Cijie
Liu‡
a,
Dawei
Zhang‡
b,
Wei
Li
*a,
Jamie A.
Trindell
c,
Keith A.
King
c,
Sean R.
Bishop
d,
Joshua D.
Sugar
c,
Anthony H.
McDaniel
c,
Andrew I.
Smith
d,
Perla A.
Salinas
d,
Eric N.
Coker
d,
Arielle L.
Clauser
c,
Murugesan
Velayutham
ef,
Joerg C.
Neuefeind
g,
Jingjing
Yang
b,
Héctor A.
De Santiago
a,
Liang
Ma
a,
Yi
Wang
a,
Qiang
Wang
h,
Wenyuan
Li
i,
Qingsong
Wang
j,
Qingyuan
Li
a,
Hanchen
Tian
a,
Ha Ngoc
Ngan Tran
i,
Xuemei
Li
i,
Brandon
Robinson
i,
Angela M.
Deibel
a,
Gregory
Collins
a,
Nhat Anh
Thieu
a,
Jianli
Hu
i,
Valery V.
Khramtsov
ef,
Jian
Luo
*bk and
Xingbo
Liu
*a
aDepartment of Mechanical and Aerospace Engineering, Benjamin M. Statler College of Engineering and Mineral Resources, West Virginia University, Morgantown, WV 26506, USA. E-mail: wei.li@mail.wvu.edu; xingbo.liu@mail.wvu.edu
bProgram in Materials Science and Engineering, University of California San Diego, La Jolla, CA 92093, USA
cSandia National Laboratories, Livermore, CA 94551, USA
dSandia National Laboratories, Albuquerque, NM 87123, USA
eIn Vivo Multifunctional Magnetic Resonance Center, Robert C. Byrd Health Sciences Center, West Virginia University, Morgantown, WV 26506, USA
fDepartment of Biochemistry and Molecular Medicine, School of Medicine, West Virginia University, Morgantown, WV 26506, USA
gChemical and Engineering Materials Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
hShared Research Facilities, West Virginia University, Morgantown, WV 26506, USA
iDepartment of Chemical and Biomedical Engineering, Benjamin M. Statler College of Engineering and Mineral Resources, West Virginia University, Morgantown, WV 26506, USA
jDepartment of Chemistry, Bavarian Center for Battery Technology (BayBatt), University of Bayreuth, Universitätsstrasse 30, Bayreuth, 95447, Germany
kDepartment of Nano and Chemical Engineering, University of California San Diego, La Jolla, CA 92093, USA. E-mail: jluo@alum.mit.edu
First published on 18th December 2023
Non-stoichiometric perovskite oxides have been studied as a new family of redox oxides for solar thermochemical hydrogen (STCH) production owing to their favourable thermodynamic properties. However, conventional perovskite oxides suffer from limited phase stability and kinetic properties, and poor cyclability. Here, we report a strategy of introducing A-site multi-principal-component mixing to develop a high-entropy perovskite oxide, (La1/6Pr1/6Nd1/6Gd1/6Sr1/6Ba1/6)MnO3 (LPNGSB_Mn), which shows desirable thermodynamic and kinetics properties as well as excellent phase stability and cycling durability. LPNGSB_Mn exhibits enhanced hydrogen production (∼77.5 mmol moloxide−1) compared to (La2/3Sr1/3)MnO3 (∼53.5 mmol moloxide−1) in a short 1 hour redox duration and high STCH and phase stability for 50 cycles. LPNGSB_Mn possesses a moderate enthalpy of reduction (252.51–296.32 kJ (mol O)−1), a high entropy of reduction (126.95–168.85 J (mol O)−1 K−1), and fast surface oxygen exchange kinetics. All A-site cations do not show observable valence changes during the reduction and oxidation processes. This research preliminarily explores the use of one A-site high-entropy perovskite oxide for STCH.
Reduction step:
(1) |
H2O splitting:
AnBO3−δ + δH2O(g) → AnBO3 + δH2(g) | (2) |
The active redox metal oxides that have been investigated for STCH include stoichiometric oxides (e.g., SnO2/SnO13 and ZnO/Zn14) and non-stoichiometric oxides (e.g., ceria and perovskite-type oxide). Stoichiometric oxides usually require high reduction temperatures (≥1873 K) to reduce, and the reduction–oxidation rates are low.15 Additionally, the reduced oxide is in the gas phase, which increases the collection and separation cost. Ceria (CeO2−δ, where δ represents oxygen non-stoichiometry) materials are well-investigated for STCH reactions due to their thermal stability and fast reaction kinetics. However, ceria suffers from high reduction temperatures (1823 K or above), limiting the theoretical hydrogen yield.16–19 Perovskite-type oxide materials (ABO3−δ) are considered a promising candidate for STCH reaction because they have a low standard partial molar reduction enthalpy resulting in high Δδ. Additionally, the Δδ value of perovskite can be tuned to achieve desirable thermodynamic and kinetic properties, which have been widely studied.20–23 For instance, the Δδ value of the perovskite family LaxSr1−xMnyAl1−yO3−δ (0 ≤ x ≤ 1, 0 ≤ y ≤ 1) is tuneable and increases with the increasing of Sr concentration.24 However, the issue of phase instability and poor cycling performance, as well as sintering and slow kinetics in the reduction step, remains a challenge. For instance, La and, Gd dopants in BaFeO3−δ have been investigated in STCH, but they suffer from the problem of phase instability after the thermochemical H2O splitting reaction. Notably, the poor cycling stability of La- and Gd-doped BaFeO3−δ system also limits the potential for development in STCH. Additionally, the time required for one redox cycle is usually longer than 1.5 hours, which is unfavourable for energy utilization. Therefore, searching for materials with desirable phase stability and kinetics during short-time redox cycling reactions is important.
High-entropy ceramics (HECs) include a wide number of materials such as high-entropy oxides, borides, carbides, silicides, sulfides, phosphides, and phosphates.25–28 Specifically, high-entropy perovskite oxides (HEPOs) were reported in 2018,29 and subsequently attracted great interest because of their catalytic, dielectric, ferroelectric, magnetic, thermoelectric, magnetocaloric, & electrocaloric properties, as well as promising applications in solid oxide fuel cells, batteries, and supercapacitors.30–33 Recent studies found high-entropy oxides with favourable kinetics and stability in the cycling redox reaction.34–38 For example, the (FeMgCoNi)O1.2@SiC composite demonstrated a hydrogen yield that surpassed the thermodynamic limits of cutting-edge materials, including spinel ferrites and ceria.39 Also, (FeMgCoNi)O1.2 showed no performance degradation for 10 cycles. Recently, HECs have been further extended to compositionally complex ceramics (CCCs) where maximizing the configurational entropy is not always needed or beneficial.28,40 Notably, a recent report showed that compositionally complex perovskite oxides (CCPOs) with non-equimolar B-site mixing exhibit excellent STCH performance with Co as the redox-active element.41
Herein, we reported a Mn-based HEPO for STCH reaction via A-site mixing with the chemical formula (La1/6Pr1/6Nd1/6Gd1/6Sr1/6Ba1/6Mn)O3, denoted as LPNGSB_Mn for brevity, for STCH reaction with further improved performance (and are Co-free). LPNGSB_Mn possesses excellent phase stability even after 50 cycling reactions. LPNGSB_Mn exhibits a favourable kinetic property (oxygen exchange coefficient), desirable thermodynamic parameters (Δδ, enthalpy, and entropy of reduction), and high H2 production (∼77.5 mmol moloxide−1) within 1 h. The conclusion that Mn is the only redox centre in this material is supported by X-ray photoelectron spectroscopy (XPS) and electron energy loss spectroscopy (EELS) results. Moreover, LPNGSB_Mn shows excellent phase stability and cycling durability even after over 50 long cycles. This work also provides a new pathway for utilizing A-site HEPO in thermochemical applications such as chemical looping and explores the potential of HEPOs for use in two-step seawater splitting. In this study, we explore both kinetic and thermodynamic aspects in a high-entropy system. Additionally, our extended testing over 50 cycles indicates long-term stability and potential for application, thereby enriching the current understanding beyond the state-of-the-art redox oxides in this field.39,42,43
Sample abbreviations | Nominal composition |
---|---|
LS21_Mn | (La2/3Sr1/3)MnO3 |
LPNGSB_Mn | (La1/6Pr1/6Nd1/6Gd1/6Sr1/6Ba1/6)MnO3 |
X-ray diffraction (XRD) patterns revealed that samples exhibited rhombohedral crystal structures (with space group Rc) without any detectable secondary phase (Fig. 1a). Rietveld refinements confirm all compositions are Rc phase by assuming random A site occupation of La, Pr, Nd, Gd, Sr, and Ba (Fig. S1 and S2†). Table S1† displays the refined lattice parameters for samples. In addition, the neutron total scattering conducted at Oak Ridge National Laboratory (ORNL) Spallation Neutron Source (SNS) Nanoscale-Ordered Materials Diffractometer (NOMAD) further confirmed that LS21_Mn has a rhombohedral crystal structure, as shown in Fig. S3.† The fitting results of the NOMAD data are presented in Table S2.† The comparison between the XRD and NOMAD neutron total scattering results shows excellent agreement, which further validates the crystal structure and space group. The crystal structure is shown in Fig. 1b. Additionally, the tolerance factor of LPNGSB_Mn can be calculated by eqn (3).
(3) |
Fig. 1 (a) XRD patterns of LPNGSB_Mn and LS21_Mn. The standard XRD card for La0.65Sr0.35MnO3 with structure is shown for reference. (b) Crystal structure of LPNGSB_Mn. |
The morphologies, microstructure, and elemental distribution of LPNGSB_Mn were characterized using scanning electron microscopy (SEM) in combination with energy-dispersive X-ray (EDX) spectroscopy (Fig. 2). The fresh sample showed irregularly connected spherical particles with an average diameter of approximately 5–15 μm. The EDX mappings showed a homogeneous distribution of elements.
The scanning transmission electron microscopy (STEM) with EDX mapping (Fig. 3) was used to characterize the atomic microstructure and elemental distribution of LPNGSB_Mn, which revealed a uniform distribution of all elements. These results show a homogenous occupancy of A sites between the A site dopants, but that B-sites are occupied by Mn. STEM-EDX quantitative analysis displayed the average composition for all metal percentages as shown in Table S3.†
To assess the redox capability, the LPNGSB_Mn series samples were tested by temperature programmed reduction (TPR).45 Fig. S4† displays that LPNGSB_Mn has a larger Δδ than LS21_Mn. LPNGSB_Mn shows a Δδ value of 0.0822, which is approximately 2.6 times greater than that of LS21_Mn (Δδ = 0.032).
EPR technique was used to study the magnetic properties of perovskite oxides. The formation of oxygen vacancy in LPNGSB_Mn was investigated using EPR spectroscopy. Room temperature X-band EPR spectra were recorded for the powder samples of fresh LPNGSB_Mn and reduced LPNGSB_Mn (thermally reduced at 1350 °C under nitrogen atmosphere). EPR spectra of fresh LPNGSB_Mn and reduced LPNGSB_Mn samples are shown in Fig. S5.† Both fresh LPNGSB_Mn and reduced LPNGSB_Mn samples exhibited a broad and symmetric signal of high-spin Mn4+ (t32ge0g, S = 3/2) located in the cubic symmetry of the perovskite B site.46–48 The broad spectrum is due to isotropic ferromagnetic exchange coupling arises from the hopping of electrons between Mn4+ and nearest neighbour Mn3+ ions in the crystal lattice.48–50 The calculated g value for both spectra is g = 1.98. No EPR signal was observed below 2000 G (data not shown). The linewidth (ΔHpp) values of fresh LPNGSB_Mn and reduced LPNGSB_Mn samples, calculated from the maximum and minimum values of the spectrum, were 704 and 680 G, respectively. As compared to the ΔHpp of fresh LPNGSB_Mn, the ΔHpp value of and reduced LPNGSB_Mn sample was significantly decreased (from 704 G to 680 G). EPR spectroscopy has been used to study the oxygen vacancy defects in the perovskite oxides.47,48,51 Under a high external thermal energy, some oxygen ions deviated from the original sites and oxygen vacancies are generated in perovskite oxides. The increased sites of oxygen vacancies increase the electron concentration inside the crystals. Our EPR study shows that the g (=1.98) value of the reduced LPNGSB_Mn sample is same as the fresh LPNGSB_Mn. It shows that the lattice structure and coordination environment of Mn4+ in LPNGSB_Mn sample is not changed even after heated at 1350 °C under nitrogen atmosphere. The formation of oxygen vacancies results in defect induced free electron spins. EPR studies have shown that the electrons trapped in the formation of oxygen vacancy sites exhibits a sharp signal around g = 2.003–2.004.52,53 In our study, due to the broad EPR spectra that lack any resolved fine structure, the characteristic g-value of oxygen vacancy cannot be extracted from the spectrum. Importantly, the change in ΔHpp is attributed to the changes of magnetic interaction between the Mn4+ and newly formed oxygen vacancies in reduced LPNGSB_Mn sample. The decreased ΔHpp in reduced LPNGSB_Mn sample demonstrates that there is an increased exchange/magnetic interaction between Mn4+ and neighbouring electrons with the free spins induced by the oxygen vacancies. Overall, the EPR study clearly demonstrates that LPNGSB_Mn under external thermal energy and nitrogen atmosphere resulted in oxygen vacancies.
To reveal the redox-active elements in LPNGSB_Mn, in situ electron energy loss spectroscopy (EELS) was conducted to investigate their redox activity by heating LPNGSB_Mn to 700 °C under a vacuum (Fig. S6†). The EELS spectra of Mn, O, La, Pr, Nd, Gd, and Ba are shown in Fig. S6a–g.† For the A-site elements, no cation peak shift was observed, indicating no valence change in the A-site elements.41 For the B-site elements, Mn is the only redox-active element, as evidenced by the shift in the Mn L-edge to lower energies (Fig. S6a†). The XPS analysis of LPNGSB_Mn shows the same trend, with a shift in the peak edge to lower energies, further demonstrating that Mn is the redox-active element (Fig. S6h†). The Mn 2p peak has two split spin–orbit components of 2p3/2 (∼642.3 eV) and 2p1/2 (∼653.5 eV). The differences in the binding energy of split (ΔBE) were 11.2 eV in fresh LPNGSB_Mn and increased to 11.7 eV in reduced LPNGSB_Mn. The results show a shift of the Mn 2p3/2 and Mn 2p1/2 peaks toward lower binding energies, indicating that Mn has been reduced.54 The absence of the satellite peak at 648 eV indicates that Mn2+ does not dominate in this oxide.55 Thus, Mn3+, and Mn4+ are the predominant valence states in this perovskite-type oxide.
The XPS results also confirmed that rare earth elements (La, Pr, Nd, Gd) remained stable without any change in LPNGSB_Mn before and after the reduction process (Fig. S7 and S8†). One observable change, shown in Fig. S8e,† is that the Sr signal increases in intensity after reduction at 1350 °C. This change in Sr signal can be attributed to Sr segregation, which is commonly observed in perovskite oxides like LaSrMnO3 series.56,57
Note that direct water thermolysis catalysed by the samples and an alumina tube at 1100 °C produces a small amount of H2, which is also reported in the literature.58–62 The H2 production from direct water thermolysis was measured at 800–1100 °C (Fig. S9†). Thus, the amount of hydrogen background produced through direct thermolysis was subtracted from the total hydrogen production to obtain the net H2 production from the STCH redox reaction. To evaluate the water-splitting capabilities of LPNGSB_Mn and LS21_Mn in terms of hydrogen production and reversibility, these materials were subjected to consecutive H2O-splitting cycles. Fig. 4a shows the cumulative hydrogen production for both samples under different protocols in terms of different oxidation temperatures and reduction/oxidation durations at different cycles. Fig. 4b presents the corresponding oxygen production under these protocols. The protocols implemented are detailed in Table S4.† For all materials under different protocols, the molar ratio of O2 to H2 produced in the reduction and oxidation step respectively, was approximately 0.5 (Fig. S10 and S11†), indicating that the splitting of H2O is realized by the redox reaction in a stepwise way. As shown in Fig. 4a and Table 2, hydrogen production increases with the number of cycles. Notably, LPNGSB_Mn exhibits the highest H2 production (∼77.5 mmol moloxide−1) at 900 °C in the oxidation step. The H2 production of LPNGSB_Mn is comparable with the reported oxides tested by the same reactor at Sandia National Laboratories, as shown in Table S5.†63,64
Fig. 4 H2 (a) and O2 (b) production for LS21_Mn and LPNGSB_Mn under different protocols and cycles, respectively. The plots of molar H2 production rate versus time for LPNGSB_Mn under protocols P2 and P3 in different cycles (c–f). The plots of molar H2 production rate versus time for LS21_Mn under protocols P2 and P3 in different cycles (g and h). The plots of molar H2 production rate versus time for LPNGSB_Mn under protocols P4 and P5 in different cycles (i and j). Cycling stability of H2 production of LPNGSB_Mn (k) and LS21_Mn (l) under protocol P2. Detailed testing protocols are summarized in Table S4.† Results of (a–j) were obtained in a STCH reactor at Sandia National Laboratories, while results of (k) and (l) were obtained in another homemade reactor. |
Condition | T red/Tox (°C) | t red/tox (min) | Flow rate (sccm) | Cumulative H2 production (mmol moloxide−1) | Steam to hydrogen conversion (%) |
---|---|---|---|---|---|
a In all cases, the cycle numbers are designated as C1 to C4. For example, C1 represents the first cycle. The protocol numbers are designed as P1 to P5 indicating different conditions which are detailed in Table S4. Tred and Tox are the reduction and oxidation temperature, respectively. tred and tox are the reduction and oxidation time, respectively. | |||||
C1-LPNGSB_Mn-P1 | 1350/1100 | 5/20 | 200 | 21.8 | 0.45 |
C2-LPNGSB_Mn-P1 | 1350/1100 | 5/20 | 200 | 26.3 | 0.54 |
C3-LPNGSB_Mn-P1 | 1350/1100 | 5/20 | 200 | 30 | 0.61 |
C4-LPNGSB_Mn-P1 | 1350/1100 | 5/20 | 200 | 29.3 | 0.60 |
C1-LS21_Mn-P1 | 1350/1100 | 5/20 | 200 | 22 | 0.55 |
C2-LS21_Mn-P1 | 1350/1100 | 5/20 | 200 | 26.7 | 0.67 |
C1-LPNGSB_Mn-P2 | 1350/1100 | 30/30 | 200 | 51 | 0.70 |
C2-LPNGSB_Mn-P2 | 1350/1100 | 30/30 | 200 | 57 | 0.78 |
C3-LPNGSB_Mn-P2 | 1350/1100 | 30/30 | 200 | 60 | 0.82 |
C4-LPNGSB_Mn-P2 | 1350/1100 | 30/30 | 200 | 60 | 0.82 |
C1-LS21_Mn-P2 | 1350/1100 | 30/30 | 200 | 32.95 | 0.55 |
C2-LS21_Mn-P2 | 1350/1100 | 30/30 | 200 | 43.35 | 0.71 |
C1-LPNGSB_Mn-P3 | 1350/900 | 30/30 | 200 | 64 | 0.87 |
C2-LPNGSB_Mn-P3 | 1350/900 | 30/30 | 200 | 73 | 1.0 |
C3-LPNGSB_Mn-P3 | 1350/900 | 30/30 | 200 | 76.5 | 1.05 |
C4-LPNGSB_Mn-P3 | 1350/900 | 30/30 | 200 | 77.5 | 1.05 |
C1-LS21_Mn-P3 | 1350/900 | 30/30 | 200 | 47 | 0.78 |
C2-LS21_Mn-P3 | 1350/900 | 30/30 | 200 | 53.5 | 0.89 |
C2-LPNGSB_Mn-P4 | 1350/1100 | 30/30 | 200 | 27.9–51 | — |
C2- LS21_Mn-P4 | 1350/1100 | 30/30 | 200 | 34.15–46.1 | — |
C2-LPNGSB_Mn-P5 | 1350/900 | 30/30 | 200 | 33.6–41.95 | — |
Initially, the hydrogen production of LS21_Mn (∼26.7 mmol moloxide−1) and LPNGSB_Mn (∼26.3 mmol moloxide−1) is similar when both thermally are reduced for 5 min (protocol P1). However, the reduction and oxidation time increases, the hydrogen production of LPNGSB_Mn and LS21_Mn is 57 and 43.35 mmol moloxide−1 under protocol P2, respectively. In a comparison between conditions of protocols P2 and P3, with the reduction temperature fixed at 1350 °C, the oxidation temperatures are set at 1100 and 900 °C, respectively. A lower oxidation temperature of 900 °C is favourable, yielding a hydrogen production of ∼73 mmol moloxide−1 for LPNGSB_Mn and ∼53.5 mmol moloxide−1 for LS21_Mn, respectively, as shown in Fig. 4a. The hydrogen production of LPNGSB_Mn in the 4th cycle at 900 °C (∼77.5 mmol moloxide−1) is higher than 1100 °C (∼60 mmol moloxide−1), suggesting a greater extent of the reaction at 900 °C, indicating a more thermodynamically favourable condition compared to 1100 °C. The oxidation reaction kinetics are favoured at higher temperatures, as shown in the plots of molar hydrogen production rate versus time (Fig. 4c–h). The oxidative water splitting step is an exothermic reaction and thus thermodynamically favoured at a lower temperature. In contrast, the H2 production kinetics at 1100 °C are higher than at 900 °C, as indicated by the higher peak rates at 1100 °C. The detailed values can be found in Table S6.† The favoured thermodynamics at 900 °C likely cause the higher H2 production within 30 min. A similar effect of lower oxidation temperature on the increased H2 production has been reported in La0.6Ca0.4MnO3.65
Fig. 4i and j shows the rate curve for LPNGSB_Mn during high-conversion water-splitting cycles (with a molar ratio of H2O to H2 at 1000:1) at temperatures of 1100 and 900 °C with detailed conditions described in Table S4.† The plots of gas molar production rates versus time for high conversion water-splitting cycles are shown in Fig. S12.† LPNGSB_Mn exhibits similar peak rates in the presence of H2 at 1100 and 900 °C, as shown in Fig. 4i and j. Fig. S13† compares LS21_Mn and LPNGSB_Mn in high-conversion water-splitting cycles, where LPNGSB_Mn shows a higher H2 production peak rate than LS21_Mn. Moreover, hydrogen production can be detected in LPNGSB_Mn at 900 °C under protocol P5, while LS21_Mn shows negligible H2 production under the same conditions. After STCH cycles, the sample of LPNGSB_Mn was kept as the reduced state and characterized by the HAADF-STEM. The atomic-level crystal structure of reduced LPNGSB_Mn remains intact, and the distribution of elements is homogenous (Fig. S14†), indicating its phase stability. The STEM-EDX quantitative analysis of reduced LPNGSB_Mn is shown in Table S7.†
In addition, it delivers similar H2 production under the seawater vapor feeding condition. Therefore, this STCH technology can flexibly function for splitting low-grade water without the reliance on the costly deionized water due to the use of H2O vapor feeding, which is a promising technological complement to proton exchange membrane and anion exchange membrane water electrolysis that need to use deionized water.66–71 Furthermore, the surface oxygen exchange kinetics for a dense LPNGSB_Mn pellet (Fig. S15†) were measured by the electrical conductivity relaxation (ECR) method. The ECR result (Fig. S16†) can be fitted to obtain the surface oxygen exchange coefficient (Ks).72,73 The Ks of LPNGSB_Mn is 7.992 × 10−5 cm s−1.
Table 2 summarizes the STCH production results under different conditions/protocols. To investigate the correlation between H2 production and material properties, we used excess steam to react with a small quantity of perovskite oxide samples to ensure the sufficient solid–gas contact and mass transfer for analysing the thermodynamic limit situation. Therefore, the steam-to-H2 conversion percentages under all conditions are lower than 1.1%.
We investigated the cycling ability of LS21_Mn for 20 cycles and LPNGSB_Mn for 50 cycles. Fig. 4k and l shows the cycling test results. LPNGSB_Mn and LS21_Mn maintained stable hydrogen production, respectively. The cycling stability of LPNGSB_Mn under harsh cycling conditions is comparable to that reported for other STCH oxides.41,63 LS21_Mn exhibits a degradation of 12% after 20 cycles. In contrast, LPNGSB_Mn shows a degradation of 18% after 50 cycles. The gradually decreased hydrogen production may be attributed to the particle coarsening of samples, which may decrease both the heat transfer rate and the oxygen release rate. The morphologies and EDX maps of pristine LPNGSB_Mn and LPNGSB_Mn cycled for 50 cycles are shown in Fig. 2 and S17–S19.† After 50 cycles, LPNGSB_Mn had an average diameter of approximately 10–25 μm and did not show obvious element segregation. Regarding the texture of the samples, there was a considerable difference in the structural variation. The fresh LPNGSB_Mn sample had a rough surface with particle dispersion (Fig. 2), compared to the 50-cycled sample, which had a relatively smoother surface (Fig. S17d†) with some particle aggregation and material sintering. The larger grain-size observed after the 50-cycling experiment could be attributed to the LPNGSB_Mn being exposed to high temperatures (1100–1350 °C) for a longer time. The distribution of different elements was analysed (Fig. 2, S18 and S19†). The elements of La, Pr, Nd, Gd, and Mn were distributed evenly in both the pristine and cycled LPNGSB_Mn, while the elements of Ba and Sr displayed small segregation in the cycled LPNGSB_Mn. This small difference can be attributed to the sample being subjected to high-temperature sintering. Therefore, the negligible element aggregations are consistent with the phase stability observed in the XRD pattern (Fig. S20†). This phenomenon commonly occurs in perovskite oxides containing alkaline earth elements like Sr, which have a significant influence on material activity and stability.57
The pristine and 50-cycled LPNGSB_Mn was characterized by Raman spectroscopy. The Raman spectra are shown in Fig. S21,† and a three-peak model was used to fit the spectra. The fitting results were summarized in Table 3 below:
Sample | Peak 1 (cm−1) | Peak 2 (cm−1) | Peak 3 (cm−1) |
---|---|---|---|
LPNGSB_Mn pristine | 218 | 497 | 620 |
LPNGSB_Mn cycled | 207 | 490 | 613 |
The observed vibrational band close to 600 cm−1 is probably due to Mn–O vibrational modes coupled with the MnO6 octahedral structure, which are associated with the existence of oxygen vacancies nearby.74,75 The small peak shift between two samples could be attributed to the variation in the heavy ion content. The peaks close to 200 cm−1 and 490 cm−1 could be attributed to the A1g mode from La vibration and the Eg mode from oxygen bending vibration, respectively. The peak around 620 cm−1 can be assigned to the B2g mode, representing the in-phase stretching of LPNGSB_Mn.76–79
The structural stability of LPNGSB_Mn was further demonstrated based on the result of Raman.77 Additionally, the red-shift is observed in the Raman spectra of 50-cycled LPNGSB_Mn indicating the increasing defects in the material structure.80 Collectively, the results of XRD, SEM, EDX and Raman spectra indicate LPNGSB_Mn maintained the relatively stable composition, structure and phase.
Two thermodynamic properties, reduction enthalpy and entropy, are key factors that determine the H2 production of STCH materials.81,82 Therefore, we measured the δ over a range of PO2 values and temperatures for LS21_Mn and LPNGSB_Mn through a reported TGA method.83–85Fig. 5a and b show the oxygen non-stoichiometry of LPNGSB_Mn and LS21_Mn, respectively, as a function of temperatures at different oxygen partial pressures PO2.
Fig. 5 Oxygen non-stoichiometry of (a) LPNGSB_Mn and, (b) LS21_Mn as a function of temperatures at different oxygen partial pressures PO2. Arrhenius representation of (c) LPNGSB_Mn and (d) LS21_Mn in 1000/T and ln(PO2) for obtaining reduction enthalpy and entropy by the van't Hoff method at specific δ range from 0.0025–0.04. (e) Standard enthalpy and (f) entropy for LS21_Mn, LPNGSB_Mn, and some redox oxide materials reported in literatures (e.g., CTM55,19 LSMA6446,24 LSC,86 and LSM64 (ref. 87)). The oxygen non-stoichiometry of (a) LPNGSB_Mn measured at 1400 °C was reprinted with permission from ref. 88. Copyright 2023 The Electrochemical Society. |
According to the van't Hoff method,84 the standard entropy change and the standard enthalpy change can be acquired from the correlation with PO2 and temperature as the following equation.83,85,86
ΔG°(T) = −RTlnKeqred | (4) |
(5) |
(6) |
(7) |
An Arrhenius plot of vs. 1000/T (at a specific δ) with linear fitting can be acquired. Fig. 5c and d show the plots for LPNGSB_Mn and LS21_Mn, respectively. The value of and can be obtained from the slope and the intercept of the straight line, respectively. Consequently, the enthalpy and entropy of LS21_Mn and LPNGSB_Mn as a function of oxygen non-stoichiometry are obtained (Fig. 5e and f), respectively and compared with those of some reported redox materials such as La0.8Sr0.2CoO3 (LSC),86 Ca(Mn0.5Ti0.5)O3−δ (CTM55), La0.6Sr0.4MnO3−δ (LSM64),87 La0.6Sr0.4Mn0.4Al0.6O3−δ (LSMA6446).24 LPNGSB_Mn is in a favourable window of and The reduction enthalpy and entropy of reduction are in the range of 252.51–296.32 kJ (mol O)−1 and 126.95–168.85 J (mol O)−1 K−1, respectively.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3ta03554a |
‡ These authors (C. L. and D. Z.) contributed equally to this work. |
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