the yttrium ions. Apparently, this 324
makes spectroscopically little difference when water vapor is supplied. This suggestion is 325
19
corroborated by the observation that the Y-resonant and Ce-resonant VB XPS show iden-326
tical behavior. 327
328
Figure 9: Sketch of the BCY20 structure showing Y, Ce, O, and protons from the water 329
or from the hydroxyl groups. 330
331
The oxygen core level spectra in Figure 3 show that the temperature range (600 K to 500 332
K) where the VB XPS spectra are recorded contains still significant spectral weight for 333
the O-H groups (592 K and 545 K), notwithstanding that at 532 K the spectral weight 334
from O-H groups is clearly dominating the spectrum. The hydrogen in the O-H groups 335
are confirmed at say 545 K (Figure 3) in the VB XPS spectra recorded at 537 K (on- and 336
off- Ce resonant), and at 548 K and 544 K (on- and off- Y resonant). It appears therefore 337
that we must include in the interpretation of the VB XPS spectra and in the formulation 338
of the electronic structure not only the B-site metal ions and the structural oxygen, the 339
oxygen vacancies and the oxygen from the water molecules, but also the protons in the 340
20
hydroxyl groups, which may be structural (localized) protons at low temperatures, and 341
“free” or mobile (delocalized) or polaron protons at higher temperatures when the hydro-342
gen bonds with the structural oxygen (including the oxygen ions that have become struc-343
tural by filling the oxygen vacancies) “melt”. Early studies which suggest a critical role 344
of protons on the electronic structure are based on optical spectroscopy. Sata et al. [20] 345
observed that the optical absorption edge shifted and the band gap increased depending 346
on the Yb-doping concentration in SrZrO3, suggesting that holes are formed at the top of 347
the VB due to Yb doping. In analogy to observations made on dry and wet CaZrSc-oxide 348
with optical spectroscopy, doped protons from moist environment will exchange with 349
doped holes and oxygen vacancies that have been formed by B-site cation doping [21]. 350
The absorption in CaZr0.95Sc0.05O3-δ is lower upon annealing in moist atmosphere, indi-351
cating that the doped proton exchanges with a hole or an oxygen vacancy [21]. An X-ray 352
spectroscopy study conducted on In-doped CaZrO3 suggested that proton states exist in 353
the bulk, and maybe also surface states, proton induced level at the top of the VB [22]. 354
We believe that this experimental in-situ study on the chemistry and the changes of the 355
electronic structure of proton conductors during hydration and annealing will be helpful 356
for understanding the conditions when the proton changes from a localized state to a de-357
localized state where proton conductivity actually sets on. 358
359
Conclusion 360
We investigated the chemical interactions of water with the BaCe0.8Y0.2O3-δ proton con-361
ductor under realistic working condition at elevated temperature and high water pressure 362
in-situ combining ambient pressure X-ray photoelectron spectroscopy and electrochemi-363
cal impedance spectroscopy. We observe three different temperature regimes for the pro-364
21
ton transport along with the structural change of BCY. Applying water pressure at inter-365
mediate temperature affects the oxygen core level, Ce and Y core level as well as the va-366
lence band spectra, revealing the filling of oxygen vacancies in BCY. The corresponding 367
increase in electric conductivity is paralleled by chemical shifts in the oxygen core level 368
spectra. Changes in the oxygen core level spectra, particularly emerging new spectral 369
weight, suggests that oxygen ions near Y3+ and Ce3+ can be distinguished from oxygen 370
ions near Ce4+. The filling of oxygen vacancies with oxygen from water vapor is impres-371
sively reflected by the substantial decrease of the leading peak in the valence band spec-372
tra. Difference spectra of Ce4p1/2 and Y3p1/2 resonant VB spectra show a shift of the lead-373
ing peak by 0.5 eV, which we interpret as that gap states of oxygen vacancies next to Y is 374
0.5 eV closer to the Fermi energy than the corresponding gap state of an oxygen vacancy 375
next to Ce. 376
377
22
Acknowledgement 378
The research leading to these results received funding from the European Community's 379
Sixth Framework Marie Curie International Reintegration Programme grant n.° 042095 380
(HiTempEchem - X-ray and Electrochemical Studies on Solid Oxide Fuel Cells and Re-381
lated Materials), Swiss National Science Foundation project # 200021-124812 (Effect of 382
lattice volume and imperfections on the proton-phonon coupling in proton conducting 383
lanthanide transition metal oxides: High pressure and high temperature neutron and im-384
pedance studies) and by the Korean-Swiss Cooperative Program in Science and Technol-385
ogy project “Spectroscopy on Photoelectrochemical Electrode Materials (SOPEM)”(Call 386
2010). We are grateful to Selma Erat (Empa, ETHZ) for assistance at the beamline, and 387
Songhak Yoon (Empa) for the high temperature XRD measurements. This research was 388
supported by the U. S. Department of Energy through the Sandia Laboratory Directed 389
Research and Development program under Contract DE-AC04-94AL85000. The ALS is 390
supported by the Director, Office of Science/BES, of the U.S. DoE, No. DE-AC02-391
05CH11231. 392
393
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References 394 395 [1] Norby, T. Solid State Ionics 1999, 125, 1-11. 396
[2] Kreuer, K. D. Annu. Rev. Mater. Res. 2003, 33, 333-359. 397
[3] Malavasi, L.; Fisher, C. A. J.; Islam, M. S. Chem. Soc. Rev. 2010, 39, 4370-4387. 398
[4] Braun, A.; Ovalle, A.; Pomjakushin, V.; Cervellino, A.; Erat, S.; Stolte, W. C.; 399
Graule, T. Appl. Phys. Lett. 2009, 95, 224103. 400
[5] Chen, Q.; Braun, A.; Yoon, S.; Bagdassarov, N.; Graule, T. J. Eur. Ceram. Soc. 2011, 401
31, 2657-2661. 402
[6] Chen, Q.; Huang, T.-W.; Baldini, M.; Hushur, A.; Pomjakushin, V.; Clark, S.; Mao, 403
W. L.; Manghnani, M. H.; Braun, A.; Graule, T. J. Phys. Chem. C 2011, 115, 24021-404
24027. 405
[7] El Gabaly, F.; Grass, M.; McDaniel, A. H.; Farrow, R. L.; Linne, M. A.; Hussain, Z.; 406
Bluhm, H.; Liu, Z.; McCarty, K. F. Phys. Chem. Chem. Phys. 2010, 12, 12138-12145. 407
[8] Whaley, J. A.; McDaniel, A. H.; El Gabaly, F.; Farrow, R. L.; Grass, M. E.; Hussain, 408
Z.; Liu, Z.; Linne, M. A.; Bluhm, H.; McCarty, K. F. Review of Scientific Instruments 409
2010, 81, 086104. 410
[9] Grass, M. E.; Karlsson, P. G.; Aksoy, F.; Lundqvist, M.; Wannberg, B.; Mun, B. S.; 411
Hussain, Z.; Liu, Z. Rev. Sci. Instr. 2010, 81, 053106-053107. 412
[10] Hussain, Z.; Huff, W. R. A.; Kellar, S. A.; Moler, E. J.; Heimann, P. A.; McKinney, 413
W.; Padmore, H. A.; Fadley, C. S.; Shirley, D. A. J. Electron. Spectrosc. Relat. Phenom. 414
1996, 80, 401-404. 415
[11] Wu, J. Defect chemistry and proton conductivity in Ba-based perovskites. Disserta-416
tion, Caltech, 2004. 417
24
[12] Koel, B. E.; Praline, G.; Lee, H. I.; White, J. M.; Hance, R. L. J. Electron. Spectrosc. 418
Relat. Phenom. 1980, 21, 31-46. 419
[13] Dupin, J.-C.; Gonbeau, D.; Vinatier, P.; Levasseur, A. Phys. Chem. Chem. Phys. 420
2000, 2, 1319-1324. 421
[14] Deng, X.; Lee, J.; Wang, C.; Matranga, C.; Aksoy, F.; Liu, Z. Langmuir 2011, 27, 422
2146-2149. 423
[15] Mullins, D. R.; Overbury, S. H.; Huntley, D. R. Surf. Sci. 1998, 409, 307-319. 424
[16] Burroughs, P.; Hamnett, A.; Orchard, A. F.; Thornton, G. J. Chem. Soc., Dalton 425
Trans. 1976, 1686-1698. 426
[17] Higuchi, T.; Tsukamoto, T.; Matsumoto, H.; Shimura, T.; Yashiro, K.; Kawada, T.; 427
Mizusaki, J.; Shin, S.; Hattori, T. Solid State Ionics 2005, 176, 2967-2970. 428
[18] Higuchi, T.; Yamaguchi, S.; Sata, N.; Shin, S.; Tsukamoto, T. Jpn. J. Appl. Phys. 429
2003, 42, L1265-L1267. 430
[19] Higuchi, T.; Matsumoto, H.; Shimura, T.; Yashiro, K.; Kawada, T.; Mizusaki, J.; 431
Shin, S.; Tsukamoto, T. Jpn. J. Appl. Phys. 2004, 43, L731-L734. 432
[20] N. Sata, M. Ishigame and S. Shin: Solid State Ionics 86–88 (1996) 629. 433
[21] T. Higuchi, T. Tsukamoto, N. Sata, M. Ishigame, S. Yamaguchi, S. Shin, 434
Optical Absorption Spectra of Protonic Conductor CaZr0:95Sc0:05O3, Jpn. J. Appl. 435
Phys. 2003, 42(3), 1331-1332. 436
[22] T. Higuchi, S. Yamaguchi, K. Kobayashi, T. Takeuchi, S. Shin, T. Tsukamoto, Elec-437
tronic Structure in the Bulk State of Protonic Conductor CaZrO3 by Resonant Soft-X-ray 438
Emission Spectroscopy, Jpn. J. Appl. Phys. 2002, 41(2), L938-L940. 439
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441
442
443 Supporting Information 444 445 446
447
448
Figure S1: X-ray diffractogram of powder from the BCY20 pellet recorded with Cu K-a 449
radiation, confirming phase purity (which phase is it?). 450
451
452
453
454 X-ray 455
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456
457
We have monitored the evolution of the spectral weight at 593 K of either peak in UHV 458
condition in excess of 7 hours, collecting a total of 485 spectra. The heating profile is 459
shown in Figure S4 a. The transient of the relative peak heights of Ox and O-H and their 460
ratio O-H/Ox is displayed in Figure S4 b. The spectral weight of the hydroxyl groups is 461
rapidly increasing, and the spectral weight of the structural oxygen is decreasing to the 462
same extent. Overall, the ratio of the spectral weights increases sharply within 1 hour of 463
keeping the temperature around 593 K, and then remains virtually constant for the fol-464
lowing 6 hours. 465
We believe thus that the O-H groups are formed during annealing on the sample surface 466
from residual water from exposure to ambient conditions, thus causing a relative decrease 467
of the spectral weight from Ox. Comparison with thermogravimetry data (Figure S5 a, 468
adopted from BaCe0.85Yb0.15O3 in Ref. [11]) shows that surface water is released at 373 K 469
and structural water at 593 K, suggesting that structural oxygen Ox in BCY20 indeed 470
could be released from the sample at 593 K in UHV. 471
472
27
473
Figure S4: Heating profile (left) and evolution of spectral weight (right) of the O1s core 474
level XPS peaks for O-H, Ox, and their ratio O-H/Ox. 475
476
Figure S5: Ion current from water release (solid line from 350 K to 600 K) and XPS peak 477
height ratio for O-H/Ox. 478
479