Pavla
Eliášová
*a,
Břetislav
Šmíd
b,
Jana
Vejpravová
b,
Shuo
Li
a,
Federico
Brivio
a,
Michal
Mazur
a,
Daniel N.
Rainer
a,
M. Infas H.
Mohideen
a,
Russell E.
Morris
c and
Petr
Nachtigall‡
a
aFaculty of Sciences, Charles University, Hlavova 8, Prague 2 128 43, Czech Republic. E-mail: pavla.eliasova@natur.cuni.cz
bFaculty of Mathematics and Physics, Charles University, Ke Karlovu 5, Prague 2 121 16, Czech Republic
cEaStCHEM School of Chemistry, University of St. Andrews, St. Andrews KY16 9ST, UK
First published on 13th March 2024
Transition metal carbides and nitrides (MXenes) show a high potential for electrochemical energy storage in batteries and supercapacitors and for electrocatalysis. Their excellent electronic and magnetic characteristics have been highlighted in several theoretical studies. However, experimental research on MXenes is yet to confirm their predicted properties as candidates for controllable magnetic 2D materials. Here, we report our theoretical and experimental study of V2CTx MXenes (T = O, OH, F), providing key insights into their magnetism. Based on our density functional theory (DFT) analysis, we predicted ferromagnetic (FM) and antiferromagnetic (AFM) states of V2CTx, which are determined by the O/F ratio of surface functional groups. Accordingly, we prepared V2CTx MXenes in the form of multilayered powders and thin films with different O/F ratios. No experimental evidence of FM or AFM properties was found in any material. Nevertheless, powders and films with almost identical chemical compositions (in terms of O/F ratio) displayed different magnetic properties, whereas films with disparate chemical compositions revealed a similar magnetic character. Therefore, the preparation route and form of the final V2CTx material override the effect of the O/F ratio, which is often overestimated in theoretical studies. Moreover, these findings underscore the importance of preparing MXene materials to experimentally confirm their theoretically predicted properties.
MXenes display high electrical conductivity, redox active surface area and mechanical strength, in addition to rich surface chemistry. These properties endow MXenes with a high potential for many applications. As a case in point, these materials have been extensively studied for electrochemical energy storage applications, such as lithium-ion batteries,8 and electrochemical capacitors,9 and for photovoltaic applications.10 Furthermore, MXenes have been tested in electrocatalytic oxygen and hydrogen evolution and CO2 reduction,11 water desalination12 and, more recently, electromagnetic interference (EMI) shielding.13
MXenes have an Mn+1Xn general formula where M is a transition metal, and X stands for carbon or nitrogen. Only MXenes with M = Ti, V, Nb, Mo, Cr, Hf, Sc, Ta, W, or Y have been reported thus far, most of which prepared by wet-etching the aluminium layer of a parent MAX phase with a general formula of Mn+1AXn, where A represents elements of groups 13 and 14 of the periodic table, primarily aluminium. After aluminium removal, the surface of MXenes becomes covered by mixed terminations. MXenes are then designated by Mn+1XTx, where T can be O, OH, NH, F, Cl, Br, S, Se, or Te, depending on the etching14,15 and post-etching procedures.16–19 Typically, these etching procedures involve using (concentrated or in situ-formed) hydrofluoric acid and/or hydrochloric acid, which lead to O, OH, F and Cl terminal groups. In just over a decade, more than 30 stoichiometric MXenes have been synthesized, and more than a hundred MXenes (disregarding variable surface terminations) have been theoretically predicted.20,21 As one of the fastest growing class of 2D materials,7 MXenes have been the object of research of many theoretical studies, predicting excellent electronic and magnetic characteristics. For these properties, they stand out as ideal candidates for controllable magnetic 2D materials.21–26
Most pristine and functionalized MXene materials are non-magnetic due to strong covalent bonding between the transition metal and the X element and to surface functional groups, as shown by density functional theory (DFT) calculations.27 Conversely, MXenes based on Cr, V and/or Mn should be magnetically active, according to theoretical predictions.21,23–25,28,29 But whether symmetrical or asymmetrical with respect to the upper and lower surfaces, surface functionalization of these materials (e.g., F, O or OH) likely changes their magnetic properties. For example, Mn2CF2 is an intrinsic half-metal with a high Curie temperature (520 K), which can be used for spin injection in spintronics,24 and functionalized M2N (M = Mn, Cr and Ti) MXenes are half-metallic as well.30 So, half-metal materials, which are metallic in one spin channel and semiconductor or insulator in another, show ferromagnetism potentially applicable for spin injection.31
These theoretical results motivate experimentalists to develop new synthesis routes for 2D high-temperature spin-polarized materials with ferromagnetism or antiferromagnetism for potential spintronic applications. However, such properties are yet to be experimentally confirmed, and their applications in spintronics remain limited by the lack of intrinsic magnetism of MXenes. Making matters worse, experimental studies on the magnetic behavior of MXenes are few and far between. Nevertheless, magnetism has been experimentally identified in 2D MXenes such as Cr2TiC2Tx (but not in its parent 3D MAX phase),32 Mn3N2 (even at 300 K),33 and Ti3C2Tx (functionalized via treatment with hydrofluoric and chlorosulfonic acid).34 The last study has also shown that the magnetic properties of MXenes are affected by their surface terminal groups.34 In turn, the distribution of these terminal groups is affected by the etching conditions and post-synthetic treatments applied to prepare these materials.14–19 Therefore, we aimed at studying the relative contribution of these factors while experimentally testing the theoretically predicted electromagnetic properties of V2CTx28 as a model MXene.
Combining both experimental and theoretical approaches, we conducted a detailed study of the magnetic properties of V2CTx MXene. In our study, V2CTx materials were prepared by wet etching, applying different acid concentrations and post-synthetic treatment in oxygen flow to modify the terminal groups (the ratio between O and F groups; O/F ratio) and to assess their effect on MXene magnetism. These materials were obtained in the form of multilayered powders and ultrathin films and characterized by powder X-ray diffraction (PXRD), scanning transmission electron microscopy (STEM), and X-ray photoelectron spectroscopy (XPS), in addition to magnetic measurements. The experimental data were compared with DFT simulations to gain insights into the magnetic behavior of V2CTx materials.
As calculated, the formation energies (Eform defined in eqn (S1), ESI†) of functionalized V2CF2 and V2CO2 MXenes are relatively high (−4.13 and −4.89 eV, respectively) and represent the lower and upper bounds of mixed MXenes. In other words, the formation energies of all mixed V2COxF2−x MXenes are within these bounds (Table S1, ESI†), indicating that strong chemical bonds are formed between V and surface functional groups. The stacking of individual layers is shown in Fig. S2 (ESI†). The interlayer distances of various V2COxF2−x MXenes range from 0.218 to 0.246 nm in V2CF2 and V2CO2, respectively, corroborating previous findings (0.24 nm).36 Also in line with the experimental data and with previous reports,37 the calculated lattice parameters of V2COxF2−x MXenes (Table S1, ESI†) range from 0.295 to 0.316 nm.
Electronic states, spin polarization and magnetic properties were assessed for all V2COxF2−x MXenes considered in this study (Fig. S1 and Table S1, ESI†). As shown by the potential magnetic configurations (Fig. S3, ESI†), the presence of O and F on the surface of MXenes leads to charge transfer towards the surface (Bader charge analysis).38 This charge transfer affects the position of the V-3d orbitals in both spin channels. Our calculations of the local magnetic moments of V2CO2 revealed that V atoms are in a high spin state with 1 unpaired d electron (e.g., d1↑ spin configurations), corresponding to a V4+ electronic configuration. Thus, V2CO2 MXene is a ferromagnetic (FM) half-metal and has a total magnetic moment of 2μB (per unit cell), which mainly derives from V atoms. In contrast, V2CF2 MXene is an antiferromagnetic (AFM) semiconductor, and its V atoms are in a high spin state with 2 unpaired d electrons (e.g., d2↑ spin configurations), formally corresponding to a V3+ electronic configuration. The calculated magnetic moments of V atoms increase with the concentration of surface F-functionalization, ranging from 1.12 (V2CO2) to 1.84μB (V2CF2, see Table S1, ESI†).
Because the expected ratio between O and F functionalization is 2:
1, the results from the V2CO1.5F0.5 MXene model (with a 3
:
1 O/F ratio) are particularly relevant to experimental findings. All O and F configurations on the V2CO1.5F0.5 MXene model (Fig. S1, ESI†) are found in the FM ground state. Using V2CO1.5F0.5-C and V2CO1.5F0.5-E MXenes as prototypes (the letters from C to E denote specific configurations of O/F surface atoms, as defined in Fig. S1, ESI†), we show their partial density of states (PDOS) in Fig. S4 (ESI†). In addition, spin-polarized densities are shown in Fig. S5 (ESI†) together with the variation of the heat capacity of V2CO1.5F0.5 MXenes as a function of temperature calculated using Monte Carlo simulations. The corresponding Curie temperature is 7 K. The results show that not only spin polarization increases with the oxygen concentration but also the Curie temperature (TC) increases with the asymmetry of surface functionalization in V2CO1.5F0.5 MXenes. Accordingly, the Curie temperature can be engineered via surface functionalization.
We further considered four configurations of V2CO1.33F0.67 MXenes modeled using a (3 × 3) supercell (Fig. S6, ESI†) with a 2:
1 O/F ratio. All V2CO1.33F0.67 MXenes are found in the ferromagnetic ground state and are half metals (Fig. S6, ESI†). To gain insights into the intriguing electronic properties of V2CO2, V2CF2 and V2CO1.33F0.67 MXenes, PDOS of V-3d orbitals were plotted, as shown in Fig. S7a (ESI†). Given the local symmetry on V atoms of V2CO2 and V2CF2 MXenes, the V-3d orbitals split into a non-degenerate a (dz2) orbital and two 2-fold degenerate e orbitals, namely (dyz + dxz) and (dx2−y2 + dxy). Both the conduction band minimum (CBM) and the valence band maximum (VBM) depend on the V-3d orbitals. The spin polarization of V-3d orbitals of V2CO1.33F0.67 MXenes is stronger around the Fermi level than that of V2CO2 MXenes, but weaker in the deeper valence bands. Schematics of the spin polarization of V atoms in symmetrically and asymmetrically functionalized surfaces are shown in Fig. S7b (ESI†). Due to the different chemical environments in functionalized V2CO1.33F0.67 MXenes, the non-degenerate V-3d orbitals result in the ferromagnetic spin state.
Varying the concentration of O and F on one of the surfaces provides an effective way to control the spin polarization of V atoms. Computational results indicate that the magnetic state of V2COxF2−x MXenes is primarily determined by (i) the relative concentration of O and F surface atoms; all considered configurations of surface functional groups give the ferromagnetic state if the O/F ratio is above 2. But the relative stability of ferromagnetic and antiferromagnetic states is also modulated by (ii) the degree of asymmetry in the functionalization of upper and lower surfaces. Therefore, these two factors determine the magnetism of V2COxF2−x MXenes.
To exfoliate the layers, a freshly etched multilayered V2CTx (wet powder) was directly intercalated with a 25% tetramethylammonium hydroxide solution. Subsequent series of centrifugation and mechanical shaking yielded a black supernatant of exfoliated V2CTx layers. The exfoliated layers were immediately collected by filtration to prevent their degradation. Each material was denoted by the prefixes del (delaminated) and CA or DA depending on the etching conditions, as described in Table 1 (i.e. CA-del-V2CTx and DA-del-V2CTx). All thin films had a bronze hue. To demonstrate the reproducibility of etching in a diluted acid solution, we prepared delaminated films of V2CTx in two independent experiments to compare their properties and labeled them as DA-del-V2CTx (1) and DA-del-V2CTx (2). In their PXRD patterns (Fig. 2), all films have the same profile with similar intensities, and the (002) peak has the same position at 6.9° 2θ (corresponding to d-spacing 1.28 nm). Only DA-del-V2CTx (1) shows low intensity peaks of the parent MAX phase, indicating a minor fraction of unreacted V2AlC.
The films of delaminated V2CTx are displayed in Fig. 3e and f. In these films, the interlayer distance was 1.15–1.2 nm in DA-del-V2CTx (2) FILM and 0.97 nm in CA-del-V2CTx FILM. The d-spacing calculated from the (002) position in the PXRD pattern of the films was 1.28 nm. In contrast to these materials, the samples shown in Fig. 3c and d were prepared from the suspension of delaminated V2CTx, not the film. As determined by PXRD and STEM, the differences in d-spacing of the same films may be attributed to the treatment of these materials prior to analysis. For instance, the PXRD patterns of the films were measured on materials prepared by filtration of the suspension of delaminated V2CTx. As a result, the layer assemblies stacked on top of each other during the filtration.
Subsequently, the films were dried under vacuum, crushed into a powder and analyzed. As the delaminated V2CTx in suspension is dropped directly onto the holey-carbon copper TEM grid and then vacuumed under the STEM, water molecules between layers should more easily desorb (or de-intercalate) from a few layer assemblies than from films in which all layers are stacked on top of each other. As expected, when the films were crushed to a powder, deposited onto the TEM grid, and then exposed to high vacuum in situ within the STEM microscope, another portion of intercalated water molecules was desorbed. This desorption is thought to be the main reason for the discrepancy between d-spacings calculated based on powder XRD patterns and those determined from STEM images.
Multilayered powder DA-ml-V2CTx and the corresponding film, DA-del-V2CTx (1), have very similar chemical compositions, V2C0.80F0.96O0.90 and V2C0.71F1.05O1.02, respectively. In V 2p photoemission spectra of both materials, the strongest contribution is associated with V3+ at 515 eV (Fig. 4). The peak at 513 eV is attributed to V2+, indicating the presence of an unreacted V2AlC phase.42,46 Traces of unreacted V2AlC are also visible in the XRD pattern of DA-ml-V2CTx and DA-del-V2CTx (1) (Fig. 2). However, the V-C peak overlaps at the same binding energy (∼513 eV), which increases the peak.42 The peak at ∼516 eV is assigned to the V4+ component of a monolayer of vanadium oxide on the surface of vanadium carbide.39,42,46 The weak signal at ∼518 eV is assigned to the V5+ component, suggesting only minimal surface oxidation and thus the formation of vanadium oxide.
![]() | ||
Fig. 4 Component peak-fitting of XPS spectra of parent V2AlC, multilayered DA-ml-V2CTx and all delaminated films V2CTx. |
Two V2CTx films prepared under the same conditions, that is, treatment with diluted acids (DA-del-V2CTx (1) and DA-del-V2CTx (2)) had virtually identical chemical compositions and very similar XPS profiles (data fitting is shown in Table S2, ESI†). The similarity of these two samples prepared by repeating the etching procedure in diluted acid solutions supports the reproducibility of this etching protocol.
The CA-del-V2CTx film prepared in a concentrated acid solution had a higher concentration of fluorine groups and a lower concentration of oxygen groups, V2C0.65F1.18O0.77, than the films prepared in diluted acids, V2C0.69–0.71F1.05–1.06O1.02–1.07. In a previous study, the chemical stability of V2CTx materials has been tested by heating multilayered V2CTx powders up to 600 °C in nitrogen, carbon dioxide, air or hydrogen atmosphere, monitoring changes by Raman spectroscopy and XPS.42 Here, we tested the stability of V2CTx films by exposing the films to oxygen for 4 and 8 hours. We applied only mild conditions at room temperature because we intended to replace fluorine groups on the V2CTx surface whilst avoiding vanadium oxidation into vanadium oxide. Our theoretical calculations indicated that V2CTx would be a ferromagnetic material if the oxygen groups prevailed on the surface (the computational findings are discussed above). Based on our XPS analysis, after 4 (DA-del-4O2-V2CTx) and 8 (DA-del-8O2-V2CTx) hours in oxygen flow, the films displayed only a slightly lower F/O ratio than fresh DA-del-V2CTx (1) (see Table 1).
The V3+/V5+ ratio can be used as an indicator of the undesired transformation of V2CTx MXene into vanadium oxide. The fresh film DA-del-V2CTx (1) has a V3+/V5+ ratio of 2.98, but after 4 and 8 hours in oxygen, the films have V3+/V5+ ratios of 2.51 and 2.3, respectively. This decrease in V3+/V5+ ratio indicates that the concentration of vanadium oxide increases due to oxygen exposure. However, the concentration of fluorine groups remains relatively high (V2C0.71–0.74F0.88–0.94O1.08–1.4). After 10 months of storage in a desiccator, the film prepared in concentrated acid solution, CA-del-V2CTx, was also exposed to oxygen flow for 8 hours to assess surface changes. The V3+:
V5+ ratio significantly dropped from 4.02 to 1.79, and the overall composition changed from V2C0.65F1.18O0.77 to V2C0.71F0.87O1.74. This result demonstrates that the V2CTx film is slowly degraded even when stored in a desiccator, but fluorine groups remain in the composition and are not arbitrarily exchanged for oxygen groups, as proposed in previous studies.40,42
![]() | (1) |
For samples with realistic C values, the effective magnetic moment was calculated using the following formula:
![]() | (2) |
![]() | (3) |
The parameters derived from the fit of the modified Curie–Weiss law are outlined in Table S3 (ESI†). Our analysis confirmed that Pauli paramagnetism occurs in V2AlC (χ0 = 9.3 × 10−8 m3 mol−1) and that localized paramagnetism prevails in multi-layered DA-ml-V2CTx, with μeff = 1.67μB, which is close to the theoretical spin-only value of the free V4+ ion (1.73μB). In the samples with “mixed” paramagnetism, μeff ranges from 0.55 to 0.61μB, and χ0 ranges from 2.3 × 10−9 to 2.9 × 10−8 m3 mol−1. In all samples with Curie paramagnetism, the θP values are <2 K, which is consistent with the absence of a long-range magnetic order down to 2 K.
The magnetization isotherms, M(H) recorded at 4 and 300 K, shown in Fig. 6 and Fig. S13 (ESI†), respectively, corroborate the proposed scenario. The M(H) of V2AlC is almost identical at both temperatures, as expected for temperature-independent Pauli paramagnetism. A closer inspection of the M(H) curve around the origin reveals moderate hysteresis (∼50 mT), which may be attributed to ferromagnetic impurity revealed by molar susceptibility analysis. The M(H) of DA-ml-V2CTx, recorded at 4 K has a clear Brillouin-type character, reaching ∼0.6μB f.u.−1 at 7 T, while the other samples reach much lower values (∼0.05–0.1μB f.u.−1 at 7 T), as expected for “mixed” paramagnetism.
Based on our XPS analysis (Table 1), multilayered DA-ml-V2CTx powder has a similar chemical composition to that of the thin film DA-del-V2CTx (1), which was prepared from DA-ml-V2CTx by organic intercalation and delamination (V2C0.80F0.96O0.90vs. V2C0.71F1.05O1.02, respectively). In both samples, the ratio between F and O groups is approximately 1:
1. Nevertheless, the DA-ml-V2CTx powder displays localized paramagnetism, with μeff = 1.67μB, while the thin film DA-del-V2CTx (1) shows “mixed” (metallic and localized) paramagnetism with μeff = 0.55μB. These differences in magnetic properties may be explained by differences in the integrity of crystallites as thin films crystallites contain numerous holes and cracks (evidenced by STEM images).
The main difference in chemical composition was identified between the fresh film CA-del-V2CTx and the same film after 10 months (and additionally after 8 hours in oxygen flow) CA-del-8O2-V2CTx (V2C0.65F1.18O0.77vs. V2C0.71F0.87O1.74, respectively). Even when significantly varying the O/F ratio from 0.65:
1 to 2
:
1, the two films displayed similar magnetism, that is, mixed paramagnetism, with effective magnetic moments of 0.56 and 0.61μB, respectively.
Although ab initio calculations usually predict a localized magnetic moment on V and a long-range magnetic order aligned with temperatures from units to tens of Kelvin,48 our experimental results rule out a ferromagnetic or antiferromagnetic order of localized magnetic moments on V. Instead, most V2CTx samples revealed superposition of metallic (Pauli) and localized paramagnetism, except for multi-layered DA-ml-V2CTx, nearing localized magnetism. This magnetic behavior can be understood considering the complexity of materials, in contrast to idealized theoretical models. Real samples contain various types of defects, local functionalization inhomogeneities and holes and cracks in crystallites (as evidenced by microscopy). Thus, the stable, long-range magnetism of fully localized spins is most likely suppressed by the intrinsic structural and spin disorder. Moreover, the magnetic properties are more affected by the crystallite sizes, shapes and the level of their disruption (for instance, holes and cracks) than by the actual chemical composition (particularly O/F ratio).
Ultimately, inconsistencies between experimental observations and theoretical predictions underscore the need for a more realistic description of magnetism in such complex materials. However, the level of crystallite damage during the etching and delamination process is difficult to predict. For now, this task remains highly challenging, if not impossible.
The chemical composition of the samples was measured on an X-ray photoelectron spectrometer equipped with a non-monochromatized Mg Kα X-ray source (1253.6 eV) and with a Phoibos 150 (SPECS GmbH, Germany) hemispherical analyzer operating in Fixed Analyzer Transmission (FAT) mode. After their preparation, the samples were kept under argon atmosphere for protection and mounted on a carbon double tape placed on a sample holder for XPS analysis. Survey spectra were collected at 40 eV pass energy, 0.5 eV step size, and 100 ms dwell time. Core-level spectra of O 1s, V 2p, N 1s, C 1s, F 1s, Cl 2p and Al 2p were collected at 20 eV pass energy, 0.05 eV step size and 100 ms dwell time. The satellite peaks from the non-monochromatized Mg X-ray source at 8.4 and 10.2 eV displacements and with 8.0 and 4.1% relative intensities, respectively, were filtered out of the spectra. The data were analyzed using KolXPD fitting software (KolXPD, Kolibrik.net, Czech Republic). All photoemission spectra were fitted with a mixture of Lorentzian and Gaussian function profiles after a Shirley background subtraction.
SEM images were obtained under a JEOL JSM-IT800 microscope using a secondary electron detector. Images were taken at a 1 kV accelerating voltage. All samples were deposited on conductive carbon tape mounted onto the SEM holder.
STEM images were acquired under a JEOL NEOARM 200 F microscope equipped with a Schottky-type field emission gun at 200 kV accelerating voltage, with annular dark-field (ADF) detector.
Details on the computational methods are described in ESI.†
The magnetic properties of the samples were measured using a properly calibrated MPMS XL-7 device (SQUID magnetometer, Quantum Design). Kept under an argon protective atmosphere, the samples were rapidly transferred in a gelatine capsule, fixed in polystyrene onto a sample holder with a negligible background signal, and inserted inside the sample chamber of the magnetometer, which was evacuated and flushed with inert helium gas three times. The experiments were performed under helium gas exchange to enable fast sample thermalization. The variation of magnetization as a function of temperature, M(T), was recorded at a constant magnetic field of 1, 2, and 4 T with a 2 K step after cooling the sample in the remnant field of the superconducting coil (below 0.5 mT). Magnetization isotherms, M(H), were recorded at 4 K and 300 K under varying magnetic fields up to ±7 T with a 0.5 T step. All magnetization data were recalculated to the molar units using the mass determined from XPS experiments.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4tc00132j |
‡ Deceased. |
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