Yue
Chen‡
abc,
Wenye
Xuan‡
def,
Weijian
Zhang‡
ag,
Mangayarkarasi
Nagarathinam
bc,
Guiying
Zhao
ag,
Jianming
Tao
ah,
Jiaxin
Li
ag,
Long
Zhang
ag,
Yingbin
Lin
*ag,
Yubiao
Niu
i,
Hsin-Yi Tiffany
Chen
*ef,
Svetlana
Menkin
bj,
Dominic S.
Wright
bj,
Clare P.
Grey
bj,
Oleg V.
Kolosov
*bc and
Zhigao
Huang
*ah
aCollege of Physics and Energy, Fujian Normal University, Fujian Provincial Key Laboratory of Quantum Manipulation and New Energy Materials, Fuzhou 350117, China. E-mail: yblin@fjnu.edu.cn; zghuang@fjnu.edu.cn
bThe Faraday Institution, Quad One, Harwell Science and Innovation Campus, Didcot OX11 0RA, UK
cDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK. E-mail: o.kolosov@lancaster.ac.uk
dDepartment of Chemistry, University of Liverpool, Liverpool L69 7ZD, UK
eDepartment of Engineering and System Science, College of Semiconductor Research, National Tsing Hua University, Hsinchu 30013, Taiwan. E-mail: hsinyi.tiffany.chen@gapp.nthu.edu.tw
fDepartment of Materials Science and Engineering, College of Semiconductor Research, National Tsing Hua University, Hsinchu 30013, Taiwan
gFujian Provincial Engineering Technical Research Centre of Solar-Energy Conversion and Stored Energy, Fuzhou 350117, China
hFujian Provincial Collaborative Innovation Centre for Advanced High-Field Superconducting Materials and Engineering, Fuzhou 350117, China
iWe Are Nium Ltd., Research Complex at Harwell (RCaH), Rutherford Appleton Laboratory, Harwell, Didcot OX11 0FA, UK
jYusuf Hamied Department of Chemistry, University of Cambridge, Lensfield Road, Cambridge CB2 1EW, UK
First published on 23rd July 2025
The interplay between solvent co-intercalation, solid–electrolyte interface (SEI) formation, and gas evolution at the graphite anode–electrolyte interface plays a critical role in battery performance; yet, it remains poorly understood at the nanoscale. In this study, we introduce ultrasound-based operando atomic force microscopy (AFM), which breaks the spatial-resolution limitation of ultrasound-based techniques, to visualize the dynamics of solvent co-intercalation, SEI formation, and subsurface gas evolution in graphite anodes for lithium-ion batteries. Remarkably, we observe that gas evolution leads to the formation of “subsurface molecular bubbles”—gaseous pockets trapped between graphite layers—that compromise interfacial stability during battery formation cycles. AFM and density functional theory calculation results revealed that these subsurface molecular bubbles are primarily induced by the co-intercalation and decomposition of Li+(EC)4 solvation complexes. We also found that the solvent co-intercalation and interlayer decomposition effects can be fully suppressed by incorporating a low-permittivity, non-solvating diluent solvent (fluoride benzene) through optimizing the de-solvation energy and the interfacial molecular architectures. By applying this optimized electrolyte in both graphite/Li half-cells and lithium cobalt oxide (LCO)/graphite full-cells, we achieve stable cycling with negligible molecular bubble formation, compact SEI growth, and high coulombic efficiency (>93%) during high-rate (0.5C) battery formation.
Broader contextThe drive for cost-effective lithium-ion battery (LIB) production has intensified efforts to shorten formation cycles; yet, accelerated protocols often degrade electrode–electrolyte interfaces, impairing performance. While solid–electrolyte interphase (SEI) formation is well-studied, atomic-scale interfacial dynamics during early cycling remain poorly understood, hindering rational process optimization. Here, operando atomic force microscopy with near-field ultrasonic excitation uncovers hidden subsurface molecular bubbles in graphite anodes, formed by trapped decomposition gases between graphite carbon layers during Li+(EC)4 co-intercalation. These bubbles mechanically destabilize the SEI, increasing irreversible capacity losses. Crucially, we demonstrate that non-solvating diluent solvents suppress bubble formation by tuning solvation structures and de-solvation energetics, enabling stable full-cell operation under rapid formation. By linking molecular-scale interface evolution to macroscopic performance, this work provides both fundamental insights into a previously overlooked degradation pathway and actionable strategies for designing efficient formation protocols—critical advances toward scalable, sustainable energy storage systems. |
The formation of the SEI and gas evolution in graphite anodes are closely interrelated interfacial phenomena. The SEI is a result of electrolyte decomposition, which forms a passivating film that separates the reactive electrode from the electrolyte.5 Gas evolution, on the other hand, is often associated with the decomposition of the electrolyte and the subsequent reactions occurring at the graphite–electrolyte interface.3,6 Interestingly, the SEI formation often involves the generation of gases (carbon dioxide and hydrocarbons7–9), and these gases, in turn, can affect the formation and stability of the SEI, causing uneven ion transportation at interfaces3 and ultimately leading to diminished shelf life and battery lifetime. So far, various measures, such as electrolyte additives, surface modification, and electrode engineering, are being explored to enhance the stability of the SEI and mitigate gas evolution in graphite anodes.6,10,11 However, when it comes to interfacial structural degradation, gas evolution on the electrode–electrolyte interface at the nanoscale is often overlooked.12 For example, the lost initial coulombic efficiency (ICE) of the graphite anode is often attributed to the SEI formation, but much less attention has been paid to anode structural damage due to gas evolution on the graphite–electrolyte interface.
It is intuitively reasonable to assume that the gases generated at the edge planes of graphite can diffuse into both the graphite interlayers and liquid electrolyte. The gas released into the electrolyte can be sandwiched in hydration layers in the graphite–liquid interface13,14 or can form macroscale bubbles inside the battery pouches, which has been studied extensively by chromatographic mass spectrometry,15 X-ray tomography,16 neutron radiography17 and ultrasonic non-destructive testing.18,19 In contrast, the gases that diffuse into (or are generated inside) the graphite interlayers may be trapped inside the solid lattice20 and may damage the graphitic lattice. The trapped gas is rarely explored and its effects are far from being understood due to the lack of nanoscale interfacial characterization techniques. Although traditional in-situ/operando electrochemical atomic force microscopy (EC-AFM) has shown promising potential to reveal the nanoscale morphological interfacial structure and property evolution,11,21 it still lacks subsurface characterization capability that can probe the trapped gas. For example, the nano-bumps observed on the carbon anode surface were previously interpreted as the nanoblisters22 filled by co-intercalated liquid solvent between the carbon layers, but it was unclear the whether there are gas products inside the bumps. Another example is oxygen redox in the cathode lattice,23 which has raised more and more research interest; yet, it is still challenging to detect the trapped gas molecules experimentally.24–26 The large difference in the acoustic impedance of gas vs. liquid and solid phases suggests deploying ultrasound-based techniques to study the buried gas evolution behaviour on battery interfaces.
Thanks to the non-invasive and non-destructive characteristics of ultrasound, ultrasound-based techniques enable in situ/operando monitoring of gas evolution in the internal structures of a battery.27–29 These ultrasound-based techniques exhibit high sensitivity to changes in the physical and chemical properties of materials inside the battery package, allowing the detection of small variations and transient gas evolution behaviour, as well as the identification of potential issues or abnormalities within the battery. However, the above-mentioned ultrasound-based characterization techniques, such as the ultrasound-based 2D imaging method,27 merely allow the millimetre-scale localization of gas evolution within the pouch cell.28 This is because the spatial-resolution (104–6 nm) of the ultrasound-based technique is limited by the wavelength of ultrasound in the sample. To study the nanoscale sized graphite–electrolyte interfaces during gas evolution and to facilitate the comprehensive investigation of the origins of macroscale gas evolution processes, it is necessary to bridge the gap between these two by a non-invasive technology that cannot be provided by standard ultrasound techniques. Electrochemical ultrasonic force microscopy30 (EC-UFM) uses ultrasound as a tool to probe local nanomechanical properties via the highly localized AFM tip contact, achieving resolution dictated by the tip size, not the sound waves. Therefore, EC-UFM is a powerful tool to study the buried gas evolution behaviour, in situ and operando, with nanoscale resolution.31,32
In this work, we introduced a novel ultrasound-based operando atomic force microscopy technique (Notes S1 and S2, ESI†) to study the complex interrelations of SEI formation and gas evolution on the graphite–electrolyte interface at the nanoscale. This directly imaged microscopic subsurface “molecular bubbles” trapped inside graphene interlayers, revealing the previously largely ignored factor of interfacial structural degradation during battery formation. We find that it is solvent co-intercalation and decomposition between the carbon interlayers that are the main causes of subsurface molecular bubble formation. To complement UFM observations, density functional theory (DFT) calculations predict that Li+(EC)4 is the most likely solvation complex that participates in both co-intercalation and decomposition. To inhibit this interfacial degradation, we tune the electrolyte component by adjusting the dipole–dipole interactions using a low-dielectric constant diluent and then thoroughly investigate in-depth intermolecular interactions and interfacial electrolyte structures of our optimized electrolytes using molecular dynamics (MD) simulation and force distance spectroscopy. The optimized electrolyte enables fundamental suppression of the formation of subsurface molecular bubbles and the SEI, with the intact graphite–electrolyte interface improving the cycle stability and coulombic efficiency of battery cells under an elevated current density (0.5C) during the battery formation process.
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Fig. 1 Macroscale and nanoscale interfacial structural degradation of the graphite anode during the initial formation in 1 M LiPF6 in EC![]() ![]() ![]() ![]() ![]() ![]() ![]() |
Operando EC-AFM (Fig. 1c) was used to study the nanoscale “invisible” interfacial degradation processes on the graphite anode surface further. As shown in Fig. 1d, the evolution of the surface morphology of the basal planes on a graphite particle surface is observed by EC-AFM at open circuit potential (OCP) and different charging voltages (No. 1–4). Initially (at No. 1 OCP), the basal planes of the graphite particle surface are smooth and clean (as confirmed by the SEM image in Fig. S2b, ESI†) due to the atomic flat characteristics of the carbon (001) plane. Surprisingly, we observed the nucleation and growth of multiple “nano-bumps” during galvanostatic charging (see Video S2, ESI†). The first nano-bump appears on the flat graphite surface at voltage region No. 1, after which the size of the nano-bump increases with the lithium-ion intercalating into the graphite. At the end of the charge, in addition to the nano-bumps formed on the anode surface, we observed dispersed SEI nanoparticles covering the graphite surface (see the AFM image at voltage region No. 4 in Fig. S2c and S2d, ESI†). These nano-bumps are a result of local delamination (as outlined in Fig. 1e), similar to the previously reported gas bubbles or liquid blisters trapped between the layers of 2D materials.34,35Fig. 1f shows the statistical value of the maximum height vs. reduced radius ratio (hmax/R) of the nano-bumps for different nano-bump shapes. The aspect ratio (hmax/R) of the nano-bumps is related to the total adhesion energies γ by36
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Fig. 2 Nanoscale SEI formation and delamination observed by operando EC-AFM and in situ nanomechanical mapping via electrochemical ultrasonic force microscopy (EC-UFM). (a) Schematic diagram of electrochemical AFM combined with ultrasonic wave excitation and the graphite atomic steps consisting of four overlapped carbon layers. (b) The cyclic voltammetry (CV) curve of the AFM EC-cell during the first lithiation in 1 M LiPF6 in EC![]() ![]() ![]() ![]() |
Fig. 2b is the 1st CV in 1 M LiPF6 in EC:
DEC = (1
:
1 vol%) electrolyte; the voltage range can be divided into three different regions according to the different electrochemical processes that occur on the graphite surface. In region I (OCP → ∼2.25 V), the cathodic current stays constant at <1 μA (Fig. S4a, ESI†), indicating that the electrode surface is located within the thermodynamically stable voltage window. When entering the voltage region II, the typical surface-topography image recorded between 2.27 and 2.09 V can be found in Fig. 2c, in which a few scattered SEI nanoparticles (white spots) start to appear on the graphite basal plane. With the voltage decreasing to about 1.35 V, the cathodic current increases by three times. Meanwhile, more irregular nanoparticles that may be attributed to LiF start to form on the graphite basal plane2 (Fig. 1c, No. 3). However, the initially monitored carbon atomic step height remains constant at around 1.01 nm (Fig. S3, ESI†), indicating that intercalation has not yet occurred in this voltage region (2.25–1.35 V). Interestingly, significant topographical changes do happen when the electrode voltage reaches voltage region III (0.80–0.65 V), in which many dense nanoparticles fully cover the electrode surface and the observed carbon step height increases to about 1.55 nm (Fig. S3, ESI†). Moreover, the first nano-bump formed in the measured area (Fig. 1c, No. 4) was also observed at this voltage region. Upon subsequent measurements (Fig. 2c, No. 5 and No. 6), SEI nanoparticles with larger size and featuring more nano-bumps continued to form on the electrode surface until the electrode current changed from cathodic to anodic. However, the surface morphology and nano-bump size stay relatively unchanged from the anodic scan to the end of the CV cycle (Fig. 2c, No. 7–9), indicating that nano-bump formation is concurrent with SEI formation and lithium intercalation.
We further introduced UFM to explore the nature of subsurface substance inside the nano-bumps. In UFM, high frequency ultrasonic excitation (∼4 MHz) with an amplitude of a few angstroms modulated at a few kHz frequency is applied from underneath the sample. The resulting cantilever deflection at modulation frequency (UFM signal) provides a measure of local mechanical properties of the sample for a wide range of elastic stiffness levels from crystalline materials to porous structures and polymers, as well as an indication of obstacles to the ultrasonic vibration propagation under the sample, such as gas or liquid bubbles. Generally, brighter UFM contrast corresponds to stiffer materials and the absence of subsurface delamination.41,42 The UFM image is obtained by nano-tip scanning across the sample surface (Note S2, ESI†) and can be obtained simultaneously with topography as shown in Fig. 2d–i. Fig. 2d shows the topography and UFM image of carbon steps before the CV cycles, the native subsurface dislocations43 and a native pore, buried underneath the top carbon layer, which appear in the UFM image as dark lines and circles, respectively. Importantly, it is also worth noting that this native pore region appears as a slightly dented surface (concave topography) as shown in 3D topography (Fig. S4(b) (ESI†)). This is significantly different from the nano-bumps generated during the electrolyte decomposition, which shows a convex topography as shown in Fig. S4(c) (ESI†). As sketched in Fig. 2e, the pore (or gas bubble) is an obstacle to ultrasonic waves, “blocking” the ultrasonic excitation coming from the substrate and therefore they appear the darkest UFM contrast compared with the SEI and graphite substrate. To study the subsurface bubbles buried under the SEI, the top SEI layer was scratched by the AFM tip before each UFM measurement (Fig. S5, ESI†). Fig. 2f and h show the UFM measurements of the carbon step after the 1st and 2nd CV cycles (see Fig. S6 (ESI†) for the DMT modulus at the same scan area). In Fig. 2f, the nano-bump (in white dashed circles) presents a significantly decreased ultrasonic response in the UFM image (α region in the red box). This indicates that the space underneath these nano-bumps has similar ultrasonic permittivity compared with the pore structure, confirming that it is a gas-filled space that has a large damping effect on the ultrasound vibration. Therefore, UFM confirms that these nano-bumps are subsurface bubbles, rather than blisters filled with liquid electrolyte. The reason is the drastic difference of acoustic impedance (product of density and sound velocity) between the solid graphite (∼3 × 106 Pa s m−1) and gas (∼4 × 102 Pa s m−1), but a smaller difference with the impedance of liquids (∼1.5 × 106 Pa s m−1). It is also worth noting that the β region (at the edge of carbon steps) also shows local delamination with an increased height (Fig. 2f) but exhibits a more inhomogeneous ultrasonic response compared with the α region. This indicates that the β region may be a local delamination region filled by the liquid electrolyte and gases simultaneously.
The force–distance curves of the bubble region with vertical force modulation44 and ultrasonic force modulation are shown in Fig. S7 and S8 (ESI†), in which one can find that the UFM response at the graphite region is about one order of magnitude larger than the UFM response at the bubble region during the indentation. Moreover, as shown in Fig. 2j, by numerical fitting of the vertical force-indentation curves during the tip indentation into the bubble described using a non-linear plate model45 (Fig. S9 and Note S4, ESI†), we conclude that the top of this bubble consists of about 3 carbon layers, as illustrated in Fig. 2g. After the 2nd lithiation/de-lithiation cycle, the sizes of bubbles trapped inside the carbon interlayers have barely increased, while more round-shape “nano-islands” fully covering the graphite surface appear, preferentially accumulated on the step edges (Fig. 2h). These nano-islands have smaller ultrasonic responses compared with graphite but are larger than subsurface bubbles (Fig. S10, ESI†). Ultrasonic force spectroscopy (UFS) measurements performed on the bubble, nano-island and graphite substrate are shown in Fig. 2k. Under an ultrasonic excitation amplitude of 2.50 nm, the “nano-island” region exhibits a UFS response of about ∼1.08 nm, which is larger than that in the bubble areas (∼0.35 nm), but smaller than the graphite substrate (∼1.60 nm). The mechanical modulus of nano-islands determined by UFS is therefore lower than that for graphite and is around ∼108–109 Pa according to numerical simulation results (Fig. S11, ESI†) and close to the values of reported inorganic SEI components.11,21,46 Therefore, as sketched in Fig. 2i, we attribute these nano-islands to stiff inorganic SEIs that seal the entrances of solvent co-intercalation, resulting in the rumination of subsurface bubble growth.
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Fig. 3 The initial stage of lithium/solvent co-intercalation and SEI formation revealed by UFM. (a) Surface topography of the graphite anode under the different polarization voltages. (b) Cross-section and histogram of the step height of carbon layers during the different polarization voltages. (c) Raman spectra of the graphite surface at each polarization voltage. (d) Zoom-in ultrasonic mapping on the few-layer graphite surface at a polarization voltage of 1.0 V. (e) The 1st CV curve of a few-layer carbon step anode cycled in NaPF6 EC![]() ![]() ![]() ![]() |
The solvent co-intercalation was further revealed via UFM, as shown in Fig. 3d. The UFM image of the triple-layer graphene shows three different levels of contrast in the nanomechanical mapping via ultrasonic response. Compared with the UFM image before the solvent co-intercalation (Fig. S12, ESI†), we find an “electrolyte-immersed like” region near the carbon step edges (as denoted by the white dashed line in Fig. 3d). The ultrasound response inside the dashed-line area (Fig. 3d) is larger than the SEI seeds but smaller than the graphite substrate. UFS with different excitation amplitudes were recorded at the typical graphite substrate region, electrolyte-immersed region and one of the carbon step edges at the points marked as f, g and h, respectively, in Fig. 3d. The UFS results are presented in Fig. S13 (ESI†). UFS in the electrolyte-immersed region indicates lower stiffness. This region can be attributed to the solvent co-intercalated GIC, which is softer than the original graphite due to the insertion of solvent molecules between carbon layers. Moreover, UFS at the carbon step edge shows a negligible signal, confirming that the subsurface SEI/gas accumulated at the carbon edge forms a softer and lower acoustic permittivity region compared with GIC. In summary, the solvent co-intercalation and decomposition were observed to occur at the very end of the graphite edge during the initial stage of SEI/bubble formation (at ∼1 V vs. Li+/Li), which are the preconditions of subsurface molecular bubble formation.
Considering that only about 30 ppm water in battery electrolytes, one possible gas evolution reaction could be the two electron reduction of the co-intercalated EC solvent molecules,2 which generate lithium ethylene dicarbonate (LEDC) and C2H2 gas at the carbon step edges. We performed a reference experiment to confirm the correlation between the co-intercalation and subsurface molecular bubble, shown in Fig. 3e–k, in which we replaced the cation Li+ with Na+ (1 M NaPF6 in EC:
DEC = 1
:
1 vol%) and evaluated the voltage-dependent electrochemical processes that occurred on a triple-layer carbon step (see Video S3 (ESI†) for the operando AFM observation) presented in Fig. 3e is the 1st CV curve during the sodiation. Compared to the CV curve in Fig. 2c for lithium electrolyte, the CV curve in Fig. 3e shows only a reduction peak corresponding to the decomposition of the electrolyte, with no oxidation peak found during the anodic scan, indicating that the reversible sodium/solvent intercalation is not present in this system. The SEI related reduction peak almost disappeared during the second cycle (Fig. S14, ESI†), suggesting that the electrolyte decomposition mainly occur on the anode surface during the first CV cycle. The surface topography images in Fig. 3 panels (f)–(k) revealed that the onset of SEI formation occurs at around 1.1 V, while the carbon atomic step height does not change, step edge curls do not appear, whereas SEI accumulation at the carbon atomic step was observed (Fig. S15 and S16, ESI†). To summarise, if there is no cation/solvent co-intercalation, even when the electrode surface is polarized beyond the electrochemical stability window of the electrolyte, the subsurface “molecular bubbles” cannot be generated.
First of all, we tuned the ratio of Li+(EC)4, Li+(EC)3(DEC)1 and Li+(EC)2(DEC)2 by varying the EC:
DEC ratios in 1 M LiPF6 in EC/DEC electrolytes; FTIR spectroscopy was then performed as shown in Fig. 4a and b (full spectra can be found in Fig. S17, ESI†) to confirm the ratio of these solvation complexes. In the C–O band region of DEC (Fig. 4a), we observed a non-negligible proportion of a solvated C–O band (∼1302 cm−1) of DEC, confirming that the DEC molecules participate in the solvation with Li+.48 With the increase of the EC ratio, the peak intensity of solvated DEC decreased from about 37.8% to 23.8%, indicating a decrease of Li+(EC)3(DEC)1 and Li+(EC)2(DEC)2 in the electrolyte. By contrast, the C–O peak intensity of the solvated EC was slightly enhanced (Fig. 4b), indicating a much stronger and more stable Li+–EC coordination interaction compared with Li+–DEC. With the increasing EC ratio from EC
:
DEC = 4
:
6 to EC
:
DEC = 7
:
3, the FTIR peak intensity of solvated-EC vs. solvated-DEC increased by about 64%, confirming the abundance of the Li+(EC)4 solvation complex in the electrolyte, with a high EC ratio. In this high-Li+(EC)4 content electrolyte, we observed more profound graphite surface delamination by operando AFM (Fig. S18, ESI†), supporting the proposition that the higher proportion of Li+(EC)4 in the electrolyte may cause more solvent co-intercalation-induced interfacial degradation.
Importantly, we also noticed that there is an evident blueshift of the C–O peak of solvated DEC (∼1303 cm−1), which can be attributed to the enhanced dipole–dipole interaction of solvated DEC with free EC molecules.49 These dipole–dipole interactions were also observed in the EC/DEC-mixed solvent without the lithium salt (Fig. S19, ESI†). It has been reported that dipole–dipole interactions between the free-solvents and solvated solvents play a significant role in battery interfacial chemistry.49,50 Given that the polarizing effect of Li+ on the EC/DEC molecules can further enhance these dipole–dipole interactions between free-solvent and Li+(EC)x(DEC)y and affect their electrochemical behaviours,51 we considered these interactions to evaluate the adsorption energy, chemical stability and de-solvation energy of Li+(EC)x(DEC)y using DFT calculations. As shown in Fig. 4c, we constructed the models with the Li-solvation complexes, Li+(EC)4, Li+(EC)3(DEC)1 and Li+(EC)2(DEC)2, absorbing on the graphite edge plane to evaluate their adsorption and de-solvation energies. The intermolecular interactions between the free solvents and lithium–solvation complexes were treated by an implicit model by tuning the dielectric constant of the simulation system. The dielectric constants were swept from 10 to 100 according to the changes of EC:
DEC ratios52 in the electrolytes. As shown in Fig. 4d, in the solvent environment with various EC
:
DEC ratios, Li+(EC)4 always shows the lowest energy of adsorption onto the graphite surface, but the highest de-solvation energy. This indicates that for Li+(EC)4 it is energetically favourable to adsorb on the graphite edge planes and then co-intercalate into the graphite lattice without the de-solvation process. By contrast, Li+(EC)3(DEC)1 and Li+(EC)2(DEC)2 exhibit relatively high adsorption energies on the graphite surface, indicating that they are statistically distributed further away from the graphite electrode surface. However, once they approach the graphite surface, they tend to desolvate before entering the graphite lattice without solvent co-intercalation. This further suggests that Li+(EC)4 is the culprit for the initial solvent co-intercalation and graphite delamination, confirming the AFM observations in Fig. S18 (ESI†).
According to the DFT calculations in Fig. 4d, it can be noted that modifying the dielectric environment will allow control over the de-solvation processes of Li+(EC)x(DEC)y. It has also been reported that the de-solvation energy of lithium complexes can be tailored using weakly/non-solvating diluents, which has been employed as a promising strategy to inhibit solvent co-intercalation into graphite, as well as to enhance graphite–electrolyte interfacial stability.53,54 Hence, as a proof of concept, weakly-solvating (1,4 dioxane, DX) and non-solvating solvents (fluorobenzene, FB) with dielectric constants of about 2.25 and 5.42, respectively, were chosen as the diluents to test the ability to suppress the Li+(EC)4 co-intercalation. Fig. 4e shows focused analysis of the lowest unoccupied molecular orbital (LUMO) and highest occupied molecular orbital (HOMO) of Li+(EC4) with additional consideration of the intermolecular interactions from the free solvents. A DX and a FB were attached to Li+(EC)4 to represent the intermolecular interaction of free solvents in the electrolytes with DX and FB diluents. As shown in Fig. 4e, the LUMO orbital remains in one of the solvated EC molecular orbitals, and the additional DX or FB molecules can elevate the LUMO energy level of Li+(EC)455 by about 0.28 eV and 0.14 eV, respectively. Moreover, the higher the LUMO orbital energy of the solvated EC is, the weaker the intermolecular interactions between the solvated EC and the lithium ion.56 This indicates that DX and FB have both weakened the intermolecular interaction between EC and Li+ inside Li+(EC)4, which can reduce its de-solvation energy and facilitate the pure lithium intercalation into the graphite anode. Additionally, this aside, the HOMO orbital fully transfers to the additive DX/FB molecules in Li+(EC)4 + DX (−8.61 eV) and Li+(EC)4 + FB (−9.14 eV), and the HOMO levels are still sufficiently low to resist oxidation reactions on the cathode surface.
Apart from the “passivation” and “dragging” effects of FB molecules toward the Li+(EC)4 complex, we also observed the preferential adsorption of FB molecules on the graphite surface. As shown in Fig. 5d and e, interfacial molecular structures near the graphite surface in the electrolytes with and without FB diluent were measured by AFM-based force–distance spectroscopy57 (Note S5 and Fig. S23, ESI†). In the conventional electrolyte without FB diluent (Fig. 5d), we observed the adhesive force region (at around 0.31–1.88 nm) as a result of the competitive effects of solvation force and Derjaguin–Landau–Verwey–Overbeek (DLVO) force,58,59 followed by a repulsive force region at the inner electrical double layer (EDL) due to the confined effect of the tip and sample surface.57,60 However, the adhesive force region disappeared in the electrolyte with FB diluent (Fig. 5e). After adding FB, the disappearance of the adhesive force region is due to the change in the specific adsorption of ions/molecules on the graphite surface, which modified interfacial dielectric permittivity. This unambiguously points to the localized preferential adsorption and accumulation of low-dielectric-constant FB molecules on the graphite surface; therefore, the anode–electrolyte interfacial compatibility can be greatly affected by this disproportionate distribution of solvent near the electrode surface.61 The preferential accumulation of FB on the graphite–electrolyte interface was also confirmed by DFT calculations (Fig. 5f), in which we found that FB has a lower adsorption energy of −0.48 eV on the graphite surface compared to EC (−0.4 eV). The preferential accumulation of a low-dielectric FB and DEC molecular layer may act as a protective molecular layer preventing solvent co-intercalation and decomposition.
Additionally, the preferential adsorption of FB on the graphite–electrolyte surface may result in the formation of an SEI layer with stable metallic-fluorine species.62,63 This is because that the FB diluent enhanced Li+–PF6− interaction, which facilitates the PF6− to enter the first solvation shell (Fig. 5c) and help to form an anion-derived SEI layer.64–66 The anion-derived SEI with an inorganic–fluoride rich species was confirmed by the X-ray photoelectron spectroscopy (XPS) milling spectra in Fig. 5g and h. As shown in the figures, with the increase of milling depth, the F 1s peak intensity at around 685.5 eV (attributed to LiF67) decreases on the graphite surface cycled in FB-free electrolyte (Fig. 5g) but increases on the graphite surface cycled in electrolyte with FB additive (Fig. 5h).
According to the comprehensive characterization, we summarized the key understanding of solvent co-intercalation, subsurface gas evolution and SEI formation behaviours on the graphite–electrolyte interface in the electrolyte with and without the FB additive as shown in Fig. 5i and j. As sketched in the figures, the FB molecules preferentially adsorb on the graphite surface, participating in reducing the de-solvation energy of Li+, which effectively inhibits the Li+(EC)4 co-intercalation and decomposition within the graphite interlayers. As a result, the subsurface molecular bubbles or other types of micro-structural damage disappeared in the graphite anode matching with the optimized FB electrolyte. This optimized FB-contained electrolyte has special interfacial molecular structures that can also facilitate the formation of a stable inorganic-rich SEI layer. Benefiting from the reduced lithium de-solvation energy and optimized interfacial chemistry, the formation charge/discharge curves of the graphite/LCO cells using EC/DEC-based electrolyte with FB diluent greatly exceeds that of cells without FB diluent as shown in Fig. 5k. At 0.05C formation, the solvent co-intercalation voltage occurring at around 3.5–3.8 V disappeared after adding FB diluent. Moreover, the fluctuations in the formation charge/discharge curves are also smoothed after adding FB diluent at 0.5C formation, suggesting that time and energy-consuming formation processes can be avoided in the optimized electrolyte. More importantly, we fabricated the graphite/LCO pouch cell (4 Ah) to evaluate the capability of FB additives to accelerate the formation process of high mass loading electrodes (Fig. S24, ESI†). Although the coulombic efficiencies of these pouch cells are not excellent due to the high electrode mass loading (about 19.4 mg cm−2 for the cathode and 10.1 mg cm−2 for the anode (single-side)), it is evident that the pouch cell with the FB additive after formation at a large current density (0.5C) shows even better cycle capacity retention compared with the cell using a small formation rate (0.2C) in the electrolyte without the FB additive. This holds significant promise for reducing battery formation time while preserving a robust and high-quality SEI surface passivation layer, thereby lowering the overall costs of secondary lithium/sodium-ion battery fabrication.
Focusing on solvent co-intercalation and decomposition, we combined implicit and explicit models to study the weak interactions between the free solvent and the Li+(EC)4 solvation complex using DFT calculations. Our DFT calculations, by taking into account the intermolecular interactions of free solvent outside the primary solvation shell in EC/DEC electrolytes, suggest that the specific complex involved in co-intercalation is Li+(EC)4, possessing high de-solvation energy and low adsorption energy on the graphite edge plane. Leveraging the understanding of interfacial degradation in conventional EC/DEC electrolytes, FB diluent was introduced to reduce the cation–solvent (ion–dipole) interaction of Li+(EC)4, enabling pure cation intercalation and enhancing chemical stability. The graphite electrode surface lithiation in the optimized electrolyte is smooth and clean, without interfacial structural degradation, facilitating enhanced cycle stability and formation current density of LCO/Graphite full cells.
Overall, our ultrasonic-based EC-AFM nanoscale characterization studies aim to uncover the underlying/root causes for the formation of gases within the carbon layers – ‘the hidden subsurface bubbles’ clearly indicate that the formation of nano-bumps/delamination and the subsequent inaccessible lithium storage site contribute to the initial capacity loss in addition to SEI layer formation. This phenomenon not only enhances our understanding of the interfacial degradation mechanism in Li ion batteries, but also holds promise for translation to other batteries. Although substantial research has been carried out to unravel the formation, storage and cycling degradation mechanism through invasive and non-invasive techniques, these insights through nanoscale characterization techniques underpin the importance of yet another perspective that could enrich our understanding of the battery degradation mechanism.
The pouch cells were fabricated in the commercial production line in EBTEB Electronics Co. Ltd. In the LCO//graphite pouch cell, the cathode typically consists of about 97% LiCoO2, 1.7% carbon black, and 1.3% PVDF binder, and the anode is composed of about 96% graphite, 1.3% conductive additive, and 2.7% carboxymethyl cellulose (CMC) binder. The solvents used for cathode and anode electrodes are NMP and DI water, respectively. The current collectors used for the cathode and anode are 10 μm Al foil and 10 μm Cu foil, respectively. We applied calendaring pressures of about 80 MPa for both cathode and anode electrodes to obtain the total thickness of about 105 ± 3 μm and 124 ± 3 μm for the double-side coated region, respectively. This yields a single-side mass loading of about 19.4 mg cm−2 for the cathode and 10.1 mg cm−2 for the anode. For a 4 Ah pouch cell, the typical amount of electrolyte used is about 2.0 g Ah−1; the fabricated pouch cell unit (including the control circuits and outside plastic package) has an average weight of about 102 g, corresponding to about 145 Wh kg−1 (measured at 1C and using a middle value voltage of 3.7 V vs. Li+/Li). The typical formation protocol for the pouch cell (without the FB additive) involves an initial charge at a low C-rate (0.2C) to a cut-off voltage of 3.2 V, 3.6 V, 4.1 V and 4.2 V, followed by a resting period (120 s) to allow the formation of a SEI on the anode. The cell is then discharged to 3.0 V at 0.2C. This process is repeated for two charge/discharge cycles to stabilize the cell, ensuring proper activation of the electrodes and long-term performance. The protocol is typically carried out at room temperature (around 25 °C).
Eads = Etot −(Ecomp + Egraphite) |
Edesol = (Emol + ELi+) − Ecomp |
MD simulations of electrolytes with/without FB were performed using GROMASC software.75 The temperature was controlled at 300 K using the Nose–Hoover thermostat. The many-body force field OPLS-AA was used.76 The partial atomic charges of PF6−, FB, and EC/DEC are obtained from LigParGen77 and Automated Force Field Topology Builder (ATB).78 The electrostatic interactions were computed using the Particle Mesh Ewald (PME) method. The cut-off distance of 1.5 nm was adopted for electrostatics and van der Waals interactions. The polarization of the electrode is employed as demonstrated in our previous work.11 The simulation boxes were 5.6 × 5.5 × 11.0 nm3 with 3 layers of the graphene sheet as the carbon anode. In the simulation boxes, the reference electrolyte consists of 156 LiPF6, 1000 EC and DEC molecules. The FB added electrolyte consists of 156 LiPF6, 770 EC and DEC, 460 FB molecules corresponding to the molar concentration and solvent ratio in the two electrolytes under ambient conditions. The equilibrium states of the system were reached by doing an energy optimization and then an NVT simulation of 15 ns with 1 fs for each step. The RDF and coordination number analyses were employed for the trajectory of last 1 ns.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5ee01076d |
‡ Y. C., W. X. and W. Z. contributes equally. |
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