Startseite Density Functional Theory Calculations of H/D Isotope Effects on Polymer Electrolyte Membrane Fuel Cell Operations
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Density Functional Theory Calculations of H/D Isotope Effects on Polymer Electrolyte Membrane Fuel Cell Operations

  • Satoshi Yanase EMAIL logo und Takao Oi
Veröffentlicht/Copyright: 29. April 2015

Abstract

To elucidate hydrogen isotope effects observed between fuel and exhaust hydrogen gases during polymer electrolyte membrane fuel cell operations, H-to-D reduced partition function ratios (RPFRs) for the hydrogen species in the Pt catalyst phase of the anode and the electrolyte membrane phase of the fuel cell were evaluated by density functional theory calculations on model species of the two phases. The evaluation yielded 3.2365 as the value of the equilibrium constant of the hydrogen isotope exchange reaction between the two phases at 39 °C, which was close to the experimentally estimated value of 3.46–3.99 at the same temperature. It was indicated that H+ ions on the Pt catalyst surface of the anode and H species in the electrolyte membrane phase were isotopically in equilibrium with one another during fuel cell operations.

1 Introduction

Fuel cells (FCs) are an energy device that converts the change in the Gibbs free energy that occurs during the reaction in which water is formed from hydrogen and oxygen to electric energy. During FC operations, hydrogen ions are generated by oxidation of hydrogen atoms on the platinum (Pt) catalyst of the anode of a cell and transferred to the cathode through an electrolyte membrane. They finally combine with electrons from an external circuit and oxygen atoms to form water molecules on the Pt catalyst of the cathode.

Hydrogen gas (hydrogen molecules) as the fuel for FC operations consists of two stable hydrogen isotopes: protium (H) and deuterium (D). H/D isotope effects are expected to be observed during processes of adsorption of hydrogen molecules on surfaces of the Pt catalyst, dissociation of the adsorbed hydrogen molecule into hydrogen atoms, oxidation of the hydrogen atoms to hydrogen ions on the catalyst, and the transfer of the generated hydrogen ions to the electrolyte membrane throughout FC operations.

To investigate and understand the redox mechanism on Pt catalysts of FCs, analysis of H/D isotope effects on FC operations can be a powerful tool. In our previous article [1], we tried to detect the H/D isotope effects upon an FC operation using a polymer electrolyte membrane fuel cell (PEMFC) system operated at 39 °C. As a result, we observed that the lighter isotope of hydrogen, H, was enriched in the unreacted (exhausted) hydrogen gas. In other words, the heavier isotope of hydrogen, D, was preferentially transferred to the electrolyte membrane. The value of the H/D isotope separation factor obtained, S, ranged from 3.46 to 3.99. Here, S is defined as

(1)S=(D/H)p/(D/H)d, (1)

where (D/H)d is the D to H isotopic ratio in the exhaust gas and (D/H)p is that of the hydrogen gas reacted at the anode and transferred to the membrane. These results were in a sense surprising. The theory of kinetic isotope effects tells us that the lighter isotope of a chemical element in general reacts faster than the heavier counterpart. If the isotope effects we observed in our experiment are the kinetic ones, the values of S should be less than unity. The S values larger than unity obtained in our FC experiments suggested that the observed H/D isotope effects should be analyzed and elucidated based on the theory of equilibrium isotope effects.

To elucidate the H/D isotope effects we observed, we calculated equilibrium constants of hydrogen isotope exchange reactions expected to occur during FC operations by the density functional theory (DFT) in the same article [1]. The H/D isotope exchange equilibrium between the electrode catalyst phase and the electrolyte membrane phase is expressed in a general form as

(2)Dcat+HelecHcat+Delec, (2)

where H(D)cat denotes the H(D) atom or ion in the electrode catalyst phase and H(D)elec denotes that in the electrolyte membrane phase. The H(D) atoms in the electrode catalyst phase are reduced to H+(D+) ions on the Pt catalyst. In the electrolyte membrane phase, the H+(D+) ions transferred from the anode are expected to exist as H2O, oxonium ion (H3O+) and/or H+ of the sulfonic groups (−SO3H) of electrolyte membranes. Therefore, the following isotope exchange equilibria can be assumed.

(3)Pt-D++H2OPt-H++HDO, (3)
(4)Pt-D++H3O+Pt-H++H2DO+, (4)

and

(5)Pt-D++R-HPt-H++R-D, (5)

where, “Pt-H+(D+)” denotes the H+(D+) ion bonded to a Pt atom on the catalyst surface and “R−” denotes the sulfonate (−SO3) group forming a covalent bond to the polymer matrix of the electrolyte membrane. Based on the Bigeleisen–Mayer theory on equilibrium isotope effects [2], the isotope exchange equilibrium between two chemical species can be quantitatively analysed using their reduced partition function ratios (RPFRs), (s/s′)f. The general expression for the RPFR is – under the Born-Oppenheimer and harmonic oscillator approximations and the approximation that the rotations are classical (i.e., that the ratio of their partition functions is unity) – given as

(6)(s/s)f=Πi=1puiexp(ui/2)/{1exp(ui)}uiexp(ui/2)/{1exp(ui)}, (6)

where ui= hcωi/(kT) and ui=hcωi/(kT);p=the degree of freedom of molecular vibration; h=Planck’s constant; c=the velocity of light; ωi and ωi=the wave numbers of the ith molecular vibration of the heavier and the lighter isotopic species, respectively; k=the Boltzmann constant; and T=the absolute temperature. Thus, the RPFR for the given species and for the given isotopic pair can be theoretically estimated by knowing all the isotopic vibrational frequencies of the species. The equilibrium constants of Reactions (3) and (4), K3 and K4, can be given as the ratios of the RPFRs of the two H species involved in the individual reactions:

(7)K3=fH2O/fPt-H+ (7)

and

(8)K4=fH3O+/fPt-H+, (8)

where fH2O,fH3O+ and fPtH+ are the H/D RPFRs of H2O, H3O+ and Pt–H+, respectively. We carried out geometry optimisation and normal mode analysis of these chemical species by DFT calculations at the UB3LYP/Lanl2dz level of theory and estimated RPFRs of fH2O,fH3O+ and fPtH+, and K3 and K4 at 25 °C. Calculated values of K3 and K4 were 3.358 and 3.976, respectively. Although temperature was different from the experimental temperature of 39 °C, the computational results agreed well with the experimentally obtained S values, which ranged from 3.46 to 3.99.

In the above mentioned calculations, we approximated surfaces of the Pt catalyst by a single Pt atom, which was certainly an oversimplification. For a more exact comparison between computational and experimental results, a cluster of Pt atoms may be preferable as the model of the Pt catalyst surface. Sebetci [3] reported DFT calculation results of PtnHm (n=1–5, m=0–2) but did not refer to the values of their H/D RPFRs. As the model of H species in the electrolyte membrane phase, we considered an isolated H2O molecule and an isolated H3O+ molecular ion, i.e., H2O and H3O+ in vacuo, which was also an oversimplification. In addition, the theoretical evaluation of the equilibrium constant, K5, of Reaction (5), which was not attempted in the previous article [1], will be needed to better understand the experimentally observed H/D isotope effects.

In the present work, we adopted a Pt10 cluster, the structure of which is depicted in Figure 1, to model the Pt catalyst surface of the anode of the FC used in the previous article [1]. As the model of the electrolyte membrane (Naffion N-212), we considered the −SO3 group interacting with an H3O+ ion and seven H2O molecules. In this article, we discuss the H/D isotope exchange equilibria of (2) based on the computational results on the RPFRs of our present models.

Figure 1: Pt10 Cluster as a model molecule of Pt catalyst. The six coplanar Pt atoms are intended to be the Pt catalyst surface.
Figure 1:

Pt10 Cluster as a model molecule of Pt catalyst. The six coplanar Pt atoms are intended to be the Pt catalyst surface.

2 DFT Calculations

Although H, H+, H2, and H2+ are possible H species on surfaces of the Pt catalyst of a FC, it is hardly thinkable that H2 and H2+ are the H species in equilibrium with H species in the electrolyte membrane phase during actual FC operations. Thus, as the H species adsorbed on surfaces of the Pt catalyst, a H+ ion and a H atom bonded to the surface of the Pt10 cluster, Pt10-H+ and Pt10–H, were considered as model H species in the electrode catalyst phase. The structure of the Pt10 cluster was taken from the crystal structure of Pt [4]; Pt has the face-centered cubic (fcc) structure with the lattice constant a=392.42 pm and the nearest interatomic distance of 277.48 pm. As shown in Figure 1, the surface of metallic Pt is represented by the seven coplanar Pt atoms with the experimentally obtained nearest interatomic distance, forming a regular hexagon. As the adsorption site of H+ and H, we consider the central Pt atom and a peripheral (edge) Pt atom of the hexagon. In the geometry optimisation of Pt10–H+ (and Pt10–H), the structure of Pt10 was kept fixed at the experimentally obtained one, and only H+ (H) was moved to achieve the minimum on the potential energy surface of Pt10-H+ (Pt10–H). In other words, we focused only on the Pt-H+ (Pt-H) bond, because our primary interest was in the interaction between a Pt atom and H+ (H) and not in the structure of the Pt crystal. In the vibrational analysis at the optimised geometry, we set the mass of a Pt atom at 1016, which means that none of the Pt atoms move in any vibrational mode, and consequently only three vibrational modes related to the movement of H+ (H) are given a non-zero wave number. These manipulations are considered effective in the present study as we are only interested in Pt–H+ (Pt-H) bonding on surfaces of the Pt catalyst and not in the whole body of the Pt catalyst, and what we need is the H/D RPFR related to the H+ (H) movement and not the movements of Pt atoms.

As model H species in the electrolyte membrane phase, we considered the H3O+ ion bonded to the −SO3 group of an acid polymer constituting the electrolyte membrane and surrounded by seven H2O molecules. As the model acid polymer, we considered part of the structure of the heptahydrated copolymer of tetrafluoroethylene and perfluoro -[2-(fluorosulfonylethoxy)propylvinyl ether], generally known as Nafion; Nafion is the most popular polymer for electrolyte membranes of FCs and was used as the electrolyte membrane in our previous article [1]. Thus, as the electrolyte membrane phase, we considered C5F11-SO3···(H3O+)(H2O)7 and totally ignored the presence of polymer chains.

All the DFT calculations were made with our unix and personal computers or at the computer facility at Sophia University using Gaussian 09 program package (Gaussian Inc.) [5]. Winmostar (X-Ability Co., Ltd, Tokyo, Japan) [6], Gaussview (Gaussian Inc., CT, USA) and Freewheel (Butch Software Studio, Tokyo, Japan) were used for the graphics. The theoretical level and the basis set chosen was UB3LYP/LanL2dz, so that the present DFT calculations are consistent with our previous ones [1]. The possible spin multiplicities (SMs) were 2 or 4 for Pt10–H and 1 or 3 for Pt10–H+. Calculations were made for all these SMs. All the geometry optimisations were conducted without symmetry constraints under the condition of the fixed coordinates for the 10 Pt atoms. The H-to-D RPFRs (H/D RPFRs) at 25 °C and 39 °C were calculated by using the unscaled frequencies obtained by the normal mode analysis at respective optimised structures.

3 Results and Discussion

3.1 Model Hydrogen Species in the Electrode Catalyst Phase and their RPFRs

The optimised structures of Pt10–H+ and Pt10–H are shown in Figure 2a–d and their computed physical parameters are summarised in Table 1.

Figure 2: Optimised structures of Pt10–H and Pt10–H+. (a) Pt10–H with H absorbed on the central Pt atom, (b) Pt10-H with H absorbed on a peripheral Pt atom, (c) Pt10-H+ with H+ absorbed on a center Pt atom, and (d) Pt10–H+ with H+ absorbed on a peripheral Pt atom. No significance is attached to the relative sizes of the spheres.
Figure 2:

Optimised structures of Pt10–H and Pt10–H+. (a) Pt10–H with H absorbed on the central Pt atom, (b) Pt10-H with H absorbed on a peripheral Pt atom, (c) Pt10-H+ with H+ absorbed on a center Pt atom, and (d) Pt10–H+ with H+ absorbed on a peripheral Pt atom. No significance is attached to the relative sizes of the spheres.

Table 1

Calculation conditions and results for Pt10–H and Pt10–H+ as model hydrogen species in the electrode catalyst phase.

Entry no.Model molecule/ionCalculation conditionsOptimised structurea
Total chargeSpin multiplicityStructure No. on Figure 2Position of H/H+Mulliken charge on H/H+Pt–H/H+ bond distance/ÅRPFRb at 25 °CRPFRb at 39 °C
1Pt10–H02(1)Central0.2151.5604.22163.8681
204(1)Pt0.2141.5624.27613.9125
302(2)Peripheral0.0981.5683.76123.4727
404(2)Pt0.0941.5683.71583.4340
5Pt10–H+11(3)Central0.2471.5634.30563.9372
613(3)Pt0.2471.5594.24833.8909
711(4)Peripheral0.1431.5673.91233.6004
813(4)Pt0.1491.5623.87643.5729

aOptimised with keywords; SCF=(QC, maxcycle=200); opt=(maxcycle=200, modredundant).

bWith no frequency scaling.

Two types of optimised structures were obtained. In one structure, an H+ ion (or an H atom) is bonded to the central Pt atom of the Pt10 cluster surface, as shown in Figure 2a or c. In the other structure, the H+ (H) is bonded to a peripheral Pt atom of the Pt surface, as shown in Figure 2b or d. Even in the cases where the H+ (H) was positioned above the midpoint of two adjacent Pt atoms in the Gaussian input, the final converged structure was either of the two structures. We may thus conclude that the optimised structures shown in Figure 2 are the most stable ones for the Pt10–H+ and Pt10–H systems and that the H+ (H) directly interacts with one of the Pt atoms and does not form bonds of similar strength with multiple Pt atoms at a time.

The values of the Mulliken charge on the H+ ion (and a H atom) are listed in the seventh column of Table 1. The value of the Mulliken charge on the H+ ion is larger than that on the corresponding H atom, simply because the total charge of the Pt10–H+ is set to 1.0 whereas it is zero for Pt10–H. It is also seen that the values of Mulliken charge for the H+ ion (the H atom) bonded to the central Pt atom of the cluster are larger than that bonded to the peripheral Pt atom of the cluster. In addition, the SM has little influence on the Mulliken charge of H+ (H).

The experimental Pt-H distance of a PtH molecule is reported to be 1.529 Ǻ [7]. The computed Pt–H distance of the PtH molecule at the UB3LYP/LanL2dz level of theory is 1.543 Ǻ, which agrees with the experimental one within the 1 % error. The present Pt–H+ and Pt-H bond distances for the Pt10–H+ and Pt10–H systems range from 1.559 to 1.568 Ǻ and are slightly larger than that of the PtH molecule. This difference may be attributable to the difference in the number of Pt atoms involved in the two systems. It is also seen in Table 1 that The Pt–H+ and Pt–H bond distances are independent of the value of the SM and the kind of H species, H+ or H.

The experimental harmonic wave number of the PtH molecule is reported to be 2295 cm−1 [7]. On the other hand, the normal mode analysis of the same molecule at the UB3LYP/LanL2dz level of theory yields 2288 cm−1, which is not very different from 2295 cm−1. In normal mode analyses of the Pt10–H+ and Pt10–H species, 27 wave numbers are obtained for all of the considered species, and among them, three wave numbers are real and the other 24 are zero as expected. The H/D RPFRs at 25 °C and 39 °C were calculated by using six real wave numbers calculated for the pairs of the H and D species and (6), and the results are summarised in the ninth and tenth columns of Table 1. The values of RPFRs at 25 °C for the Pt10–H+ and Pt10-H species range from 3.8764 to 4.3056 and from 3.7158 to 4.8707, respectively. For both Pt10–H+ and Pt10–H, the RPFR value for the H species bonded to the central Pt atom is larger than that bonded to a peripheral Pt atom. The SM has little effect on the RPFR value except for the cases of entries 1 and 2, for which the SM value of 4 gives a larger RPFR value than the SM value of 2.

The value of RPFR in general becomes larger for a more stiffly bonded atom [2], and the stiffness of the bond may primarily be reflected in the Pt–H bond distance in the present case. That is, the H species with a shorter H–Pt bond distance is expected to have a larger RPFR value. This general view seems to be directly applied to the Pt10–H species. For the given SM value, the H atom bonded to the central Pt has a larger RPFR value that that bonded to the peripheral Pt atom, because the former has a shorter Pt–H bond distance than the latter. The general view, however, is not applied to the Pt10–H+. A shorter bond distance does not necessarily resulted in a larger RPFR value for a given SM value. For the Pt10–H+, the number of second closest Pt atoms may be important. That number is six for the H+ bonded to the central Pt atom, while it is only two for the H+ bonded to the peripheral Pt atom, which may account for the larger RPFR value of the former H+ than that of the latter H+.

The value of the H/D RPFR at 25 °C for the Pt–H+ in which surfaces of the Pt catalyst were approximated by a single Pt atom was calculated to be 3.6381 in our previous study [1]. This value is slightly raised to 3.6505 if we set the mass of the Pt atom at 1016 as in the case of the present study. This enhancement in the RPFR value with increasing Pt mass is reasonable, since only the H+ ion moves in the Pt-H stretching and other vibrational modes when the Pt atoms are given an artificially large mass. The present model of the H+ on the Pt catalyst surface, Pt10-H+, yielded the RPFR value of 3.8764 ∼ 4.3056 at 25 °C, larger than the RPFR value for the Pt–H+. This difference in the RPFR value between the present and previous models may be ascribable to the fact that, while only the Pt–H stretching mode contributes to the H/D RPFR in the previous model, the Pt-Pt-H bending modes also contribute to the RPFR in addition to the stretching mode.

To check the basis set dependence of the value of the H/D RPFR, the structures of the Pt10–H+ species were optimised and their RPFR values at 25 °C were calculated using the frequencies obtained at the optimised structures at the UB3LYP/cep-4g level of theory. The value computed was 4.2394, 4.2786, 3.9045 and 3.8937 for entries 5, 6, 7, and 8 of Table 1. The mean difference in the RPFR value between UB3LYP/LanL2dz and UB3LYP/cep-4g was 1.6 %.

3.2 Model Hydrogen Species in the Electrolyte Membrane Phase and Their RPFRs

The optimised structure of the model of the electrolyte membrane phase, C5F11-SO3···H3O+ (H2O)7, is depicted in Figure 3, in which the H3O+ ion is circled with the dotted line, and some structural parameters are summarised in Table 2. In the optimised structure, one of the three Hs of H3O+ interacts with one of the O atoms of the −SO3 group. That H atom is indicated by an arrow (→) in Figure 3. The H3O+ part of H3O+(H2O)7 can be distinguished from the H2O parts since, while H2O has only two O–H covalent bonds with the bond distance of ca 1 Ǻ, H3O+ has three O–H covalent bonds. However, it is impossible to specify which H among the three Hs of H3O+ is actually H+.

Figure 3: Optimised structure of C5F11-SO3−···H3O+(H2O)7 as the model hydrogen species in electrolyte membrane phase. The H3O+ ion is shown in the dotted circle. The H with an arrow directly interacts with an O of the −SO3− group. No significance is attached to the relative sizes of the spheres.
Figure 3:

Optimised structure of C5F11-SO3···H3O+(H2O)7 as the model hydrogen species in electrolyte membrane phase. The H3O+ ion is shown in the dotted circle. The H with an arrow directly interacts with an O of the −SO3 group. No significance is attached to the relative sizes of the spheres.

Table 2

Calculation results for C5F11-SO3···H3O+(H2O)7 as the model hydrogen species in the electrolyte membrane phase.

Entry no.Substituted HO–H bond distance/ÅaRPFRb at 25 °CRPFRb at 39 °C
PositionHydrogen bond
1H of H3O+Interacting with O of H2O1.04312.742210.9481
2H of H3O+Interacting with O of SO30.99515.575813.3134
3H of H2OInteracting with O of H2O1.01714.656612.5337
4H of H2OInteracting with O of H2O1.00914.434812.3716
5H of H2ONone0.97113.409811.6643
6H of H2ONone0.97513.870911.9958

aO–H covalent bond distances of in H2O or H3O+.

bWith no frequency scaling.

In the present calculations, the O–H bond distance of H3O+ range from 0.995 to 1.043 Ǻ, and that of H2O range from 0.971 to 1.017 Ǻ. The O···H intermolecular bond distance, i.e., the hydrogen bond (HB) distance among the H3O+ ion and the seven H2O molecules are from 1.313 to 1.635 Ǻ. The O···H bond distance between the H of H3O+ and the O of −SO3 is 1.687 Ǻ.

The values of the Mulliken charge for the H atoms of H2O molecules surrounding the H3O+ ion and the −SO3 group range from 0.3708 to 0.4852, and a tendency is observed that the H atom interacting with the O atom of a neighbouring H2O molecule has a larger Mulliken charge value than those with no such interaction. Against our surmise, a tendency that the three H atoms of H3O+ have larger Mulliken charge values than the Hs of the H2O molecules is not observed. The Mulliken charge value of the H atom of H3O+ interacting with the O atom of the −SO3 group is 0.4476 and smaller than that of the other two Hs of H3O+, 0.4885 and 0.4899.

For six H atoms from seventeen H atoms of C5F11-SO3···H3O+ (H2O)7, the H/D RPFR values at 25 °C and 39 °C were calculated and results are listed in the 5th and 6th columns of Table 2. The selected six H atoms are categorised into three types; 1) those directly interacting with the O atom of the neighbouring H2O molecule, 2) those directly interacting with an O atom of the −SO3 group, and 3) those without interaction, as shown in the 3rd column of Table 2. Among the RPFR values computed at 25 °C, the largest value of 15.5758 is obtained for the H atom (the one marked with an arrow in Fig. 3) of H3O+ interacting with an O atom of the −SO3 group. The result indicates that this H atom strongly interacts with the O atom, though the value of the Mulliken charge on this H atom is not very specific compared with those of other H atoms.

It is observed that the H atom with a HB has a larger RPFR value that the one without a HB. That is, hydrogen bonding enhances the RPFR value of a H atom of a H2O in an aqueous system, which is consistent with the results of our previous study, in which H/D RPFRs are estimated for water clusters [8, 9].

The smallest value of RPFR at 25 °C, 12.7422, is observed for an H atom of H3O+ (entry 1 of Tab. 2) with a HB whose distance is 1.444 Ǻ, which is within the range of computed hydrogen bond distance of 1.313–1.635 Ǻ. This value is smaller than those of H atoms with no HB, which is against the general view above that hydrogen bonding enhances the RPFR value of a H atom of a H2O molecule. The reason may be ascribable to the lengthened O-H covalent bond of 1.043 Ǻ caused by the formation of the HB.

As we reported in the previous article [1], the value of the H/D RPFR for the isolated H2O molecule or a H2O molecule in vacuo, is 12.2181 at 25 °C, which is smaller than 13.4098–14.6566 obtained for H2O molecules with no direct interaction in the structure of C5F11-SO3···H3O+ (H2O)7. This indicates that the RPFR of an H atom with no direct interaction is slightly enhanced by the presence of H2O molecules and the −SO3 group around the H2O molecules the H atom belongs to, possibly through the O-H covalent bond. As for the H3O+ ion, the value of the RPFR for the H3O+ ion in vacuo is 14.4640 [1], which is in between the values obtained for the interacting Hs of H3O+ in C5F11-SO3···H3O+ (H2O)7 in the present study.

3.3 H/D Isotope Exchange Equilibria at 39 °C between the Electrode Catalyst Phase and the Electrolyte Membrane Phase

During FC operations, H (and D) atoms trapped on surfaces of the Pt catalyst are expected to be oxidised to H+ (D+) ions and transferred to the electrolyte membrane phase. This means that the chemical form of hydrogen on the catalyst surface in equilibrium with hydrogen in the electrolyte membrane phase is the H+ (D+) ion. Thus, we regard the average of the four RPFR values at 39 °C evaluated for the Pt10-H+ species (entries 5, 6, 7, and 8 in Tab. 1) as the RPFR value for the H species in the electrode catalyst phase. The value is 3.7503 at 39 °C.

All six hydrogen species shown in Table 2 can be candidates for H species expected to exist in the electrolyte membrane phase during FC operations. Therefore, we consider 12.1378, the simple arithmetic average of six RPFR values at 39 °C shown in Table 2 as the RPFR value for the H species in the electrolyte membrane phase.

The equilibrium constant of Reaction (2), K2, is given as

(9)K2=felec/fcat, (9)

where the values of fcat and felec are 3.7503 and 12.1378, respectively, as estimated. So, K2 at 39 °C is calculated as 3.2365. The value of K2 is larger than unity, which means that the heavier isotope D is preferentially fractionated into the electrolyte membrane phase. Moreover, it is close to the value of the experimentally obtained S, which ranged from 3.46 to 3.99 at 39 °C [1].

In our previous study [1], the model H species for the electrode catalyst phase and the electrolyte membrane phase were the isolated Pt-H+ ion, and the isolated H2O molecule and the isolated H3O+ ion, respectively, the simplest ones among conceivable models. RPFR values at 39 °C for Pt-H+, H2O and H3O+ were calculated as 3.3814, 10.7055 and 12.5265 respectively. Using these values, K3 of (7) and K4 of (8) at 39 °C are 3.1660 and 3.7045, respectively. The present K2 value of 3.2365 is in between those two values. This means that the value of equilibrium constant of Reaction (2) little depends on the kind of adopted models. In other words, the effect of interactions like hydrogen bonding on the H/D RPFR is very localised; the interaction only affects the RPFR of the H species that is directly involved in that interaction and has little influence on the RPFRs of neighbouring H species. This result is consistent with that obtained for the H/D RPFRs of water clusters [8].

Two ways to check the validity of the aforementioned considerations are conceivable. One is to compare the calculated wave numbers with experimentally obtained vibration data. To obtain vibrational data experimentally, however, seems difficult even with the state-of-the-art equipment. Another is to carry out calculations using systems that are bigger and closer to real systems than the systems employed in this study. Those systems should include more than one hydrogen atoms and/or hydrogen ions adsorbed on the Pt catalyst surface. We have already started the study based on the second approach.

4 Conclusions

To summarise the present study, we make the following statements. H/D isotope effects upon polymer electrolyte membrane fuel cell operations were analysed by density functional theory calculations. RPFRs for the Pt10–H+ ion, the model H species in the electrode catalyst phase and for the C5F11–SO3···H3O+ (H2O)7 cluster, the model H species in the electrolyte membrane phase were estimated. In the geometry optimisation of Pt10-H+, all the Pt atoms were frozen at their experimental positions, and in the vibrational analysis, their weights were set at an artificially large value of 1016. The RPFR values for the electrode catalyst phase and for the electrolyte membrane phase at 39 °C were estimated to be 3.7503 and 12.1378, respectively. Using those values, the H/D isotope exchange equilibrium constant between the two phases could be calculated as 3.2365, which was close to the value of the experimentally obtained H/D isotope separation factor that ranged from 3.46 to 3.99 at 39 °C. It was thus highly probable that H+ ions on surfaces of the Pt catalyst and H species in the electrolyte membrane phase were isotopically in equilibrium with each other during FC operations.


Corresponding author: Satoshi Yanase, Faculty of Science and Technology, Sophia University, 7-1 Kioicho, Chiyodaku, Tokyo, 102-8554, Japan, E-mail:

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Received: 2015-1-10
Accepted: 2015-3-26
Published Online: 2015-4-29
Published in Print: 2015-6-1

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