Literature DB >> 35312369

A completely precious metal-free alkaline fuel cell with enhanced performance using a carbon-coated nickel anode.

Yunfei Gao1, Yao Yang2, Roberto Schimmenti3, Ellen Murray3, Hanqing Peng1, Yingming Wang1, Chuangxin Ge1,4, Wenyong Jiang1, Gongwei Wang1, Francis J DiSalvo2, David A Muller5,6, Manos Mavrikakis3, Li Xiao1, Héctor D Abruña2, Lin Zhuang1,4.   

Abstract

SignificanceWe present a groundbreaking advance in completely nonprecious hydrogen fuel cell technologies achieving a record power density of 200 mW/cm2 with Ni@CNx anode and Co-Mn cathode. The 2-nm CNx coating weakens the O-binding energy, which effectively mitigates the undesirable surface oxidation during hydrogen oxidation reaction (HOR) polarization, leading to a stable fuel cell operation for Ni@CNx over 100 h at 200 mA/cm2, superior to a Ni nanoparticle counterpart. Ni@CNx exhibited a dramatically enhanced tolerance to CO relative to Pt/C, enabling the use of hydrogen gas with trace amounts of CO, critical for practical applications. The complete removal of precious metals in fuel cells lowers the catalyst cost to virtually negligible levels and marks a milestone for practical alkaline fuel cells.

Entities:  

Keywords:  alkaline fuel cells; carbon coating; hydrogen oxidation reaction; nickel anode; nonprecious

Year:  2022        PMID: 35312369      PMCID: PMC9060468          DOI: 10.1073/pnas.2119883119

Source DB:  PubMed          Journal:  Proc Natl Acad Sci U S A        ISSN: 0027-8424            Impact factor:   12.779


As one of the most promising hydrogen fuel cell technologies, alkaline polymer electrolyte fuel cells (APEFCs) have attracted great interest due to their potential to completely eliminate the need for precious metal catalysts (1–3). Although significant progress has been made in developing nonprecious metal catalysts for the oxygen reduction reaction, with activities comparable to that of noble metal catalysts (Pt, Pd, etc.) in alkaline media (4, 5), the performance of nonprecious metal catalysts for the hydrogen oxidation reaction (HOR) is still below that of precious metal catalysts (6). Therefore, in order to replace Pt-based anode catalysts in APEFCs, it is necessary to develop high-performance and durable nonprecious metal catalysts for the HOR. Nickel-based systems remain the most active nonprecious HOR metal catalysts with promising activity (7). However, the activity of common Ni catalysts is about two orders of magnitude lower than that of state-of-the-art Pt/C catalysts (8). Several strategies have been proposed to enhance the activity of Ni-based HOR catalysts, such as alloying with other transition metals [e.g., NiFe (9), NiCu (10, 11), and NiCoMo (12)], doping with N (13), or forming metal nitrides (14, 15). However, there are few studies that address the stability of Ni (16), especially under the operation conditions of APEFCs. It should be noted that nickel oxide species form above ∼0.2 V versus reversible hydrogen electrode (RHE), which passivates the Ni catalysts (7). This instability at high potentials significantly limits their electrochemical active window. Although nickel oxides/hydroxides have been reported to enhance HOR catalytic activity of Ni (17–20), further oxidation of Ni eventually deactivates the catalysts (16). Thus, it is pivotal to investigate the durability of Ni-based catalysts, especially during fuel cell operation. It was recently reported that surface coating can tune the electronic structure of a metal surface and improve the stability of catalysts (21–23). Small molecules such as H2 can access the metal surface through the surface coating, where the catalytic reactions can proceed (21). Thus, utilizing the surface coating is regarded as a promising strategy to protect Ni and other metals from oxidation while maintaining high HOR activity. In a previous study (24), we found that Ni coated with hexagonal boron nitride can improve HOR activity and stability. In this work, a Ni-based electrocatalyst with a 2-nm nitrogen-doped carbon shell (Ni@CNx) was synthesized via facile thermal treatment (25–27). The shell was found to prevent the metal catalyst from oxidizing, enhancing its durability under HOR reaction conditions. The peak power density (PPD) of APEFC using this Ni@CNx catalyst as the anode reached 480 mW/cm2 with a Pt/C cathode and 210 mW/cm2 with a spinel MnCo2O4 cathode at 80 °C using pure H2 and O2 as reactant gases. Ni@CNx showed a PPD of 280 mW/cm2 using H2 mixed with 100 ppm CO and CO2-free air as reactant gas, which suggested a significantly better CO tolerance of Ni@CNx relative to Pt/C.

Results

In this work, Ni@CNx was synthesized by a facile thermal treatment employing urea and nickel acetate. The crystal structure of Ni@CNx was investigated using aberration-corrected scanning transmission electron microscopy (STEM) at the atomic scale. Ni@CNx exhibited an average particle size of around 45 nm (). The mild particle aggregation observed is likely due to the high-temperature pyrolysis treatment. As shown in the bright-field (BF) STEM image (Fig. 1), a thin shell of lighter elements that was detected on the surface. BF-STEM imaging is based on the phase contrast of electrons and is more sensitive to light elements such as carbon, while the image intensity in annular dark-field (ADF) STEM scales with the atomic number (I ∝ Z1.7) and heavier elements such as Ni (Z = 28) will be much brighter than C (Z = 6) (21) (Fig. 1). The thin shell on the surface was better resolved at the atomic-scale STEM image in Fig. 1. Ni@CNx exhibited the shell (red) and core (green) regions as well as the interface (cyan). The shell showed d-spacings of 3.4 Å, a characteristic value of graphitized carbon (PDF #04–006-5764). The atomic-scale STEM image in Fig. 1 was selected from the particle in and showed the hexagonal symmetry of face-centered cubic (fcc) Ni on the [110] zone axis, as indicated by the hexagonal diffraction spots in the Fourier transform (Fig. 1, Inset). Dominant facets, including (111) (2.0 Å) and (200) (1.8 Å), were resolved on the atomic-scale STEM image, which matched well with the theoretical values of 2.04 and 1.76 Å, respectively, from the crystal model on the same [110] zone axis (Fig. 1). A hexagonal unit cell was composed by two nearby sides of 2.2 and 2.5 Å, which were consistent with the theoretical values of 2.17 and 2.51 Å, respectively. The aforementioned STEM imaging analysis suggested that the fcc-Ni was surrounded by a 1- to 3-nm shell of N-doped carbon on the surface.
Fig. 1.

Atomic-scale STEM imaging and EELS spectroscopic analysis of core-shell Ni@CNx electrocatalysts. (A) BF STEM image of a Ni NP core coated with a thin carbon shell. Dashed box shows the region that is magnified in B. (B) Atomic-scale BF-STEM image of the interface between Ni (green) and C (red) as well as the 1-nm transition region (cyan). (C and D) Atomic-scale BF-STEM images of the fcc-type metallic Ni with d-spacings of {111} and {200} and hexagonal-like symmetry. The corresponding crystal model in D was established on the same zone axis of [110] and exhibited d-spacings and symmetry consistent with the image in C. Inset shows the diffractogram of the lattice image. (E–H) ADF-STEM image and EELS elemental maps of Ni (green), C (red), and the composite map of Ni versus C. (I) EELS line profile, extracted from the dashed box in (H), exhibited the carbon shell with a thickness of 1 to 3 nm. (J) Energy-loss near-edge structure (ELNES) of the L3 and L2 edges of metallic Ni at 853 and 871 eV, respectively. The shoulder peak at around 860 eV is due to the hybridization of Ni 2p and 3d orbitals. a.u., arbitrary units; FT, Fourier transform.

Atomic-scale STEM imaging and EELS spectroscopic analysis of core-shell Ni@CNx electrocatalysts. (A) BF STEM image of a Ni NP core coated with a thin carbon shell. Dashed box shows the region that is magnified in B. (B) Atomic-scale BF-STEM image of the interface between Ni (green) and C (red) as well as the 1-nm transition region (cyan). (C and D) Atomic-scale BF-STEM images of the fcc-type metallic Ni with d-spacings of {111} and {200} and hexagonal-like symmetry. The corresponding crystal model in D was established on the same zone axis of [110] and exhibited d-spacings and symmetry consistent with the image in C. Inset shows the diffractogram of the lattice image. (E–H) ADF-STEM image and EELS elemental maps of Ni (green), C (red), and the composite map of Ni versus C. (I) EELS line profile, extracted from the dashed box in (H), exhibited the carbon shell with a thickness of 1 to 3 nm. (J) Energy-loss near-edge structure (ELNES) of the L3 and L2 edges of metallic Ni at 853 and 871 eV, respectively. The shoulder peak at around 860 eV is due to the hybridization of Ni 2p and 3d orbitals. a.u., arbitrary units; FT, Fourier transform. In an effort to further elucidate the chemical environment of Ni@CNx catalysts, electron energy-loss spectroscopy (EELS) under STEM mode was employed to investigate the elemental distribution and assess bonding information. The Ni-core and C-shell structure became startlingly clear (Fig. 1 ) when EELS elemental maps were extracted using Ni L3 and C K edges (). The EELS map of Ni and C in Fig. 1 and the composite EELS map of Ni versus C in Fig. 1 suggested that the Ni in the core was surrounded by a uniform C shell on the surface. EELS line profiles were extracted from the dashed box in Fig. 1 and quantitatively showed the carbon shell with a thickness of 1 to 3 nm (Fig. 1). Additional examples of EELS mapping analysis of other Ni@CNx confirmed that the carbon shell uniformly covered the Ni core with a thickness of 1 to 3 nm (). To gain a detailed description of the local electronic structure of Ni in the catalyst, we performed energy-loss near-edge structure (ELNES) analysis with a high energy resolution of 0.5 eV (Fig. 1). ELNES serves as the fingerprint of elements and reflects the density of unfilled states (unfilled density of states) above the Fermi level (EF), which is particularly sensitive to the local atomic environment, such as valence state, chemical bonding, and coordination environment (2, 28, 29). The ELNES of Ni exhibited the characteristic sharp L3,2 edges of metallic Ni ([Ar]3d94s1) (Fig. 1), which is consistent with the EELS reference of metallic Ni thin film (). The L3 edge was located at around 853 eV (2p3/2 to 3d3/23d5/2 transition) and had a stronger intensity than the L2 edge located at around 871 eV (2p1/2 to 3d3/2 transition) due to the higher transition probability. The shoulder peak at around 860 eV is due to the hybridization of the 2p and 3d orbitals of metallic Ni (30). If the metallic Ni were oxidized to NiO, the multiplet structure of NiO would emerge in the EELS spectrum () (31). The absence of a NiO signal suggested a metallic Ni in the core of the Ni@CNx catalysts. The ELNES spectra from more than five different regions confirmed the existence of metallic Ni (). Rotating disk electrodes (RDEs) were used to assess the HOR activity of Ni@CNx catalysts. To rigorously study the impact of the shell on the catalyst durability during the HOR, we selected Ni nanoparticles (NPs) with comparable particle sizes to the Ni@CNx catalysts (). Fig. 2 shows the HOR polarization curves for Ni@CNx and the Ni NP counterpart. At a metal loading of 0.5 mg/cm2, the Ni@CNx exhibited a better stability compared to Ni NPs. Even at a potential of 0.4 V versus RHE, the Ni@CNx exhibited clear anodic current while Ni NPs were completely inactive, with the current dropping to nearly zero. The lower HOR current density in the negative-going scan is due to the formation of a surface oxide passivation layer as shown by the dashed arrows in Fig. 2. Given that the HOR occurs primarily on Ni sites, the enhanced HOR activity of Ni@CNx relative to Ni NPs is possibly/likely due to the presence of the N-doped carbon shell, which tunes the electronic structure of Ni and suppresses the formation of Ni oxide at high polarization potentials. Previous studies have also suggested that the enhanced activity of Ni@CNx catalysts compared to Ni NPs was possibly due to the coated carbon shell (32) and/or N elemental doping (14, 33). An increase of Ni@CNx catalyst loading on the glassy carbon electrode yielded higher anodic currents ().
Fig. 2.

The electrocatalytic performance of Ni@CNx compared with Ni NPs (Ni). (A) RDE profiles recorded at a rotation rate of 2,500 rpm and a scan rate of 5 mV/s. Ni@CNx electrocatalysts (blue) and Ni NPs (red). Dashed arrows reflect the positive- and negative-going directions in the CV scans. (B) Current density of Ni@CNx and Ni NPs measured at 0.05 V after 10,000 potential cycles from −0.1 to 0.4 V versus RHE. (C) Single-cell performance with anode catalysts of Ni@CNx and Ni NPs with a loading of 15 mgNi/cm2 and cathode catalysts of 60 wt % Pt/C with a loading of 0.4 mgPt/cm2. The Inset describes a stability test at a constant potential polarization at 0.6 V. (D) APEFC performance using Ni@CNx as anode (15 mgNi/cm2) and 80 wt % MnCo2O4 (1.5 mgoxide/cm2) cathode catalysts. Red and blue curves represent power density and cell voltage as a function of current density, respectively. Fuel cell operation conditions in Fig. 2 : cell temperature of 80 °C, gas back pressure of 0.2 MPa on both sides of the cell. Fully humidified H2 and O2 were fed at a flow rate of 500 mL/min. Open and closed data points in C and D represent the cell voltage and power density, respectively.

The electrocatalytic performance of Ni@CNx compared with Ni NPs (Ni). (A) RDE profiles recorded at a rotation rate of 2,500 rpm and a scan rate of 5 mV/s. Ni@CNx electrocatalysts (blue) and Ni NPs (red). Dashed arrows reflect the positive- and negative-going directions in the CV scans. (B) Current density of Ni@CNx and Ni NPs measured at 0.05 V after 10,000 potential cycles from −0.1 to 0.4 V versus RHE. (C) Single-cell performance with anode catalysts of Ni@CNx and Ni NPs with a loading of 15 mgNi/cm2 and cathode catalysts of 60 wt % Pt/C with a loading of 0.4 mgPt/cm2. The Inset describes a stability test at a constant potential polarization at 0.6 V. (D) APEFC performance using Ni@CNx as anode (15 mgNi/cm2) and 80 wt % MnCo2O4 (1.5 mgoxide/cm2) cathode catalysts. Red and blue curves represent power density and cell voltage as a function of current density, respectively. Fuel cell operation conditions in Fig. 2 : cell temperature of 80 °C, gas back pressure of 0.2 MPa on both sides of the cell. Fully humidified H2 and O2 were fed at a flow rate of 500 mL/min. Open and closed data points in C and D represent the cell voltage and power density, respectively. To further investigate the role of the N-doped carbon shell on the performance of Ni@CNx catalysts, the thickness of the shell was tuned by varying the mass ratio of the nickel acetate and urea precursors. The pyrolysis process of urea may have generated stable N−C bonds when the carbon shell was formed, which would help control the thickness of the CNx shell (34). TEM images of Ni@CNx with different thickness of the shells are shown in . With an increasing amount of urea, the CNx shell thickness decreased from 5 nm for Ni@CNx-1 to 3 nm for Ni@CNx-2 and 1 nm for Ni@CNx-3. The X-ray diffraction (XRD) patterns and X-ray photoelectron spectroscopy (XPS) spectra () of Ni@CNx catalysts suggested that varying the mass ratios of nickel acetate and urea did not change the structure or chemical environment of Ni. Additionally, the relative ratio of nitrogen to carbon (N/C) increased with a larger amount of urea from 1.65 to 6.84% (). The N was incorporated in the carbon shell forming C−N bonds, which is consistent with the XPS spectrum of N 1s (). Additionally, no evidence of metal−N bond formation was found in the ELNES of Ni ( and Fig. 1), which suggests that N defects do not directly interact with the Ni electrocatalyst surface. As shown in , the HOR activity of Ni@CNx-2 and Ni@CNx-3, with thinner shells of 3 and 1 nm, respectively, increased, while their stability decreased relative to Ni@CNx-1 with a shell of 5 nm. Ni@CNx-2 with a medium shell thickness of 3 nm showed a good balance between HOR activity and stability. To further evaluate the stability of Ni@CNx catalysts, the HOR currents were also characterized by chronoamperometry at different potentials (). With thinner shells, Ni@CNx-2 and Ni@CNx-3 showed a higher current at 0.1 V and 0.2 V but lower current at 0.3 V and 0.4V, confirming the enhanced activity and slightly compromised stability relative to Ni@CNx-1. After a series of polarizations from 0.1 to 0.4 V, the catalysts were then polarized at 0.1 V. The current values were nearly identical to the initial polarization at 0.1 V, suggesting a good stability for Ni@CNx. Accelerated durability tests (ADTs) were also performed to evaluate the stability of Ni@CNx catalysts in alkaline media by performing 10,000 potential cycles between −0.1 and 0.5 V. As shown in Fig. 2, Ni NPs experienced a decay of the current density at 0.05 V by about 80%; in contrast, Ni@CNx exhibited a decay of less than 10%, indicating its significantly enhanced durability in alkaline media. Cyclic voltammetric (CV) profiles of Ni@CNx and Ni NPs before and after ADTs are shown in . While the redox current of Ni NPs experienced a severe decay, the current of Ni@CNx was minimally affected. The Ni@CNx catalyst was then employed as the anode in membrane electrode assembly (MEA) measurements in an APEFC (Fig. 2). With an optimal metal loading of 15 mg/cm2, a Ni@CNx anode with a Pt/C cathode achieved a PPD of 480 mW/cm2, while the PPD for Ni NPs was only 130 mW/cm2. When the catalyst loadings of Ni@CNx were varied from 5 to 15 mg/cm2, the PPD also increased from 250 mW/cm2 to 480 mW/cm2 (). Further increases in catalyst loading did not yield a significant enhancement in the PPD, which was mainly limited by the slower mass transport and charge transfer (35). MEA performance with different back pressures, Pt loadings, and operation in synthetic air or CO2-containing air was examined to evaluate the “practicality” of the Ni@CNx catalyst system (). Aiming for a practical APEFC, we evaluated the durability of the Ni@CNx catalyst during cell operation by applying a constant potential polarization of 0.6 V. As shown in the inset of Fig. 2, the current density of Ni@CNx remained stable at about 600 mA/cm2 for 20 h. At a constant current density of 200 mA/cm2, Ni@CNx exhibited stable fuel cell operation for over 100 h (). However, the current density of Ni NPs rapidly decreased from 200 mA/cm2 to nearly zero within 5 h under the same test conditions. The promising durability of the Ni@CNx anode is a groundbreaking achievement for nonprecious HOR catalysts since no durable nonprecious HOR electrocatalysts operating at large current density in APEFCs have been reported before. Aiming for completely nonprecious metal catalysts for APEFCs, we combined a Ni@CNx anode (15 mgNi/cm2) with a high-loading 80 wt % MnCo2O4 (1.5 mgoxide/cm2) cathode, which had previously shown comparable MEA performance to a Pt/C cathode (36). As shown in Fig. 2, the PPD of cell performance using a Ni-based anode and MnCo2O4 cathode achieved a record of 210 mW/cm2. To the best of our knowledge, the MEA performance of this Ni−Mn−Co fuel cell represents the highest among alkaline fuel cells with completely precious metal–free catalysts in both the anode and cathode published to date (). MEA performances with a Ni@CNx anode and Co−Mn cathode in realistic H2/syn-air exhibited a PPD of ∼90 mW/cm2 (). This proof of concept with completely nonprecious MEAs, with a Ni@CNx anode and a Co−Mn cathode, lowered the catalyst cost to virtually negligible levels. While it is prudent to target fuel cell performance for high-power–density automotive applications, it is also appropriate to keep the requirements of other fuel cell markets in mind (37, 38). The Ni/Co−Mn alkaline fuel cells could pave the way for low-power–density industrial applications, such as backup power or portable power, which prioritize low cost and longevity rather than the high-power density required for electric vehicles. The decrease of hydrogen oxidation current at higher polarizations of Ni-based catalysts is generally ascribed to the formation of Ni(OH)2 in α-form and/or β-form (39–41). Although the formation of Ni(OH)2 was reported to enhance the HOR activity of Ni-based catalysts (17–19), excessive oxidation will lead to poor HOR activity and stability (13). To better understand how the shell helped improve the stability of HOR, we employed XPS to study the near-surface chemical environment of Ni after polarization at 0.1 V and 0.3 V. As shown in Fig. 3 , after polarization at different potentials, the chemical environment of Ni changed significantly, which consisted of three components: metallic Ni, NiO, and Ni(OH)2. The surface of the Ni@CNx sample without polarization was dominated by metallic Ni, while the Ni NPs had lower metallic Ni content and more oxide/hydroxide, which indicated that the Ni@CNx catalyst exhibited a better oxidation resistance under exposure to air. When the potential was increased from 0.1 V to 0.3 V, the relative content of metallic Ni in Ni@CNx decreased from 63 to 28%, while the Ni NPs showed a more severe decay from 45 to 11%. When the majority of the metallic Ni was oxidized to Ni(OH)2, the anodic current of Ni NPs decayed rapidly, especially at polarization potentials above 0.2 V (). In comparison, Ni@CNx catalysts exhibited a better oxidation resistance at high potentials by inhibiting Ni(OH)2 formation.
Fig. 3.

XPS and TPD profiles of Ni@CNx compared with Ni NPs. (A–C) XPS spectra of Ni2p3/2 of Ni@CNx and Ni NPs after constant potential polarization for 1 h. (D) TPD of oxygen adsorbed on Ni@CNx, Ni and CNx shell, both of which had been baked in air at 60 °C for 12 h before the test, clearly showing a weakening in the Ni−O bond strength induced by the presence of the CNx shell.

XPS and TPD profiles of Ni@CNx compared with Ni NPs. (A–C) XPS spectra of Ni2p3/2 of Ni@CNx and Ni NPs after constant potential polarization for 1 h. (D) TPD of oxygen adsorbed on Ni@CNx, Ni and CNx shell, both of which had been baked in air at 60 °C for 12 h before the test, clearly showing a weakening in the Ni−O bond strength induced by the presence of the CNx shell. Additionally, the oxidation resistance through the shell of the Ni@CNx catalyst was also detected by temperature programmed desorption (TPD) measurements. As shown in Fig. 3, the peak temperature of Oads desorption from the Ni@CNx catalyst was downshifted by 37 °C compared with that on Ni NPs, which suggested that the Ni−O bond strength was weakened in the Ni@CNx catalysts (42). A temperature programmed oxidation analysis was also used to evaluate the oxidation resistance of Ni@CNx catalysts. As shown in , the peak temperature for the formation of oxygenated chemicals was upshifted by 40 °C compared with that on Ni NPs, indicating that the CNx shell can mitigate Ni oxidation. The tailing peak of the Ni@CNx sample shown in Fig. 3 was possibly due to the decomposition of the N-doped carbon shell. To study the structure of the shell, nitric acid was used to etch the Ni core to obtain just the N-doped carbon shell, which was visualized in STEM images (). The Raman spectra in indicated that there were a certain number of defects in the shell based on the D-to-G peak ratio to be 1.063 (23). Raman spectra of Ni@CNx before and after acid etching showed negligible changes of the D-to-G peak ratio. This acid etching experiment suggests that mesoporous structures of the CNx shell could allow the hydrated nickel ions to diffuse through the shell, which would also suggest that the reactants in fuel cells would be able to reach the surface of the Ni core. Additionally, according to surface area analysis (), the domain pore size of the pore size distribution was less than 2 nm, which provided confined channels to enhance the oxidation resistance. Finally, hydrogen TPD (H-TPD) was also used to evaluate the Ni−H bond strength, which showed that the peak temperature of Hads desorption from Ni@CNx catalysts was also downshifted by 17 °C compared to Ni NPs (). This indicates that the CNx shell could weaken the Ni−H bond strength to promote the Volmer step (Hads + OH− = H2O + e−) and thus improve the activity, which is consistent with our previous report (24). Practical APEFCs, operating in H2-air mode, face several challenges, including water management (2, 43, 44), carbonation of APE from air (45), and catalyst poisoning effects resulting from trace amounts of CO in H2, which is mainly produced from steam-reforming of hydrocarbons (22). Since Pt is particularly sensitive to CO poisoning (22), a high CO tolerance is pivotal to the design of nonprecious metal anode catalysts. Here, we exposed the anode catalysts to H2 gas with 100 ppm CO in MEA measurements. As shown in Fig. 4 , the PPD of Pt/C was severely degraded in H2 mixed with 100 ppm CO, which showed a dramatic decrease of ∼70%, from 0.71 W/cm2 to 0.20 W/cm2. On the other hand, Ni@CNx exhibited a much better CO tolerance, showing a significantly smaller decay in the PPD of only ∼14%, from 0.36 W/cm2 to 0.29 W/cm2. Constant current polarization measurements were also conducted to evaluate the catalyst’s CO tolerance. As shown in Fig. 4, both Pt/C and Ni@CNx catalysts were able to maintain a steady voltage of 0.83 V at 200 mA/cm2. However, the voltage of Pt/C dropped to 0.45 V in H2 mixed with 100 ppm CO, while the voltage of Ni@CNx showed a much smaller decay to 0.66 V, suggesting an impressive CO-tolerant behavior of Ni@CNx (Fig. 4). The resistance to CO poisoning is likely due to a weaker interaction strength between CO and Ni with the CNx shell protection.
Fig. 4.

The MEA performance of Ni@CNx anode compared with Pt/C anode in pure H2 and the addition of 100 ppm CO in APEFCs. (A and B) Cell performance with Ni@CNx anode (15 mg/cm2) compared with 20 wt % Pt/C (0.1 mg/cm2), both of which used 40 wt % Pt/C as cathode with a metal loading at 0.4 mg/cm2. The data in A used fully humidified pure H2 and synthetic air (syn-air, CO2-free) as reaction gas, while in B, fully humidified H2 mixed with 100 ppm CO was used as the anode reaction gas. (C and D) Constant current polarization at 200 mA/cm2 in both pure H2 and H2 with 100 ppm CO. Fuel cell operation conditions in Fig. 2 : cell temperature of 80 °C, gas back pressure of 0.2 MPa on both sides of the cell. Fully humidified H2 and air were fed at a flow rate of 500 mL/min.

The MEA performance of Ni@CNx anode compared with Pt/C anode in pure H2 and the addition of 100 ppm CO in APEFCs. (A and B) Cell performance with Ni@CNx anode (15 mg/cm2) compared with 20 wt % Pt/C (0.1 mg/cm2), both of which used 40 wt % Pt/C as cathode with a metal loading at 0.4 mg/cm2. The data in A used fully humidified pure H2 and synthetic air (syn-air, CO2-free) as reaction gas, while in B, fully humidified H2 mixed with 100 ppm CO was used as the anode reaction gas. (C and D) Constant current polarization at 200 mA/cm2 in both pure H2 and H2 with 100 ppm CO. Fuel cell operation conditions in Fig. 2 : cell temperature of 80 °C, gas back pressure of 0.2 MPa on both sides of the cell. Fully humidified H2 and air were fed at a flow rate of 500 mL/min. To shed light on the beneficial effects of the CNx coating on the Ni catalysts for the HOR, we used density functional theory (DFT) calculations. In particular, we examined the effect of coating thickness and of N-doping at coating defects. We employed a descriptor-based analysis starting from DFT-calculated binding energies of the HOR reaction intermediates H* and OH* and of the catalyst poison O*. The binding energy of H (BEH) has been proposed as a descriptor for HOR catalytic activity. By using DFT calculations at a comparable level of theory with respect to ours, Nørskov et al. (46) determined that the optimal HOR activity would be achieved for a BEH that would be less stable than that of Ni(111) by 0.27 eV. Therefore, any decrease in the magnitude of BEH on Ni(111) within that ∼0.3 eV window would be expected to lead to HOR activity improvement. We started our analysis with a simplified model for the Ni@CNx catalyst consisting of a monolayer of graphene supported on a Ni(111) surface in a top-fcc configuration (Ni@Graphene) (structure shown in ), which we determined to be the most stable structure for a graphene monolayer on Ni(111). The binding energy of the energetically most stable adsorption geometries of H*, OH*, and O* on this model are presented in Fig. 5 (numerical values for binding energies are reported in ). We note that H* and O* prefer to bind to the threefold sites of the metallic surface, whereas OH* is more stable on top of a C atom in the graphene coating, pointing away from the Ni surface. This finding suggests that the catalyst active sites for H2 dissociation and OH* adsorption can be different in the Ni@CNx catalyst. Furthermore, the preferential adsorption of OH* on the graphene coating could explain the enhanced durability of Ni@CNx, as Ni(OH)2 formation would be less extensive than on metallic Ni, in agreement with our XPS (Fig. 3) and CV measurements (). Importantly, the binding energy of H* bound directly to Ni on a Ni(111) surface covered by one layer of graphene is −2.62 eV. Compared to a pristine Ni(111) surface (BEH = −2.90), this reduced binding by 0.28 eV in the presence of graphene capping the Ni(111) would be sufficient to bring BEH right around the optimal BEH for the HOR (44). Our finding that the H* binding strength was destabilized by 0.28 eV is in qualitative agreement with the downshift in the H-TPD data shown in and can be the basis of the enhanced catalytic performance of Ni@CNx-1 and Ni@CNx-2 catalysts. Like H*, O* and OH* are also destabilized on Ni by the presence of the graphene coating. In particular, O* bound directly to a Ni(111) surface covered by one layer of graphene was destabilized by 0.80 eV compared to pristine Ni(111), in qualitative agreement with the peak downshift observed in the oxygen TPD profile in Fig. 3. Furthermore, by calculating the d-band center of Ni surface atoms in Ni(111) (−2.05 eV) and Ni@Graphene (−2.29 eV), we suggest that this negative shift of the d-band center by ∼0.25 eV () is responsible for the destabilization of all adsorbates on the Ni@Graphene model.
Fig. 5.

Binding energy of HOR reaction intermediates H* and OH* and catalyst poison O* on pristine Ni(111) and Ni@Graphene surfaces. Blue, red, and green bars indicate the binding energy of key intermediates on a pristine Ni(111) surface, on Ni on a graphene-coated Ni(111) surface, and on top of the graphene coating, respectively. Bolded red or green bars indicate the calculated most stable H*, OH*, and O* states in the presence of the graphene-coated Ni(111). The dashed horizontal line corresponds to the HOR-optimal binding of H*. A cross-sectional view of the most stable H*, OH*, and O* geometries is shown below the chart. Ni, C, O, and H atoms are represented by silver, brown, red, and green spheres, respectively.

Binding energy of HOR reaction intermediates H* and OH* and catalyst poison O* on pristine Ni(111) and Ni@Graphene surfaces. Blue, red, and green bars indicate the binding energy of key intermediates on a pristine Ni(111) surface, on Ni on a graphene-coated Ni(111) surface, and on top of the graphene coating, respectively. Bolded red or green bars indicate the calculated most stable H*, OH*, and O* states in the presence of the graphene-coated Ni(111). The dashed horizontal line corresponds to the HOR-optimal binding of H*. A cross-sectional view of the most stable H*, OH*, and O* geometries is shown below the chart. Ni, C, O, and H atoms are represented by silver, brown, red, and green spheres, respectively. To elucidate the role of N defects in the CNx coating, we performed this descriptor-based analysis on electrocatalyst models consisting of two layers of defective graphene, including pyridinic (PYR) and pyrrolic (PYL) defects, adsorbed on Ni(111). Additional details on the construction of these models are provided in the . The energy-optimized geometry of these models is shown in , and the respective binding energies of adsorbates on them are reported in . These results demonstrate that irrespectively of the defect topology studied, H is either too weakly bound [PYR(3N), and PYR(4N), ] or too strongly bound (PYL-r, ) to Ni@CNx models to explain the catalytic activity of the Ni@CNx catalysts toward the HOR. Our analysis suggests that the presence of N-containing defects alone cannot explain the origin of the enhanced electrocatalytic activity of Ni@CNx. Therefore, to explain the effect of N defects in Ni@CNx we propose an alternative model where Ni adatoms form under reaction conditions. Remarkably, our previous studies demonstrated that N-doping in graphene stabilizes single-metal atom catalysts with increased activity toward water splitting and CO oxidation (47, 48). Previous studies suggested that the synthesis of carbon-coated nickel NPs proceeds through formation of nickel carbide (Ni3C), followed by phase segregation of carbon to the shell and nickel to the core (25, 27). However, under synthesis or reaction conditions, it is possible that trace amounts of nickel atoms may be trapped in the graphitic CNx shell region. To determine the possible role of single-metal atoms trapped in N-substituted defects of graphene in the HOR, we calculated the binding energy of H*, OH*, and O* on a model Ni(111) surface coated with two layers of defective graphene in which PYR and PYL defects were saturated by a single Ni adatom. The energy-optimized geometries for these structures, without adsorbates, are shown in . Numerical values for the adsorbate binding energies on these structures are shown in , and the binding energy and optimized geometries for these structures with adsorbed OH* and O* are shown in , respectively. The BEH and the optimized structures of H* bound to supported Ni adatoms are shown in Fig. 6. The results reported in Fig. 6 corroborate the hypothesis that Ni adatoms supported on PYL (BEH = −2.72 eV) or PYR(3N) (BEH = −2.69 eV) defects may be the source of the increased activity toward the HOR, as they both reflect a destabilization of H* compared to H* on pristine Ni(111) by ∼0.2 eV. Interestingly, H* binds to Ni-adatom in the PYR(4N) defect much more weakly, and therefore we expect it plays no role in enhancing HOR activity in these catalysts. We noted that PYL defects, which are potentially responsible for the enhanced catalytic properties of Ni@CNx, constitute just a minority fraction of the defects, as suggested by their DFT-calculated relative stability () and by the XPS characterization analysis (). Thus, we propose that single Ni atoms bound to PYR (3N) graphene defects serve as one type of possible active sites of Ni@CNx for the HOR. In closing the discussion for the nature of the active site, we noted that the measured HOR activity improvement due to graphene coating (see Fig. 2) is approximately one order of magnitude, whereas the improvement that would correspond to ∼0.3-eV destabilization of H* would be ∼4 orders of magnitude. We suggest that the less-than-ideal activity enhancement in our Ni@CNx catalysts originates from other factors, such as O-containing defects in carbon layers (C–OH, C=O), not accounted for in our simplified models. One such factor could be the XPS-observed Ni(OH)2 phase (see Fig. 3) that may be adjacent to the metallic Ni phase, which would lead to a destabilization of H* by less than ∼0.3 eV, the value that corresponds to the ideal HOR catalyst. Fine-tuning our catalyst synthesis method to further reduce the presence of such factors and their influence could lead to even further improvements in HOR activity and catalyst stability.
Fig. 6.

Binding energy of H* on Ni@CNx models in the presence of Ni adatoms. The dashed line on the bar chart indicates the binding energy of H* on pristine Ni(111) (−2.90 eV). The dash-dotted line corresponds to the optimal binding of H* for the HOR. A cross-sectional view of the most energetically stable geometry for H* on each Ni@CNx model is shown below the chart. Ni, C, N, and H atoms are represented by silver, brown, blue, and green spheres, respectively. Graphene atoms in direct contact with Ni atoms in Ni@CNx models are colored in light brown, while graphene in the second layer is colored in dark brown.

Binding energy of H* on Ni@CNx models in the presence of Ni adatoms. The dashed line on the bar chart indicates the binding energy of H* on pristine Ni(111) (−2.90 eV). The dash-dotted line corresponds to the optimal binding of H* for the HOR. A cross-sectional view of the most energetically stable geometry for H* on each Ni@CNx model is shown below the chart. Ni, C, N, and H atoms are represented by silver, brown, blue, and green spheres, respectively. Graphene atoms in direct contact with Ni atoms in Ni@CNx models are colored in light brown, while graphene in the second layer is colored in dark brown. In summary, we have developed a facile method for synthesizing stable Ni@CNx catalysts with enhanced HOR activity and improved oxidation resistance relative to Ni NPs. The Ni@CNx catalysts remained stable under high polarization potentials compared to Ni NPs and also showed greater durability and tolerance to CO poisoning. The in-depth STEM and EELS analysis unambiguously indicated that Ni@CNx catalysts contained a metallic Ni core and a thin carbon shell of 1 to 3 nm. The PPD of APEFC using Ni@CNx as an anode catalyst achieved a record value of 480 mW/cm2 with a Pt/C cathode and 210 mW/cm2 with a MnCo2O4/C cathode. The former represents the highest performance ever reported for a fully nonprecious fuel cell. DFT calculations and TPD measurements suggest that the CNx shell effectively destabilized H on Ni, bringing its binding energy closer to the optimal value for HOR. In addition, the CNx shell enhanced nickel’s resistance to oxidation. Our findings highlight the strategic importance of an N-doped carbon shell for the synthesis of more active and durable Ni-based nonprecious anode catalysts for APEFCs.

Methods

Ni@CNxs were prepared by a facile method using purified nickel acetate and urea as the precursors. Ni@CNxs were characterized by XRD, XPS, Raman, and TPD measurements. The microstructures and chemical compositions were investigated by atomic-scale STEM imaging and EELS spectroscopy (Cornell Nion UltraSTEM). The HOR activity performance of Ni@CNx was evaluated in rotating disk electrode (RDE) in 0.1 M KOH. Fuel cell performance and durability of Ni@CNx anode were performed in MEAs with Pt/C or MnCo2O4/C cathode and QAPPTT ionomer and membrane. DFT calculations were performed using the Vienna Ab Initio Simulation Package (VASP). More experimental and computational details can be found in the .
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