Yeuk Ting
Law‡
a,
Spyridon
Zafeiratos
a,
Stylianos G.
Neophytides
b,
Alin
Orfanidi§
b,
Dominique
Costa
c,
Thierry
Dintzer
a,
Rosa
Arrigo
de,
Axel
Knop-Gericke
d,
Robert
Schlögl
de and
Elena R.
Savinova
*a
aInstitut de Chimie et Procédés pour l'Energie, l'Environnement et la Santé, UMR 7515-CNRS-UdS-ECPM, 25 rue Becquerel, 67087 Strasbourg, France. E-mail: elena.savinova@unistra.fr
bInstitute of Chemical Engineering Sciences, Stadiou Str., Platani GR-26504, Rion Achaias, Patras, Greece
cLaboratoire de Physico-Chimie des Surfaces, ENSCP, CHIMIE-PARISTECH, 11, rue Pierre et Marie CURIE, 75005 Paris, France
dFritz-Haber-Institut der MPG, Faradayweg 4-6, Dahlem, D-14195 Berlin, Germany
eMax-Planck-Institut for Chemical Energy Conversion, Stiftstr. 34-36, 45470 Mülheim, Germany
First published on 1st July 2015
The development of efficient energy conversion systems requires precise engineering of electrochemical interfaces and thus asks for in situ techniques to probe the structure and the composition of the dynamic electrode/electrolyte interfacial region. This work demonstrates the potential of the near ambient pressure X-ray photoelectron spectroscopy (NAPXPS) for in situ studies of processes occurring at the interface between a metal electrode and a liquid electrolyte. By using a model membrane-electrode assembly of a high temperature phosphoric acid-imbibed proton exchange membrane fuel cell, and combining NAPXPS measurements with the density functional theory, it was possible to monitor such fundamental processes as dissociation and migration of the phosphoric acid within a nanostructured Pt electrode under polarization.
X-ray Photoelectron spectroscopy (XPS) is one of the most powerful techniques for studies of the chemical composition and the oxidation state of components located within the near-surface region. However, XPS is typically operating under ultra-high vacuum thus severely restricting the range of electrochemical systems which can be investigated. The capability of the XPS for probing the chemical state of surfaces and interfaces has inspired various specialized approaches for studies of electrode/electrolyte interfaces including those involving emersed electrodes,1,2 frozen electrolytes,3 ionic liquids,4etc. Recent advances in vacuum and analyzer technologies have resulted in the development of specialized instruments which allow performing the so-called near ambient pressure photoelectron spectroscopy (NAPXPS) measurements in the pressure range of millibars.5–7 NAPXPS has already proven its extraordinary capabilities to probe in situ reversible and irreversible transformations occurring at interfaces relevant to catalysis8–10 and electrocatalysis.11–15 By applying NAPXPS to a model membrane-electrode assembly (MEA) of a low temperature proton-exchange membrane fuel cell (PEMFC), Casalongue et al.14,16,17 were able to observe chemical changes on the electrode surface and detect reactive intermediates.
This work demonstrates that NAPXPS can also provide an insight into potential-driven processes occurring in a liquid electrolyte at the interface with a polarized metal electrode. By taking advantage of the low vapor pressure of phosphoric acid (PA) we investigate the interface between a nanostructured Pt electrode and a PA-imbibed membrane of the so-called high temperature (HT) PEMFC. HT PEMFC is a subkind of the proton exchange membrane fuel cells that uses PA-imbibed poly-benzimidazole or hydrocarbon-based polymer membranes and operates at temperatures up to 200 °C.18 Due to their high tolerance to carbon monoxide and a simplified water management, HT PEMFCs are highly promising for combined heat and power generation, and can be directly fed with a reformate-based gas, avoiding expensive fuel purification processes. Although currently HT PEMFCs utilize Pt at the anode and at the cathode, non-platinum group catalysts may become a viable alternative, especially considering faster reaction kinetics under the high temperature operation.19 PA being weakly bound to the membrane, its dynamics in the catalytic layer and in the membrane-electrode assembly plays a key role in the operation and the degradation of HT PEMFCs. While conventional diagnostic tools provide valuable information regarding the global performance of a fuel cell (such as current–voltage characteristics, cell resistance, etc.20), they can only deliver indirect information on the PA distribution within a membrane-electrode assembly (MEA) under the operation conditions. Post-mortem analyses (porosimetry, acid-base titrations, gravimetric analyses21) are usually used to analyze the PA distribution in a HT PEMFC. In this work, by using a model MEA of a HT PEMFC and combining NAPXPS with the density functional theory (DFT) calculations, we observe potential-induced dissociation of PA and its redistribution in the catalytic layer in real time.
We now apply voltage between the WE and the counter electrode (CE), in a stepwise manner, and acquire XP spectra of the elements present on the surface of the working electrode. Fig. 2 demonstrates Pt 4f, O 1s, P 2p and C 1s spectra at different cell voltages. Note that in this work we focus on phenomena occurring under positive voltage bias, and thus relevant to the operation conditions of a cathode of a fuel cell or an anode of an electrolyzer. The first important question is whether the interface between Pt particles and the electrolyte is polarized under the conditions of a NAPXPS experiment. Ladas et al.,23 when studying a model solid oxide fuel cell with XPS, at that time under ultra-high vacuum conditions, observed binding energy shifts (ΔBE) following, in a 1:1 correlation, the potential of a WE. Since in electrochemical systems the rates of interfacial processes are related to the exponent of the potential difference between an electronic and an ionic conductor, the in situ information on the interfacial potentials is vital.
The analysis of spectra presented in Fig. 2A reveals that when a positive bias is applied between the WE and the CE, the position of the main Pt 4f peaks (corresponding to metallic Pt) stays constant. This is not surprising, since the WE is grounded to the spectrometer through the Au grid, and thus Fermi level of Pt is pinned to the Fermi level of the spectrometer. This also means that XP spectra of the electrode species do not provide direct information on the electrode polarization.
Meanwhile, the BEs of the elements originating from the electrolyte (O and P) and the HT membrane (C), shift to lower BEs, following polarization of the electrode/electrolyte interface. This shift arises from the fact that the binding energy scale is referenced to the Fermi level of the analyzer, and thus an increase of the potential difference at the electrode/electrolyte interface induces higher photoelectron kinetic energies, which translates into a decrease of the apparent BE of electrolyte species. We further note that the correlation between the cell bias and the BE shifts of the elements originating from the electrolyte is close but not quite equal to the 1:1 correlation observed by Ladas et al.23 This is due to the fact that unlike in ref. 23 no reference electrode (RE) was used in this work. The observed deviation of the BE shifts from the dotted line in Fig. 1D can be explained by the contribution of the ohmic losses in the membrane and overpotential at the counter electrode (see ESI†). Changes in the chemical environment of P and O also contribute to the deviation of their BE shifts from a straight line (vide infra).
Thus, NAPXPS provides a unique tool for probing the interfacial potential difference between an electrode and an electrolyte. Note that if some Pt clusters are eventually disconnected from the current collector, a potential-dependent doublet can be detected in the Pt 4f spectra (see a shoulder at the low BE side of the Pt 4f spectra at high voltage bias). At high positive potentials VWE–CE ≥ 1 V, the surface of Pt is oxidized, as shown by the modification of the peak shape and the appearance of a shoulder at the high BE side of Pt 4f peak in Fig. 2A. Detailed analysis of Pt oxidation, and its dependence on the gas ambience will be subject of a forthcoming publication.
We now turn to the analysis of spectra corresponding to electrolyte components. Quantitative elemental analysis indicates that the O 1s peak intensity is dominated by the PA electrolyte, the contribution of oxygen from either Pt oxides or polymer membrane being negligible (below 6%, see ESI†). At the open circuit voltage (OCV) the O 1s spectrum (Fig. 2B) shows at least two components: a low BE (LBE), and a high BE (HBE). These peaks simultaneously shift to lower BEs as positive voltage is applied to the WE, suggesting that they both belong to the electrolyte species. Also, as the voltage across the MEA exceeds 1.0 V, a tailing at the high BE side becomes clearly visible. This tailing can be fit with a potential independent (PI) peak at 534.1 eV. The independence of this peak of the voltage bias suggests that it originates from species which are electrically equilibrated with the Pt electrode and disconnected from the electrolyte. Likewise, a potential independent (PI) component can be observed in the P 2p spectra (Fig. 2C). Since our experimental set-up has limited spatial resolution, NAPXPS data alone do not allow one to unveil the nature of the PI peaks. The insight comes from our recent scanning photoelectron microscopy study22 which suggests that part of the Pt/PA interface is not polarized. This may be attributed to the presence of PA droplets (or a PA film) on top of the WE, which are disconnected from the bulk of the electrolyte and result in the appearance of potential-independent components in the O 1s and P 2p spectra. Note that this is characteristic of the high temperature dry operation conditions, since at lower operation temperature of 150 °C (not shown) we did not observe the PI component.
Deconvolution of the O 1s spectra into three (LBE, HBE, and PI) components indicates that while the contribution of the PI peak stays fairly constant at ca. 7–9%, the intensity ratio of the LBE and the HBE peaks strongly increases with the positive bias (Fig. 3A) evidencing significant transformations of the PA electrolyte in the interfacial region. Meanwhile, the P:O atomic ratio is potential-independent and amounts to 0.25 ± 0.03 (Fig. S2†). This value is in perfect agreement with the composition of ortho-phosphoric (ortho-PA) H3PO4 (P:O = 0.25), or (pyro-PA) acid H4P2O7 (P:O = 0.29) containing one water per H4P2O7 molecule. In what follows the abbreviation PA will be applied to both ortho- and pyro-phosphoric acid.
Fig. 3 (A) Pt/O and Pt/P atomic ratios normalized to the corresponding values at the OCV (black left-hand-side axis), and LBE (OLBE) to HBE (OHBE) oxygen intensity (red right-hand-side axis) obtained via deconvolution of spectra presented in Fig. 2B as a function of the cell voltage. (B) Apparent thickness of the PA film calculated as a function of the applied cell voltage. |
In order to disentangle the complex O 1s spectra and to unveil their evolution with the voltage bias, O 1s and P 2p core levels were calculated by means of DFT for several model systems. Four types of phenomena were investigated: condensation of H3PO4 (eqn (1)), acid-base dissociation of H3PO4 (eqn (2)) and H4P2O7, hydrogen bonding between PA molecules and/or its anions, and adsorption of PA and its anionic fragments on the Pt surface.
2H3PO4 = H4P2O7 + H2O | (1) |
2H3PO4 = H2PO4− + H4PO4+ | (2) |
Table 1 summarizes BE shifts calculated using DFT for various molecular/ionic configurations, while Fig. 4 shows spectra simulated using the calculated BE shifts (for more details the reader could refer to Table S1 and Fig. S4 in the ESI†).
Molecule/ion | Functional groupa | O 1s BE shiftb, eV |
---|---|---|
a Respective O atom is underlined. b The O 1s BE shifts are referred to PO of a H3PO4 molecule in the gas phase. | ||
H3PO4 | P | 0 |
P––H | 2.0–2.1 | |
H4P2O7 | PO | 0 |
P––P | 2.3 | |
P––H | 2.1 | |
H2O | H2 | 1.2 |
H3O+ | H3+ | 8 |
H2PO4− or H3P2O7− | P–− | −0.2–0 |
P––H | 2.2 | |
H4PO4+ | P––H+ | 8 |
H-bonded H3PO4 and H4P2O7 | P⋯H | 0.5–1.2 |
P––H⋯O | 1.6 | |
H3PO4, H2PO4− or HPO42− chemisorbed on Pt | Pt––P | 1.45 ± 0.15 |
H4P2O7 chemisorbed on Pt | Pt––P | 2.2 |
Fig. 4 Simulated O 1s XP spectra for various molecular/ionic configurations using convolution of Gaussian shape peaks with relative BE shifts calculated by means of the DFT. For more details see the ESI.† |
For a free H3PO4 molecule the O 1s BE shift between P–OH and PO is around 2.0–2.1 eV in agreement with the experimental data.24,25 Thus, for a H3PO4 molecule in the gas phase the DFT predicts an O 1s spectrum consisting of two well defined HBE and LBE peaks with a ratio of 3:1 (Spectrum 1 in Fig. 4). The O 1s shift for P–O–P bond of the gaseous dimer H4P2O7 (pyro-PA) is 2.3 eV, only slightly (0.2 eV) higher than for the P–O–H bond. This calculation is in agreement with experimental measurements of O 1s spectra in ortho- and meta-phosphates, although no precise assignment of the P–O–H and P–O–P bonds was proposed in these studies.26,27 Close O 1s BE values for P–O–H and P–O–P bonds complicate spectroscopic separation of H4P2O7 from H3PO4. In agreement with the literature,28 hydrogen bonding also affects the BE shifts, leading to a decrease of the BE for an H bond donor, and its increase for a H-bond acceptor (see Tables 1 and S1†). H-bonding of H3PO4 and H4P2O7 molecules is expected to result in broadening of the HBE peak (see simulated spectra in Fig. 4 and S4†) due to the appearance of multiple O states with high (P–O–H, P–O–P) and intermediate (PO⋯H, P–O–H⋯O, H2O) values of the BE. Dissociation of the O–H bond in H3PO4 (eqn (2)) or H4P2O7 strongly affects the O 1s BE. For a negatively charged anion, the O 1s BE drops from ca. 2.1 (characteristic of P–O–H) down to ca. 0 eV (for P–O− fragment). Thus, for a H2PO4− anion DFT predicts an O 1s spectrum consisting of two fairly similar peaks separated by 2.2 eV (spectrum 5 in Fig. 4). Meanwhile, for a H4PO4+ cation, DFT predicts an O 1s BE shift to a very high value of ca. 8 eV. Chemisorption of phosphate anions on Pt results in a strong increase of the O 1s BE, the exact value depending on the type of anion, and on the adsorbate geometry. It is worth noting that according to our DFT calculations, the most stable configuration corresponds to HnPO4(3−n)− which maximizes the number of bonds with the Pt surface. The rationale behind the calculated BE shifts is an increase of the BE with the (i) coordination number of oxygen and (ii) covalency of the O–X bond.29
Examination of the calculated P 2p signal with the DFT reveals that it is virtually independent either of the condensation of molecules (pyro- vs. ortho-phosphate), the PA dissociation, or the adsorption of PA or its anions onto the Pt surface. The BE difference between the P2p and the O 1s (gas molecule reference) was equal to 383.5 eV ± 0.2 eV regardless the type of species considered, suggesting that the P 2p peak is rather insensitive to the chemical state of oxygen due to the electron redistribution in the P–O bond.
Armed with the theoretical values of the BE shifts for various states of PA and its anions we analyze the O 1s spectra and their evolution with the applied voltage bias. Even if close values of the BE shifts for certain PA configurations prevent us from an unambiguous assignment of each of the O-containing species, the results of the DFT calculations allow us to explain the potential-induced evolution of the LBE to the HBE O 1s peak ratio. First, we conclude that even if H3PO4 condensation to H4P2O7 leads to a certain increase of the LBE/HBE O 1s peak ratio, the latter is too small to fully account for the observed potential evolution of the shape of the O 1s spectra (cf. spectra 1 and 3 in Fig. 4). This goes in line with the potential independence of the P:O atomic ratio (Fig. S2†).
Second, broader HBE vs. LBE O 1s peak in the experimental spectra (Fig. 2B) is likely to originate from the H-bonding of PA molecules. However, considering the shape of the simulated spectra for H-bonded PA molecules, one can safely conclude that the potential-induced increase in the LBE/HBE ratio cannot be explained by the variation in the extent of H-bonding in the PA electrolyte. Finally, we arrive at the conclusion that significant increase of the LBE to the HBE peak intensity ratio can only be rationalized through dissociation of the O–H bond (eqn (2)) to produce negatively charged phosphate anions (spectrum 5 in Fig. 4). This, of course, does not rule out condensation and/or H-bonding of the PA molecules, but rather means that, contrary to the PA dissociation, these processes are virtually independent of the interfacial polarization. Formation of PA anions can be justified by the electroneutrality considerations. Indeed, under positive applied bias Pt particles are charged positively, and thus negatively charged species are required to compensate the positive electrode charge by forming the so-called electric double layer at the electrode/electrolyte interface. However, if negatively charged phosphate anions were chemisorbed, forming P–O–Pt bonds, the LBE peak would disappear, since bonding of oxygen to Pt results in an increase of the O 1s BE (cf. spectra 5 and 6 in Fig. 4).
Thus, we conclude that an increase of the relative intensity of the LBE O 1s peak at positive working electrode potentials can only be explained by the formation of PA anions which do not form chemical bonds with the Pt surface. This can occur if the anions are screened from the surface by their solvation shells. Electrochemists usually name this type of adsorption (physisorption) as non-specific, contrary to specific adsorption (chemisorption) accompanied by the chemical bond formation.
It is interesting to note that even at the OCV, where Pt surface is metallic (see cyclic voltammogram in Fig. 1C) and where, according to the literature data,30–32 the coverage of chemisorbed phosphate anions is expected to be at its maximum, the shape of the experimental O 1s spectrum does not match the one calculated for H2PO4− anion chemisorbed on Pt (cf. the OCV spectrum in Fig. 2B and spectrum 6 in Fig. 4). Thus, we conclude that even at the OCV the surface coverage of the Pt electrode with chemisorbed PA anions is relatively low. We attribute this to the high operation temperature of 180 °C (the phosphate coverage decreasing strongly with the temperature30), and the small size of Pt particles (3 nm). Indeed, it was found that the adsorption of phosphate anions on metallic Pt is structure-sensitive, for low index planes decreasing in the order of Pt(111) > Pt(100) > Pt(110).33 Hence, chemisorption of phosphate anions on the surface of metallic Pt is expected to decrease with the decrease of the particle size due to the decrease of the size of (111) facets. As the voltage bias is increased above the OCV, Pt surface oxide is formed. Literature data suggest that the coverage of specifically adsorbed (chemisorbed) phosphate anions decreases upon oxidation of the electrode surface.30–32 Meanwhile, the coverage of physisorbed solvated PA anions in the electric double layer will increase to compensate the positive electrode charge. The experimentally measured LBE/HBE O 1s ratio is indicative of a potential-dependent extent of PA dissociation in the electric double layer, roughly estimated as ca. 20% at the applied bias of 1.6 V. Even if, given the complexity of O 1s spectra illustrated by Fig. S4,† this estimation is very rough, and neglects the attenuation of photoelectrons in the electrolyte film, it is clear that this value much exceeds the degree of self-ionization of ortho-PA of ca. 7.4%.34
We note in passing that we observed no experimental trace of H4PO4+ cations at 8 eV vs. the PO reference. At positive electrode bias this may be explained by migration of cations towards the negatively charged counter electrode. Puzzled by the fact that no O 1s peak was found at 8 eV even at negative electrode bias (not shown), we used DFT to estimate the BE of H4PO4+ chemisorbed on Pt. It appeared that P–O–Pt bond formation results in the charge re-distribution and in the concomitant BE shift from 8 eV for a free H4PO4+ down to 3 or even 2 eV for a chemisorbed cation (depending on its orientation relative to the Pt surface). The latter value is close to that characteristic of either P–O–H or P–O–P fragment. It is thus likely that at negative electrode bias H4PO4+ cations, which compensate the negative charge of Pt, are chemisorbed on the electrode surface, which hinders their detection.
The voltage bias not only affects the ratio between the LBE and the HBE O 1s peaks, but also the Pt/P and Pt/O atomic ratios. Fig. 3A shows that Pt/P and Pt/O ratios strongly decrease with the positive polarization suggesting that Pt is covered by electrolyte species comprising PA and its anions. Reversal of the cell voltage induces an increase of the Pt/P atomic ratio, even though the reverse scan usually shows a hysteresis suggesting slow kinetics of the underlying processes (Fig. S5†). Tuning the photon energy allows one to vary the electron penetration depth and thus to estimate the apparent thickness of the PA/phosphate overlayer covering Pt nanoparticles. This strongly depends on the applied cell voltage increasing from ca. 0.8 nm at the OCV to ca. 2.2 nm at VWE–CE = 1.6 V (Fig. 3B). An effective monolayer thickness being estimated as 0.44 nm, the thickness of the PA overlayer at VWE–CE = 1.6 V corresponds to ca. 5 monolayers.
Thus, we infer that application of the positive bias to the Pt working electrode not only leads to the migration of phosphate anions to the surface of Pt particles, to form an electric double layer, but, since they move together with their solvation shells, also to the transport of PA molecules towards the working electrode. Note that the Pt/P(O) atomic ratio is also influenced by the potential-dependent surface tension changes.22
The experimental data supported with the DFT calculations allow us to propose the following model summarized in Fig. 5. As the voltage across the MEA is increased above the OCV, the positive charge density on Pt nanoparticles increases. Since the degree of self-ionization of ortho-PA is small (7.4%),34 the applied voltage induces dissociation of PA (eqn (2)) to provide negatively charged ions (H2PO4− and possibly H3P2O7−) required for the compensation of the positive charge of the WE. Negatively charged phosphate anions migrate to the working electrode, while positively charged species (H4PO4+) migrate to the counter electrode. Since phosphate anions are solvated by PA molecules,¶ their migration towards the positively charged Pt electrode leads to the transport of PA to the working electrode via electroosmotic effect and results in the formation of a film composed from PA molecules and its anions.
It is widely accepted that the penetration of PA into the working electrode has major influence on the HT PEMFC performance. Either excessive penetration of the PA into the WE (the so-called “flooding”), or the electrode drying have detrimental effects on the cell performance.20 This work shows that the thickness of the PA layer on the Pt surface strongly depends on the electrode potential. Therefore, controlling the cell voltage (along with the temperature and humidity) in such a way that an optimum film thickness is maintained could be used as a means to increase the HT PEMFC performance.
This work opens up an opportunity to visualize the interface between the catalyst and a liquid or polymer electrolyte under operation conditions and thus to help in better understanding of the chemical state of materials of electrochemical power sources and electrolyzers. Further studies will be performed in the presence of reactive H2, O2, and other gases.
If not otherwise stated, Pt 4f, P 2p, O 1s and C 1s spectra were recorded at selected photon energies, such that the photoelectrons were emitted at kinetic energy of 400 eV. XP spectra were acquired under applied constant voltage between the working and the counter electrode. Before performing potential-dependent measurements, dedicated experiments were made in order to rule out X-ray beam damage and the ensuing artifacts. The photoemission spectra were normalized by the storage ring current and the energy dependent incident photon flux, which was measured prior and after the measurements using a gold foil with known quantum efficiency. The photon flux obtained has been corrected for higher diffraction orders that contribute only to the background but not to the peak intensity in XPS. The BE scale was calibrated with respect to the Fermi level of the electron analyzer. Curve fitting of the O 1s peaks was performed based on a mixed Gaussian/Lorentzian function. Background subtraction was carried out using the Shirley method. Quantitative calculations were performed using normalized Pt 4f, P 2p, O 1s, C 1s intensities, taking into account the photon-energy dependence of the atomic subshell photoionization cross sections.35
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c5sc01421b |
‡ Present Addresses: Yeuk Ting Law, University Ulm, Institute of Surface Chemistry and Catalysis, Albert-Einstein-Allee 47, D-89069 Ulm, Germany, e-mail: E-mail: yeuk-ting.law@uni-ulm.de. |
§ Present Addresses: Alin Orfanidi, Department of Chemistry, Technische Universität München, Lichtenbergstrasse 4, 85 748 Garching, Germany, e-mail: E-mail: alin.orfanidi@tum.de. |
¶ Note that the experimental O 1s and P 2p XP spectra do not allow to unambiguously distinguish H3PO4 from H4P2O7. However, the experimental P/O ratio suggests that if PA in the MEA is present in the form of a dimer (H4P2O7), it should also contain water, roughly in 1 H2O to 1 H4P2O7 ratio. |
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