Heyin
Chen
*a,
Agnes-Matilda
Mattsson
a,
Laura
King
a,
Haidong
Liu
a,
Ida
Nielsen
a,
Tove
Ericson
a,
Alexei
Preobrajenski
b,
William R.
Brant
*a and
Maria
Hahlin
*ac
aDepartment of Chemistry –Ångström Laboratory, Uppsala University, Box 538, 751 20 Uppsala, Sweden. E-mail: heyin.chen@kemi.uu.se
bMAX IV Laboratory, Lund University, Box 118, 221 00 Lund, Sweden
cDepartment of Physics and Astronomy, Uppsala University, Box 516, 75120 Uppsala, Sweden
First published on 27th August 2024
Traditionally, Ni-rich-layered oxide cathodes for lithium-ion batteries are produced utilizing N-methyl-2-pyrrolidone (NMP)-processed casting. However, to avoid using the reprotoxic solvent NMP, aqueous processing becomes one of the options. In this study, H2O-processed LiNi0.8Mn0.1Co0.1O2 (NMC811) electrodes have been prepared to compare with the NMP-processed counterparts to investigate the degradation mechanism. The thick cathode–electrolyte interphase (CEI), NiO-like phase formation, and the growth of electrochemically inactive NMC particles after long-term cycling lead to capacity decay. In addition, phosphoric acid (H3PO4) was utilized to lower the pH value during the water-processed electrode preparation, to avoid corrosion of the aluminium current collector. The use of H3PO4 enhanced the capacity retention of NMC811 electrodes, likely owing to the formation of a LiF-rich CEI layer in the initial cycle(s) and the alleviated formation of electrochemically inactive NMC particles. Additionally, reaction inhomogeneity is present in H3PO4-modified electrodes, which is attributed to various Li-ion reinsertion resistances throughout the porous electrode during long-term cycling. Although the performance of the water-processed NMC811 electrode is not reaching the level of NMP-processed electrodes, this study provides key insights into the involved degradation mechanisms and demonstrates a viable pathway for the development of sustainable battery manufacturing processes.
A few solutions have previously been considered, where NMC surface modification is a major strategy, for example, (1) coating with Al2O3, ZrO2, and TiO2 on the particle surface with atomic layer deposition (ALD) technique,12 (2) coating with cobalt boride, polyaniline, and Li3PO4 during the synthesis,13–15 and (3) using phosphoric acid to obtain a phosphate coating on the surface.10,16,17 Compared to expensive ALD coating and time-consuming synthesis coating, in situ coating with phosphoric acid during slurry casting is easy and thus cheap to achieve since it only includes the addition of the acid during the mixing of the NMC materials with slurry binder and H2O. It has also been shown that phosphoric acid can be used as a pH controller to avoid Al current collector corrosion.11,18 This is an important property as the corrosion product Al(OH)4− may react with electrolyte leading to co-solvent, ethylene carbonate, decomposition, and the corrosion product may also increase the charge transfer resistance at the Al/NMC electrode interface, which leads to capacity decay in the initial cycles.19 It is claimed that a phosphate coating can also improve the electrochemical cycling performance by stabilizing the NMC 523 electrode/electrolyte interphase and forming Li3P as a good ionic conductor component in the cathode electrolyte interphase (CEI).10 Also, the addition of H3PO4 acid in the slurry seems to stabilize the electrode/electrolyte interface.11 However, not much work has been done on NMC811 electrodes processed in water, and particularly it is not clear how the H3PO4-modified surface influences the CEI formation. In addition, the structural degradation mechanisms of water-processed electrodes during long-term cycling need to be investigated if it is to be implemented on a larger scale.
In this work, a systematic study was performed on aqueous-processed NMC811 electrodes, specifically the electrochemical performance, CEI layer formation, phase transitions, and charge transfer resistance. Water-processed electrodes (H2ONMC), H3PO4 modified electrodes (HPONMC) containing a small amount of phosphoric acid (0.5 wt% of total electrode material mass), and as a reference the NMP-processed electrodes (NMPNMC) were prepared. Generally, the results show that H2O-processed electrodes exhibit a thicker CEI layer leading to a inhibited H2 → H3 phase transition during long-term cycling, as determined by photoelectron spectroscopy (PES) and operando X-ray diffraction (XRD) measurements, respectively. Compared to the H2ONMC electrode, the HPONMC electrode had an improved cycling performance with a stable charge transfer resistance, which may be due to the reduction of an electrochemically inactive phase forming after extended cycling. Even though H3PO4 modification during electrode preparation cannot fully protect the NMC811 surface from reacting with H2O during water processing, it still inspires the development of a potential coating material/method for a more protective layer.
To obtain chemical composition in the outermost layer of electrodes with comparable depth profiling, P 2p, C 1s, O 1s, and F 1s core level spectra were measured with photon energies 275 eV, 425 eV, 675 eV, and 820 eV, which gives similar kinetic energy of photoelectrons (∼150 eV) and a probing depth of ∼2 nm (probing depth being 3* estimated inelastic mean free path of electrons). The binding energy in all spectra was referenced to an adventitious hydrocarbon peak at 285 eV. For the O 1s and F 1s spectra binding energy calibration, the C 1s spectra were also obtained using a photon energy of 675 eV and 820 eV, respectively. To calibrate P 2p collected with photon energy 275 eV, P 2p and C 1s spectra were collected with a photon energy of 720 eV to be utilized as references. Acquired spectra were curve fitted with the Igor Pro 9 software with a combination of Gaussian and Lorentzian functions, following linear background subtraction. The full-width half-maximum is fixed to 0.2 eV in the Lorentzian function and variable in the Gaussian function with a range of 1–1.6 eV (except for the CC peak in carbon black set to 0.7 eV). For each collected C 1s, O 1s, and F 1s spectrum, the peak intensity was normalized to 1, except for the F 1s spectra measured from the pristine H2ONMC and HPONMC electrodes due to their zero intensity. For P 2p, the spectra collected from the pristine samples were normalized to the same background intensity, while the spectra from the cycled electrodes were normalized to a different background intensity. This adjustment was necessary because these two batches of data were collected from two different endstations at the synchrotron, and no direct comparison of the intensity between these sets of spectra should be made.
XAS measurements were conducted for all electrodes and NiO, LiNiO2, Li2CO3, LiF, and LiOH references using drain current. Ni L-edge, O K-edge, and Li K-edge spectra were measured in total electron yield (TEY, depth information about 5 nm) mode.21,22 In addition, Ni L-edge fluorescence was detected using SDD (Rayspec) for the pristine electrodes. The obtained spectra were normalized by the I0 signal from a clean gold sensor in the beamline, and the background was further corrected to ensure constant pre-edge intensity. The presented Ni L-edge and O K-edge spectra were normalized to a point after the absorption edge.
Quantitative analysis of d-spacing changes of the 003 reflection was obtained from peak fitting using a Voigt function performed in using the Fityk software.24 A linear background was applied to all data sets. For the majority of the data, a single peak was sufficient to fit the data. In instances where asymmetry was observed or where a second peak was identified, a second peak was included in the fitting. An example of the single and double-peak fitting is shown in Fig. S1 (ESI†). The full width at half maximum (FWHM) values of the main peak at the 003 reflection vary from 0.015 Å−1 to around 0.03 Å−1 depending on states of charge. The peak shape, a combination of Gaussian and Lorentzian functions, remains constant during peak fitting. In a double-peak fitting, the shapes of the two peaks were set to be identical. The shifts in fitted peak position can be used to roughly calculate changes in the c-lattice parameter through their corresponding d-spacings.
The differential capacity (dQ dV−1) profiles are illustrated with various cycle numbers of the three types of electrodes in Fig. 1(d–i). The initial cycle shows a similar overpotential as the charge–discharge profile for all three types of electrodes, and negligible polarization can be seen between cycles 2–5 at 0.1C in Fig. 1d–f. During charge, NMC811 particles undergo phase transitions from hexagonal 1 to monoclinic (H1 → M), monoclinic to hexagonal 2 (M → H2), and hexagonal 2 to hexagonal 3 (H2 → H3) phase. In the dQ dV− 1 plots these phase transitions coincide with the distinct peaks at ∼3.75 V, ∼4.0 V, and ∼4.2 V.1,27,28 As can be seen in Fig. 1g, the NMPNMC electrode has a maintained peak intensity at 0.5C for 100 cycles, indicating a good phase transition reversibility and structure stability after extended cycling. In contrast, for the H2ONMC electrodes, dramatic shifts of all the dQ dV−1 peaks and peak intensity decay for the H2–H3 phase transition can be seen during cycling at 0.5C in Fig. 1h. These peak shifts provide evidence of surface polarization due to high resistance which impacts the occurrence of the phase transitions. Many reasons can cause the peak intensity drop, and we propose that structural degradation in the near-surface regions leads to the incomplete phase transition. With the following XAS and XRD measurement results, the above-mentioned suggestions are confirmed to be reasonable. Compared to H2ONMC, HPONMC electrodes exhibit reduced surface polarization, shown in the dQ dV−1 peaks in Fig. 1i, however, it still displayed higher surface polarization than the NMPNMC electrode (Fig. 1g). The intensity drops observed in HPONMC electrodes are less severe compared to those in H2ONMC electrodes. These results indicate that phosphoric acid modification can improve structure reversibility in the near-surface regions of H2O-processed electrodes during battery cycling, although not yet reaching the performance level of NMP-processed electrodes.
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Fig. 3 O 1s spectra collected on NMPNMC (a), H2ONMC (b), and HPONMC (c) electrodes as pristine (top), after 1 cycle (middle) and after 105 cycles (bottom) with photon energy 675 eV. |
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Fig. 4 O 1s spectra measured on NMCNMP, H2ONMC and HPONMC electrodes after 105 cycles with photon energy 1486.7 eV. |
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Fig. 5 P 2p spectra collected on NMPNMC (a), H2ONMC (b), and HPONMC (c) electrodes as pristine (top), after 1 cycle (middle), and after 105 cycles (bottom) with photon energy 275 eV. |
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Fig. 6 F 1s spectra collected on NMPNMC (a), H2ONMC (b), and HPONMC (c) electrodes as pristine (top), after 1 cycle (middle) and after 105 cycles (bottom) with photon energy 820 eV. |
In the soft X-ray C 1s PES spectra CO32− signals can be seen for the pristine H2ONMC and HPONMC electrodes, which most likely originates from reactions of CO2 with the surface.29 This result is in contrast to the pristine NMPNMC electrode, where no such species can be confirmed. It was previously determined in our research that the presence of water facilitates the formation of carboxylate species, and indeed an increase in the relative peak ratio of O–CO to C
O suggests that this also could occur for the H2O-processed electrodes in this study.31 The Na-CMC binder in the pristine H2ONMC and HPONMC show peak intensity corresponding to C–O, C
O, and O–C
O species. The majority of adventitious hydrocarbon species were removed after 1 cycle for both H2ONMC and HPONMC electrodes, as seen from a relatively stronger C
C peak. The relative ratios between other C 1s peaks indicate that both the H2ONMC and HPONMC electrodes are after 1 cycle rather similar to their pristine counterparts. However, upon longer cycling a thicker CEI layer is building up, mainly consisting of C–H, C–O, O–C
O, CO32− containing compounds. Further, more electronegative C moieties were detectable among the electrolyte degradation products, e.g. CFx species, after 105 cycles. In NMPNMC electrodes, negligible changes can be seen between the pristine electrodes and after they were cycled once. After 105 cycles, O–C
O species from electrolyte degradation forms in the CEI layer. Also, CH2–
F2 and CO32− species together gave intensity contributions to the peak at 290 eV binding energy. In summary, more adventitious hydrocarbon and carbonate species accumulated on the pristine H2O-processed electrodes compared to NMP-processed electrodes. After 105 cycles, CO32− species were detected in the CEI layer in all three types of electrodes, and CFx (x ≥ 2) species were also found on the H2ONMC and HPONMC electrode surfaces.
From O 1s spectra in Fig. 3, the peak at lowest binding energy ∼529 eV is assigned to M−O, the structural oxygen in the NMC811 materials. The following peak at ∼531 eV (referred to as surface O) can have a number of origins; both M–OH and CO32− species generally show a peak at ∼531 eV in the O 1s spectra, and our previous research identifies the presence of them on the NMC811 powder surface during storage.31 Thus, M–OH and CO32− species may exist on the pristine electrodes, hence giving intensity contribution in O 1s spectra. Also, R–OLi species are known to show a peak at ∼531 eV in O 1s spectra, which may be generated after electrical cycling.32,33 As shown in Fig. 3, the peak assigned to M–OH, CO32−, and R–OLi species is labeled as surface O. CO and C–O give intensity at ∼532 eV and 533 eV respectively.29,34 After the initial cycle, in the NMPNMC electrode, the peak at ∼534.2 eV is assigned to P–O species, which is contributed by salt decomposition into phosphate compounds. While, after 105 cycles, the peak shifts to slightly higher binder energy (∼534.5 eV), which could be due to the intensity contribution from the LixPOyFz species. In pristine H2ONMC and HPONMC electrodes, the peaks at ∼534 eV are attributed to C–OH species from the Na-CMC binder.35,36 After electrochemical cycling, P–O species may give intensity contribution to the peak at ∼534 eV, together with C–OH species in water-processed electrodes. The peaks at the highest binding energy ∼535 eV are attributed to LixPOyFz, which is assigned to degradation products from the electrolyte. In the pristine H2ONMC and HPONMC electrodes and following 1 cycle, peak ratios of C–O to C
O species in C 1s vary in O 1s spectra, which is due to contribution from the P
O species at ∼533 eV, together with C–O species in O 1s. The presence of phosphorus species is supported by the P 2p spectra, shown in Fig. 5.
With the soft X-ray PES data, signal from structural oxygen (M–O species) is visible in all three types of electrodes, as pristine and after the initial cycle. However, after 105 cycles, as the CEI layer grows, M–O species are not detectable with the soft X-rays in any of the samples. However, with an Al Kα source, M−O contribution to the O 1s spectrum can be seen in the NMPNMC electrode (see Fig. 4). This result implies that a thicker CEI layer was formed in the H2O-processed electrodes than in the NMP-processed electrodes. In the HPONMC electrode, a minor peak intensity corresponding to M−O species is observable, suggesting that M–O buried by CEI remains detectable. This implies that after 105 cycles, the HPONMC electrode exhibits a slightly thinner CEI layer compared to the H2ONMC electrode (see the overlaid spectra and fitted spectra in Fig. S2 in ESI†). The interpretation of the thickness of the CEI, as obtained from the C 1s and O 1s spectra, supports each other, however, a small difference is present. Particularly, the C 1s spectra suggest a slightly thinner CEI, compared to what the O 1s spectra do, exemplified by the clear CC peak for all electrodes after 105 cycles, while at the same time, the M–O peak in the O 1s spectra is barely visible. This phenomenon most likely originates from some carbon black particles not being buried by the binder during electrode preparation. Thus, they were not impacted or covered by the resulting CEI layer on the cycled electrodes.
In P 2p spectra (Fig. 5), peaks at lower binding energy are assigned to phosphate and PO/P–O groups and peaks at higher binding energy are attributed to LixPOyFz and LiPF6 salt residue.29 Pristine HPONMC electrodes show P
O/P–O species on the surface due to the H3PO4 acid modification, while the pristine NMPNMC and H2ONMC electrodes contain a smaller quantity of phosphorus compounds, which is assumed to dissolve into electrolyte while cycling, see Fig. S3 in ESI.† After 1 cycle, H2ONMC and HPONMC electrodes show a relatively higher contribution from LixPOyFz/LiPF6 compared to the NMPNMC electrode. This can be linked to the OH group from Na-CMC binder reacting with LiPF6 salt dissociation product PF5, which is reported by Passerini et al.29 As described in reaction scheme (I), the reaction generates POxFy-like products. In addition to that, PF5 reacts with H2O residue, and the product POF3 further generates LixPOyFz, as described in reaction scheme (II). In contrast, the formation of LixPOyFz species on the surface of the PVDF-based electrode is mainly due to the H2O residue, following the reaction scheme (II).
LiPF6 ↔ LiF + PF5 |
PF5 + R−OH → R−O−PF4 + HF | (Reaction scheme I) |
PF5 + H2O → 2HF + POF3 |
POF3 + ne− + nLi+ → LixPOyFz + LiF | (Reaction scheme II) |
After 105 cycles, major contributions from phosphate can be detected in the NMPNMC electrode, while both H2ONMC and HPONMC electrodes show similar phosphate and LixPOyFz/PF6− quantities. The phosphate-rich CEI layer is reported to stabilize the particle surface structure,37 and lithium phosphate has good ionic conductivity.15 Thus, a phosphate-rich CEI on the NMPNMC compared to the H2O-processed electrodes can be a contributing factor for the better cycling performance of NMPNMC electrodes.
As displayed in Fig. 6, for the pristine NMPNMC electrode, PVDF binder contributes to the peak at ∼688 eV and 689 eV, and no detectable F 1s signal can be observed in pristine H2ONMC and HPONMC electrodes. After the initial cycle, LiF (∼685 eV) and LixPOyFz (∼687 eV) peak intensity can be seen in F 1s spectra,29 which shows the presence of these species in the CEI layer in all three electrode types. Compared to H2ONMC electrodes, HPONMC electrodes have relatively more LiF product at the surface. LiF is formed in both electrodes according to the scheme (II). In addition to that, the larger amounts of LiF observed in the HPONMC could be due to a reaction between HF (side product from LiPF6 degradation reaction with H2O residue and the hydroxyl group) and pre-existing phosphorus species, probably LixH3−xPO4 species, resulting in the extra formation of LiF, according to reaction scheme (III). LiF is considered to give good ionic conduction in the CEI layer, and this result supports the smaller impedance observed for the HPONMC electrodes compared to the H2ONMC electrodes. Further details will be demonstrated in the following EIS results.
Li3−xHxPO4 + HF → Li2−xHx+1PO4 + LiF | (Reaction scheme III) |
The thicker CEI layers after 105 cycles are seen for all electrodes and contain relatively more LixPOyFz compared to salt residues. This ratio increased from NMPNMC to HPO NMC, with the largest ratio for H2ONMC. This could indicate an increased reactivity between the salt and the NMC surface in the same order.
To summarize, from the PES data collected from various pristine and cycled electrodes we can draw the following conclusions: (1) pristine H2O-processed electrodes are prone to accumulate adventitious carbon species on the surface and also have carbonate species on the surface that react with CO2 during storage; (2) for the cycled H2O-processed electrodes, the CEI layer contains LiF, Li2CO3, and LixPOyFz after the initial cycles, and phosphate is gradually increasing during long-term cycling. (3) Compared to NMPNMC electrodes, both H2O-based electrodes have a thicker CEI layer; and (4) HPONMC electrodes have pre-existing phosphorus species on the surface, which react to form relatively more LiF in the CEI layer compared to the H2ONMC.
O K-edge XAS spectra measured for reference chemicals and the electrodes are shown in Fig. 8. The feature at ∼534 eV is attributed to π* orbitals in Li2CO3.22 LiNiO2 and NiO give contributions to the peak at ∼528 eV and 532 eV respectively, as can be seen in Fig. 8(a). In addition, LiNiO2 also has a feature at ∼534 eV from CO32− species, which is due to its air instability and formation of Li2CO3 on the surface during storage.39 Compared to the pristine NMPNMC electrode, H2ONMC, and HPONMC electrodes have relatively higher peak intensity at 532 eV compared to the peak at 528 eV, which indicates that a NiO-like rock-salt phase is formed on the surface of these H2O-processed electrodes.25 As reported by Bichon et al., in the aqueous medium, Li-ions at near-surface regions of NMC materials will leach. Following this, transition metals can fill the lithium site and the reduction of the Ni3+ ions to Ni2+ together with oxygen loss leads to a NiO-like rock-salt phase in this lithium-deficient near-surface region.11,39,40 Interestingly, after the initial cycle, all electrodes in this study have a slightly higher intensity ratio of O–Ni3+ feature to O–Ni2+, labelled with dashed lines in Fig. 8b–d. The proposed explanation is that after the initial discharge, not all the Ni3+ can be fully reduced back to Ni2+, which also matches the capacity loss in the initial discharge. The NMPNMC electrode, on the other hand, shows almost complete reversibility. After 105 cycles, the relative peak intensity ratio between O–Ni3+ to O–Ni2+ decreased also for the NMPNMC electrode, and this is likely due to the NiO-like phase formation in line with previously reported results.28 In the H2ONMC and HPONMC electrodes after 105 cycles, due to the surface sensitivity of TEY mode, the O K-edge spectra mainly show information from the CEI layer rather than the NMC811 active material. Thus, the presence of O–Ni3+ and O–Ni2+ peaks indicates some Ni-ions were trapped in the CEI possibly linked to HF attack.41 Also, from ICP-OES results, transition metal diffusion into electrolyte is identified (see Table S1, ESI†). A substantial amount of Li2CO3 species is produced after long-term cycling, which is confirmed by the peak intensity at ∼534 eV in Fig. 8c and d. This result matches the collected C 1s PES spectra as well as Li K-edge XAS spectra.
Ni L-edge XAS spectra were obtained for pristine NMPNMC, H2ONMC, and HPONMC electrodes, following the initial cycle, and after 105 cycles, as shown in Fig. 9a–c. Fig. 9(d) displays the spectra from the reference compounds NiO and LiNiO2, and the doublet peak near 853 eV and 855 eV labelled with ‘L3 low’ and ‘L3 high’ corresponds to the 2p3/2 → 3d transition under two different photon energies. The ratio of peak intensity of L3 high to L3 low gives qualitative information about the oxidation state of Ni, with a higher value meaning a higher amount of Ni3+.2,22,42 Thus, the L3 high to L3 low peak intensity ratios have been calculated for each spectrum, as shown in Fig. 9e, to investigate the evolution of the oxidation state of Ni at the near-surface region in each sample. As for the pristine electrodes, H2ONMC and HPONMC have a lower oxidation state on Ni compared to NMPNMC, which supports the NiO phase formation in the H2O-processed electrodes. After the initial cycle, the intensity ratio values increase in all three types of electrodes. Thus, the same conclusion can be drawn as from the O K-edge data that some Ni3+ ions were not reduced back to Ni2+ during the initial discharge. After 105 cycles, the peak intensity ratio drops for the NMPNMC electrode, indicating NiO formation during cycling. This data also matches the interpretation of the O K-edge XAS data presented earlier. The Ni L-edge data from H2ONMC and HPONMC electrodes after 105 cycles gives information on the CEI layer rather than the active materials, which also confirms the presence of Ni-ions in the CEI layer.
d-Spacing values for the 003 reflection were determined through peak fitting. In the case of single-peak fitting for the 003 reflection, one d-spacing value will be obtained, while with a double-peak fitting, two d-spacing values were obtained, corresponding to two different phases (see Fig. S1†). As depicted in Fig. 10a and d, a fitting using a single peak (and therefore with a single phase) was sufficient for all states of charge of the NMPNMC electrode. In comparison to the fresh NMPNMC electrode, the aged NMPNMC electrode shows negligible changes to the phase transition. This observation suggests that NMPNMC electrodes exhibit minimal resistance to Li-ions insertion and extraction from the bulk material. Unlike NMPNMC electrodes, a single peak was insufficient for fitting the 003 reflection for H2ONMC and HPONMC electrodes and subsequently a second peak (phase) was included in the fitting, respectively (see Fig. S6 and S7†). In the H2ONMC electrode, the second peak appears at ∼4.3 V, and the d-spacing values for this peak (shown in green in Fig. 10b and e) are fairly invariant. We interpret this phenomenon as some delithiated particles in the electrode experiencing a higher resistance during the H2 → H3 phase transition and becoming electrochemically inactive.
After aging, a more electrochemically inactive phase exists in the H2ONMC electrode compared to the fresh one, as the peak fitting shows in Fig. S4.† It is proposed that the presence of the NiO-like rock-salt phase in the fresh cell leads to the gradual growth of the inactive phase during cycling. In HPONMC electrodes, rather than peak asymmetry, the main reflection became significantly broadened during the H3 → H2 phase transition in discharge (see example in Fig. S7†). Two or more phases existed during discharge from 4.3 V to 4.0 V in the fresh cell (Fig. 10c) or 3.9 V in the aged cell (Fig. 10f) (see the green box in Fig. 10). Further, in both the fresh and aged electrodes, two or more phases exhibit expansion along the c-axis of the unit cell revealing some electrochemical activity, even though the rate of expansion varies. A possible explanation for this is that rather than particles becoming electrochemically inactive, different parts of the electrode are experiencing varying resistance to Li-ions reinsertion and react at different rates during discharge. Instead of referring to a sluggish phase with a lower unit cell change rate, they are distinguished by naming phase 1, phase 2, and phase 3. This difference in reaction kinetics is significant enough to be detected via XRD as shown in Fig. S7.† In the fresh and aged HPONMC electrodes at ∼4.1 V, the peak broadens significantly and cannot be fitted with two phases. This implies that the beam is diffracting from parts of the electrode that are at different states of charge, where some regions (phase 3) are more sluggish than others (see Fig. S7†). d-Spacing values from phase 1 and phase 2 are shown in blue and green color, respectively, in Fig. 10f. This data suggests that HPONMC electrodes experience significant reaction inhomogeneity. However, other techniques are needed to ascertain the spatial distribution of this inhomogeneity. For example, if it exists on a particle level or if it varies as a function of depth in the electrode. Compared to the aged H2ONMC electrode, the resistance in the aged HPONMC electrode is less pronounced since all the phases were electrochemically active, unlike the electrochemically inactive phase formation in the aged H2ONMC electrode.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4ta03592e |
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