Eduardo David
Ruiz-Santacruz
a,
José de Jesús
Vega-Soria
a,
Aura Karina
Cruz-Jiménez
a,
Uriel
Caudillo-Flores
b,
Nidia Libia
Torres-García
a and
Karina
Suárez-Alcántara
*a
aMorelia Unit of Materials Institute Research, National Autonomous University of Mexico, Antigua Carretera a Pátzcuaro No. 8701, Col. Ex Hacienda de San José de la Huerta, Morelia CP 58190, Mexico. E-mail: karina_suarez@materiales.unam.mx
bCentro de Nanociencias y Nanotecnología, Universidad Nacional Autónoma de México, Ensenada, B.C. CP 22860, Mexico
First published on 10th September 2024
Herein, a simple synthesis method for Mg2Ni composites with carbon nanofibers capable of hydrogen storage is presented. Specifically, n-butyl-sec-butyl-magnesium solution in hexane (C8H18Mg, 0.7 M) and bis-cyclopentadienyl nickel(II) (nickelocene or NiCp2) were used as precursors for the Mg2Ni nanoparticles. Subsequently, the nanoparticles were composited with carbon nanofibers (CNF) with high loading of Mg2Ni of 50 wt%, 75 wt%, 90 wt%, and 100 wt%. The physicochemical characterization of the materials indicated that the size of the as-prepared Mg2Ni nanoparticles was less than 5 nm and they were highly agglomerated due to a carbon-based binder. The best hydrogen storage values were determined to be 2.6–2.7 wt%. Among the tested materials, the composite with 75 wt% of Mg2Ni in CNF presented the best hydrogen uptake. The pressure–composition–temperature curves indicated changes in the hydriding equilibrium pressures of the Mg2Ni nanoparticles compared to the material with a similar composition produced using ball-milling and thermodynamic calculations. Thus, the results presented herein indicate the beneficial effect of nanosizing on hydriding reactions.
Recently, the formation of Mg-nanoparticles, nanoconfinement, or nanomodification has been proposed as strategies to surpass the kinetic and thermodynamic limitations of bulk Mg.12–15 In theory, reducing the particle size can lower the dehydrogenation temperature and significantly increase the kinetics. The particle size threshold for Mg has been reported to be as low as 1.3 nm.13 Employing the same approach, the formation of Mg2Ni/Mg2NiH4 nanoparticles can be of interest. However, the number of published papers on this subject is limited. Thus, this work presents the synthesis and characterization of Mg2Ni nanoparticles composited with a carbon material. The selected synthesis method is a bottom-to-top method using organometallic precursors, and the results are compared to a “classic” material prepared via the mechanical milling of elements.
M. Fichtner proposed that the reversibility of hydriding/dehydriding reactions in nanoparticles of complex hydrides may be reduced if the nanoparticles are free-standing on a surface and enhanced if they are enclosed.16 Thus, the compositing of materials plays an important role in the fabrication of nanomaterials for hydrogen storage. Hydrogen storage nanoparticles have been mixed with several carbon materials such as activated carbon, graphite, carbon aerogel scaffolds, carbon aerogel microspheres, mesoporous carbon, graphene, carbon nanospheres, a variety of carbon nanotubes, and carbon nanofibers.17–25 Thus, carbon nanofibers (CNF) can be an interesting compositing material, given that they are cheaper than other nanosized carbons and have a high surface area. Herein, we present the use of carbon nanofibers as a compositing material for Mg2Ni nanoparticles. Alternatively, the loading of hydrogen storage nanoparticles in carbon materials is typically low (about 10–20 wt%).26,27 This translates into a reduction in the hydrogen storage capacity due to the weight of the compositing material. Thus, studies on hydrogen storage nanomaterials with a high loading of active materials are necessary. In the present work, we used a variation of the synthetic method of Zlotea et al.26 with high loads of Mg2Ni in carbon nanofibers of 50 wt%, 75, wt.% and 90 wt%; and 100 wt% Mg2Ni nanoparticles (i.e. no addition of CNF) for comparison.
A material containing 75 wt% of Mg2Ni and 25 wt% of carbon nanofibers was prepared by ball milling as a reference. Stoichiometric quantities of Mg, Ni (Alfa-Aesar, 325 mesh, 99.86 purity), and CNF powders were loaded in a milling vial together with 6 balls with a diameter of 1 cm. The milling balls were made of yttria-stabilized zirconia and the milling vial with a volume of 50 mL was made of stainless steel. The total milling time was 20 h and the milling batch was 1 g. The milling was performed in a Retsch® mill working in room-temperature mode at an agitation rate of 25 Hz. Then, the ball-milled precursors were annealed at 400 °C for 1 h under high vacuum.9,28 The ball-milling/annealing preparation of Mg2Ni is well-known. However, the formation of Mg2Ni just by ball-milling is rare, while the formation of Mg2Ni is easy by applying heating under vacuum or cycling in the hydrogen of the milled precursors. The milling and annealed material was characterized, tested, and presented as needed for comparison.
X-ray diffraction (XRD) characterization was performed in a Bruker D2 Phaser diffractometer. Cu Kα (1.540598 Å) wavelength was used. The powders were compacted in a dedicated sample holder; then, they were covered with Kapton® tape for protection against ambient oxygen and moisture. Crystalline phase identification was performed with the help of the Maud software and crystallographic databases including Inorganic Crystal Structure Database Karlsruhe (ICSD) and Crystallography Open Database (COD).
Scanning electron microscopy (SEM) images of selected samples were collected in a JSM-IT300 microscope. The samples were dispersed on carbon tape inside an argon-filled glovebox. Then, they were transferred to the SEM chamber reducing the oxygen contact using a glove bag. However, brief air exposure occurred during the transfer to the vacuum chamber of the SEM apparatus. SEM images were obtained with secondary or backscattered electrons at an acceleration voltage of 10 and 20 kV. Elemental mapping was performed by an SDD X-MaxN EDS detector, Oxford Instruments attached to the microscope with an energy resolution of 127 eV.
Transmission electron microscopy (TEM) images were collected on a JEOL ARM-200F, Schottky-type field emission transmission electron microscope with atomic resolution, equipped with a spherical aberration corrector (Cs) in STEM mode. A few milligrams of each studied material were dispersed in THF by ultrasonic agitation. The samples and THF were confined in small vials and sealed in argon inside a glovebox. Then, the sealed vials were taken out of the glovebox and mixed in an ultrasonic bath for 10 min. Then, the vials were returned to the glovebox, and the slurries were deposited dropwise on dedicated copper grids and left to dry at room temperature. The materials on the grid were transported to the transmission electron microscope in vials sealed in argon. The materials were briefly exposed to air during transfer to the TEM apparatus. TEM images were taken in both dark-field and bright-field modes.
Fourier-transformed infrared spectroscopy (FTIR) was performed on a Thermo Scientific Nicolet iS10 FTIR spectrometer using an attenuated total reflectance (ATR) accessory with a diamond crystal. About 2 mg of materials was mixed with 50 mg of dry KBr in an agate mortar and compacted in a dedicated press. The KBr was dried in a vacuum oven at 120 °C for 2 h, and then quickly transferred to a glovebox. The mixing and compaction of the materials were performed inside the glovebox. However, the materials were briefly exposed to air during data collection. The presented spectra are an average of 32 spectra collected for each sample in the range of 4000–650 cm−1 at a spectral resolution of 1 cm−1.
X-ray photoelectron spectroscopy (XPS) analysis was performed to determine the chemical state of the studied materials. All measurements were performed in a SPECS spectrometer with a PHOIBOS® 150 WAL hemispherical energy analyzer with angular resolution (<0.5°), equipped with an XR 50 Al-X-ray and μ-FOCUS 500 X-ray monochromator (Al excitation line) sources. To this end, the materials were transported to the XPS in sealed argon-filled vials. The samples were degassed at 10−5 mbar in the pretreatment chamber before being transferred to the analysis chamber. The measurement chamber had a residual pressure of less than 5 × 10−9 mbar during the measurements. Data was processed with the CasaXPS software and the background was modeled as Shirley-type.
Further heating to 260 °C under high vacuum was performed just before the PCT experiments to eliminate the organic part of the precursors. This step was essential for hydrogen storage, given that preliminary experiments without heating under vacuum resulted in poor hydrogen storage. The proposed complete reaction for the formation of Mg2Ni is as follows:
2C8H18Mg + NiCp2 → Mg2Ni + nCxHy, | (1) |
Other reports indicate the direct formation of hydrided nanoparticles of Mg, Mg–Ni, or Mg–Fe when the heating of organometallic precursors in a hydrogen atmosphere is performed.26 However, this method is more complicated because of the use of a pressurized gas reacting with a liquid solution.
Fig. 2 presents a series of TEM images of the as-prepared samples. Fig. S16 to S26 (ESI†) show the TEM images at different magnifications of as-received CNF, as-prepared materials, and particle size distributions. The image of the as-received CNF (Fig. S16, ESI†) is consistent with the characteristics reported by the supplier, i.e. 100 nm in diameter, 20–200 μm long, and a conical assembly of graphitic platelets. In Fig. S16,† it can be noticed that the center of the as-received CNFs is empty and their ends are closed. Fig. 2(a)–(d) demonstrated that independently of the Mg2Ni load, the as-prepared materials were in the form of nanoparticles. Q. Peng et al. suggested that the hydrogenolysis of NiCp2 produced finer Ni-nanoparticles than other forms of Ni-nanoparticle production.29 After dispersion in THF for TEM sample preparation, the big agglomerates observed in SEM were destroyed and the nanoparticles were observed to be distributed in agglomerates (Fig. S17 and S20†) or on the surface of the CNF (Fig. S21 and S23†). The most frequent nanoparticle diameters are 3.7 nm, 2.3 nm, 4.0 nm, and 3.1 nm for 50%Mg2Ni-CNF, 75%Mg2Ni-CNF, 90%Mg2Ni-CNF, and 100%Mg2Ni, respectively. The size distributions are presented in Fig. S18, S22, S24, and S26 of the ESI,† respectively. We can remark that the synthesis route is simple, without the need for special equipment, and even in the absence of a hydrogen atmosphere during the preparation of the materials, the precursors reacted, and the produced nanoparticles are small and homogenous. Additionally, according to the comparison of the TEM images (Fig. S25†) and the characterization presented in the next sections, we conclude that the nanoparticles are surrounded by an amorphous carbon-based material produced by the partial release and decomposition of the organic part of the precursors. The formation of a carbon layer was also observed by other researchers when using organic precursors and solvents. For example, X. Lu et al. produced Mg2Ni nanoparticles with a size of 300–500 nm by the wet chemical ball milling of the Mg and Ni elements and a mixture of organic agents and solvents.32 Carbon layers may help decrease the unwanted oxidation and sintering of nanoparticles, but also reduce the interaction of hydrogen with the nanoparticles.
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Fig. 2 TEM images of (a) as-prepared 50%Mg2Ni-CNF, (b) as-prepared 75%Mg2Ni-CNF, (c) as-prepared 90%Mg2Ni-CNF and (d) as-prepared 100% Mg2Ni. |
The XRD patterns of the as-prepared materials are presented in Fig. 3. All diffractograms present the diffraction of the Kapton tape routinely used to protect the samples from unwanted oxidation. Kapton produces three amorphous peaks in the 2θ range of 15° to 25° and a strong background that extends up to 34°. From the bottom to top, the first frame (Fig. 3(a)) presents the X-ray diffraction pattern of the as-received carbon nanofibers. The CNF material presented diffraction peaks consistent with graphite but with changes in the expected peak intensity due to the alignment of the graphitic platelets. The most intense peak is located at the 2θ value of 26.23°, corresponding to (002). The other CNF diffraction peaks are much less intense than expected. The graphite peak positions are shown in Fig. 3 as green lines. The second frame (Fig. 3(b)) presents the pattern of 75%Mg2Ni-CNF-MM produced by ball-milling and annealing. All the diffraction peaks correspond to Mg2Ni. Fig. S27 of the ESI† presents the tracking of the ball-milling time of Mg and Ni. Long milling times resulted in the amorphization of Mg and Ni. However, the formation of Mg2Ni only appeared after annealing,9 indicating the importance of this process for the formation of the intermetallic material. The most intense peak of CNF is very low in the ball-milled material, indicating a decrease in the size of the carbon nanofibers, which is consistent with the SEM images. The rest of the frames (Fig. 3(c)–(f)) present the diffraction of the Mg2Ni nanoparticles from the wet-synthesis with a decrease in the content of CNF. The intensity of the (002) peak progressively decreased. In the case of the 50 wt%, 75 wt%, and 90 wt% content of Mg2Ni from the wet synthesis, no indications of the formation of crystalline micro-sized materials can be observed. Thus, we conclude that all the formed Mg2Ni are nanoparticles for the series of materials with carbon nanofibers. For the Mg2Ni without CNF (100%Mg2Ni), a series of peaks indicate the presence of some unreacted NiCp2 precursor. Additionally, the 100%Mg2Ni material also presents an unknown peak at the 2θ value of 10.94°, which is probably related to the decomposition of an intermediate.
Fig. 4 presents the experimental XPS and deconvoluted data at the C 1s, Mg 2p, Ni 2p, and O 1s edges. Fig. 4(a) presents the C 1s edge, where the four composites present the characteristic graphite (C–C) peak of C at 284.8 eV (red lines in Fig. 4(a)).33 In the case of the 50%Mg2Ni-CNF material, the graphite peak is dominant in the XPS spectrum. However, another component of the materials is located at 285.3 eV (dark yellow peaks), which is attributed to C–H.33 The C–H peak presented a small shift to 285.0 eV in the 75%Mg2Ni-CNF material and 284.9 eV in the 90%Mg2Ni-CNF material. Interestingly, this peak was not present on the surface of the 100%Mg2Ni material. Meanwhile, the 75%Mg2Ni-CNF presented an additional peak (dark green) located at 284.3 eV, which can be related to CC.33 Finally, the 75%Mg2Ni-CNF, 90%Mg2Ni-CNF, and 100%Mg2Ni materials present a small peak (blue peaks) that can be interpreted as C–O interactions at about 290–288 eV.
Mg and its alloys easily oxidize in the presence of even minor quantities of oxygen. The formed oxide can reduce the kinetics and hydrogen uptake. In Mg and its alloys, the presence of oxides is evident by a prominent peak at 51.2 eV.34 The metallic Mg 2p XPS signal is expected at lower energies (49.6 eV (ref. 34 and 35)). At the oxidized surface of Mg, the XPS data was deconvoluted clearly into two or more peaks. Alternatively, the Mg 2p XPS signal of the materials with CNF was deconvoluted in a single peak. However, we did not discard the presence of a small amount of oxide because oxygen is practically omnipresent. In the Mg 2p XPS data of the Mg2Ni-CNF materials, the main peak values are 50.5 eV, 50.7 eV, 50.3 eV, and 50.3 eV for 50%Mg2Ni-CNF, 75%Mg2Ni-CNF, 90%Mg2Ni-CNF, and 100%Mg2Ni, respectively. These values indicate that there is no particular trend with respect to the CNF content. These peaks can be related to the presence of a partially reduced Mg precursor. Accordingly, 100%Mg2Ni was better deconvoluted into three peaks. In addition to the peak at 50.3 eV, the binding energy of the second peak is located at 49.6 eV (blue line), indicating the presence of metallic Mg. The third peak is located at 51.8 eV and is related to the formation of a small quantity of surface oxides of Mg (dark-green peak near the baseline in light green). Together with the presence of unreacted and decomposed intermediates of NiCp2 in the XRD characterization, the XPS data indicate that the Mg-organometallic precursor can be reduced to some degree even if NiCp2 is not.
Fig. 4(c) presents the Ni 2p XPS signal of the studied composites. The Ni 2p edge is composed of Ni 2p3/2 (major intensity), Ni 2p1/2, and their satellite signals. The positions and intensities of the main peaks and satellites depend on the oxidation state and geometry of the Ni compounds.36 The satellites associated with the 2p of transition metal compounds are interpreted as the excitation of a metal 3d electron into an unoccupied metal orbital concurrently with the emitted photoelectron.36,37 The intensity of satellites is dependent on the probability of the material being excited during the photoemission process.38 The Ni 2p3/2 of metallic Ni is expected at 852.6 eV, while NiO and Ni(OH)2 show the main peaks at 853–853.5 eV and 856.5 eV, respectively.35 NiO presents a clear splitting of the Ni 2p peaks,39 while the Ni(OH)2 peak presents a similar shape to the metallic Ni, but is wider.35,40 The XPS spectra in Fig. 4(c) are shifted from the expected metallic value to that for Ni2+. The Ni 2p peaks are located between the values of the NiO and Ni(OH)2.41 However, the peaks evolved with a decrease in the CNF content and presented other characteristics that discard the massive unwanted oxidation or contamination with the formation of NiO and Ni(OH)2. The red deconvoluted peak component of Ni 2p3/2 appeared at 854.1 eV, 855.3 eV, 853.5 eV and 853.2 eV for 50%Mg2Ni-CNF, 75%Mg2Ni-CNF, 90%Mg2Ni-CNF, and 100%Mg2Ni, respectively. Additionally, the peak intensity progressively decreased to a small peak in the 100%Mg2Ni material. Conversely, a dark-blue peak appeared in 75%Mg2Ni-CNF, and also shifted to a lower binding energy in the 90%Mg2Ni-CNF and 100%Mg2Ni materials. This peak appeared at 856.9 eV, 855.6 eV, and 855.0 eV for 75%Mg2Ni-CNF, 90%Mg2Ni-CNF, and 100%Mg2Ni, respectively. Thus, the peak position and intensity evolution can be interpreted as the partial formation of nanoparticles in this stage of the synthesis and the presence of unreacted or partially reacted NiCp2. To confirm this, the O 1s XPS spectra of the materials are presented in Fig. 4(d). This series of O 1s XPS spectra is dominated by a peak at around 531.8 eV to 532.4 eV (red or purple for a single peak deconvolution), corresponding to different carbon–oxygen interactions.42,43 Another peak is located at 529.8–530.5 eV (blue peaks in Fig. 4(d)), which can be associated with the formation of surface magnesium oxides. Despite this peak being prominent in the O 1s (Fig. 4(d)) for 100%Mg2Ni, the corresponding information at Mg 2p (Fig. 4(b)) indicates the formation of a small amount of oxides.
Additionally, the infrared spectroscopy characterization of the as-prepared nanosized materials is presented in Fig. S28 in the ESI.† For comparison, the infrared characterization of the as-received NiCp2 is presented in Fig. S28(a).† NiCp2 presented the characteristic peaks,44 with the most intense peaks observed at 768 cm−1 and 1001 cm−1. The C–H stretching bands of n-butyl-sec-butyl-Mg are expected at 2800–3300 cm−1. In the case of CNF, it presents weak peaks at around 2000–2300 cm−1 due to its CC bonds.45–48 The as-prepared nanosized materials (Fig. S28(b) to (e)†) present a progressive increase in the relative intensity of the most intense peaks of NiCp2, which is in agreement with the increase in concentration but somehow deformed. In parallel, Fig. S28(b) to (e)† present a decrease in the intensity of some minor peaks such as the peak at 1422 cm−1, and the progressive change in the position of the peak at 3082 cm−1, which is attributed to the C–H bonds, ending as a complex peak at 2800–2900 cm−1. The described changes are consistent with the partial decomposition of NiCp2 and n-butyl-sec-butyl-Mg during drying at 140 °C. The relative intensity of the remaining peaks indicates the progressive difficulty in the formation of Mg2Ni with an increase in the load of the precursors, NiCp2 and n-butyl-sec-butyl-Mg, and a decrease in the load of carbon nanofibers.
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Fig. 5 Pressure–composition isotherms of (a) 50%Mg2Ni-CNF, (b) 75%Mg2Ni-CNF, (c) 90%Mg2Ni-CNF, (d) 100% Mg2Ni, and (e) 75%Mg2Ni-CNF-MM, ball milled and annealed under high vacuum. |
The shape of the PCT curves presented in Fig. 5 indicates the ease of hydriding and the difficulty of dehydriding reaction for the nanosized materials. The incomplete dehydriding on the nanosized materials indicates the need for a moderate-high vacuum, which was poorly managed in our Sieverts apparatus. The dehydriding reaction on the nanosized materials could be constrained by the stability of the nanoparticles gained upon hydride formation. Meanwhile, at the ball-milled 75%Mg2Ni-CNF, the equilibrium pressure at 300 °C is well defined for the hydride and dehydriding reactions. M. Fichtner proposed a dependency of the enthalpy of the hydriding reaction, and in turn the dependency of the equilibrium pressure on particle size.16 However, the parameters of the Fichtner equations are not yet defined experimentally.16 Nonetheless, the effect of particle size is relevant to the position of equilibrium pressure for hydriding/dehydriding reactions.
Fig. 5(a)–(c) demonstrate the low equilibrium hydriding pressure of the Mg2Ni nanoparticles. In the case of the 75%Mg2Ni-CNF material, the equilibrium pressure is about 0.09 bar, 0.6 bar, and 5.2 bar at 100 °C, 200 °C and 300 °C, respectively. Meanwhile, the ball-milled 75%Mg2Ni-CNF-MM material presented hydriding equilibrium pressures of 0.44 bar, 0.78 bar, and 2 bar at 100 °C, 200 °C, and 300 °C, respectively. The listed values indicate a notable reduction of the equilibrium pressure in the nanoparticles of Mg2Ni.
Several experimental conditions for the preparation of materials can affect the hydriding and dehydriding reactions. Thus, it is difficult to compare the “same materials” reported by different research groups. Nevertheless, we include published reports to compare nano- and micro-sized Mg2Ni. Alternatively, the best way to qualify experimental results is to compare the hydriding/dehydriding equilibrium pressures versus thermodynamic data. Fig. 6 presents a comparison of the results of equilibrium pressures of this work with other thermodynamic and experimental values. Thermodynamic equilibrium pressures can be calculated according to,49 as follows:
![]() | (2) |
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Fig. 6 Thermodynamic equilibrium line (green) for Mg2Ni/Mg2NiH4. Red dots: hydriding equilibrium pressure of the 75%Mg2Ni-CNF and 75%Mg2Ni-CNF-MM materials. Blue dots: hydriding4,11,52,53 or dehydriding51 equilibrium reported data. |
Despite the importance of Mg2Ni, relatively few PCT curves have been reported. Together with the available reports, the PCT curves present different equilibrium pressures. The blue dots in Fig. 6 show the reported equilibrium pressures and serve for discussion. A. K. Singh et al. reported the desorption PCT curve of Mg2NiH4 prepared by 100 h of ball milling of the elements and after the fifth cycle;51 the equilibrium pressure was not well defined in that report, but the middle point of the curve was located at about 14 bar, and 2 wt%. Y. Wang et al. reported the PCT curves of pure Mg2Ni ball milled with low quantities of multi-walled carbon nanotubes or graphite (1–5 wt%), whose hydriding equilibrium pressure is located at about 5.5 bar at 320 °C; they achieved 3.5 wt% hydrogen storage.52 No influence of the multi-walled carbon nanotubes or graphite on the PCT curves of Mg2Ni was reported in that work.52 R. Janot et al. demonstrated a hydriding equilibrium pressure of about 3 bar at 150 °C for ball-milled Mg2Ni/10 wt%C + 5 wt%Pd and about 1 bar for the material without the addition of C and Pd.11 They achieved 2.7 and 1.4 wt% for Mg2Ni/10 wt%C + 5 wt%Pd and Mg2Ni, respectively.11 T. Hongo et al.53 presented similar PCT curves to that in Fig. 5(a)–(d), i.e. not achieving full dehydriding of the materials. In that report, Mg2Ni was processed by high-pressure torsion (HPT) and the hydriding equilibrium pressure was located at about 0.2 bar at 150 °C (as read from the plots).53 Also,53 the hydrogen uptake was about 3.25 wt%. Additionally, the desorption branch of the PCT curve was not defined53 even at low pressures as 0.01 bar. In this case, dehydriding was achieved by heating under dynamic vacuum for 20 h at 150 °C.53 R. Mazzaro et al. reported the formation of Mg–Ni (20 at%–Ni) nanoparticles whose hydriding equilibrium pressure is located at about 0.05 bar at 150 °C.4 The reviewed reports4,11,51–53 present a great variety of preparation techniques and experimental measurement conditions; nevertheless, the nano-sized Mg2Ni developed in this work can achieve similar hydrogen uptake levels. The variation in the equilibrium pressures can be a result of the preparation techniques and additives, which produce changes in the structure (superficial or bulk) of the materials.
Fig. 7 presents the SEM images of the hydrided (PCT) Mg2Ni-CNF materials at 300 °C. In general, the materials presented a breaking-up of the initial agglomerates, confirming the presence of the CNF and the existence of a binder material that is assumed to be composed of carbon material as a residue of the organic part of the precursors. The 50%Mg2Ni-CNF PCT-300 material developed a net structure due to the high amount of CNF. Meanwhile, the 75%Mg2Ni-CNF PCT-300 material developed a partial net structure due to the reduction in the content of CNF. Both materials reached near full hydrogen storage according to the Mg2Ni content; however, a low load of hydrogen storage material is not recommended due to the low hydrogen uptake. In this case, the high-load materials, 90%Mg2Ni-CNF PCT-300 and 100%Mg2Ni-PCT-300, did not present the formation of net structures, which can justify the lower hydrogen uptake than that expected. The high-load materials maintained the presence of blocks of about 10–30 μm. Additional SEM images of the hydrided materials can be found in the ESI, Fig. S29 to S32.†
Fig. 8 presents a series of TEM images of the hydrided (PCT) nanosized materials at similar magnifications. Fig. S33 to S42 of the ESI† present more TEM images at different magnifications as a complement. Fig. 8(a) presents the TEM image of 50%Mg2Ni-CNF, where the nanoparticles are dispersed on the CNF surface. Meanwhile, the TEM image of 75%Mg2Ni-CNF (Fig. 8(b)) presents a dispersion of particles, which can be interpreted as being within the CNF. This is not the only image indicating this characteristic (see Fig. S33, S36, and S37 of the ESI†). Also, the TEM images of 90%Mg2Ni-CNF and 100%Mg2Ni (Fig. 8(c) and (d)) corroborated the presence of a material whose function is a binder of the nanoparticles of Mg2Ni and Mg2NiH4, respectively. It can be concluded that the Mg2NiH4 nanoparticles are distributed on the CNF surface, between the binder material, and a minor proportion inside the CNF (Fig. 8(b)).
The sintering of materials is a common feature of nanoparticles after heating under pressure. Accordingly, in the present materials after hydriding, the nanoparticles showed a change in size. The particle size distributions are presented in Fig. S35, S38 and S40.† In the case of the hydrided 50%Mg2Ni-CNF and 75%Mg2Ni-CNF, their particle size increased to 7.9 nm, and 4.4 nm, respectively (most frequent sizes). These numbers indicate an increase of almost 100%. The 90%Mg2Ni-CNF (Fig. S40†) material presented almost the same most frequent particle size of ∼4 nm. However, the image in Fig. S40† presented a high degree of uncertainty. 100%Mg2Ni (Fig. 8(d)) presented particle sizes of 20–50 nm. In the case of the hydrided 90%Mg2Ni-CNF and 100%Mg2Ni, the determination of particle size became more complex. We attributed the reduction and lack of CNF, respectively, as a factor reducing the ability to keep the nanoparticles fixed during their preparation for TEM imaging. The role played by the CNF can be established as a support, confinement, and spacer of particles. The other roles of carbon additives are hydrogen diffusers and heat-conducting materials, where both effects improve the hydrogen storage capabilities of hydrogen storage materials.17,54
Fig. 9 presents the X-ray diffraction characterization of the hydrided materials. From the bottom to top, Fig. 9(a) presents the ball-milled and hydrided Mg2Ni, which presents a combination of low- and high-temperature phases of Mg2NiH4 (all the peaks labeled as Mg2NiH4). Also, the presence of unreacted Ni was observed. Ni particles were observed in the SEM image in Fig. 1(e); however, only after heating in hydrogen, Ni was sintered and presented diffraction peaks. No indications of crystalline Mg or MgH2 were observed. The XRD pattern of the ball-milled and hydrided 75%Mg2Ni-CNF-MM was consistent with the partial hydriding observed in the PCT experiments. In the case of the nanosized and hydrided materials (Fig. 9(b)–(e)), an increase in the peak located at the 2θ value of 29.37° can be observed. In addition to this peak, the hydrided 100%Mg2Ni presented a series of other minor peaks. All these peaks are labeled “unknown” because they do not correspond to any of the multiple known phases of Mg2NiH4; however, these peaks are close to some of the expected diffraction peaks of the low-temperature phase of Mg2NiH4.55
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Fig. 9 X-ray diffraction characterization of hydrided materials: (a) 75%Mg2Ni-CNF-MM-PCT300, (b) 50%Mg2Ni-CNF-PCT-300, (c) 75%Mg2Ni-CNF-PCT-300, (d) 90%Mg2Ni-CNF-PCT-300, and (e) 100%Mg2Ni-PCT-300. |
Fig. 10 presents the XPS signal of the PCT hydrided materials. Fig. 10(a) presents the C 1s edge, where in comparison with the as-prepared materials of Fig. 4(a), the PCT hydrided materials presented more peaks and complex fitting. The XPS of the hydrided materials present the common C–C peaks at 284.7–284.8 eV (red deconvoluted peaks). The additional peaks are as follows: (i) C–H at 285.4–285.7 eV (blue deconvoluted peaks).33 (ii) Small peaks at 281.7–283.1 eV in 75% to 100%Mg2Ni -PCT 300 materials, which can be ascribed to the presence of disordered (amorphous) C.56,57 (iii) The coexistence of small peaks at 290–288 eV, which can be interpreted as C–O interactions.33 Very interestingly, a small peak appeared at 283.9 eV (dark-red deconvoluted peak for the 75%Mg2Ni-CNF PCT-300 material), which can be related to C bonded with Ni in Ni3C.56,57
Fig. 10(b) presents the Mg 2p XPS spectra of the hydrided materials. The main peak (red or purple for accumulative single peak) is located at 50.7, 50.1, 50.4, and 50.2 eV for 50%Mg2Ni-CNF-PCT-300, 75%Mg2Ni-CNF-PCT-300, 90%Mg2Ni-CNF-PCT-300, and 100%Mg2Ni-PCT-300, respectively. Interestingly, the 75%Mg2Ni-CNF-PCT-300 material presented a clear shift to a lower binding energy compared to the as-prepared material (i.e. 50.7 eV) (Fig. 4(b) to 50.1 eV). This small shift can be related to the formation of Mg2NiH4. Also, the appearance of a peak at 49.8 eV is very interesting for the 100%Mg2Ni-PCT-300 material, which can be related to the presence of metallic Mg. The as-prepared material also presented this peak but with a higher relative intensity. The reduction in the relative intensity of the metallic Mg peak in the hydrided material can be explained by the formation of Mg2NiH4 upon heating in hydrogen, which consumed some of the Mg observed in the first stage of preparation of the particles. Additionally, 50%Mg2Ni-CNF-PCT-300 presented a prominent peak at 52.1 eV (orange deconvoluted peak), which shifted to a too high binding energy to be considered MgO. M. Ramachandran et al. reported a similar peak at 52.3 eV as Mg2C3; however, as mentioned by them, no XPS reference (standard) for Mg2C3 exists.58
Fig. 10(c) presents the Ni 2p XPS spectra of the hydrided materials. Similar to the as-prepared materials, the signal is dominated by the 2p3/2 peaks together with the presence of 2p1/2 and satellite peaks. Unlike the as-prepared materials, the hydrided materials stood out due to the presence of a new peak (red deconvoluted peak) located between 852.8 eV and 852.9 eV. The Ni main peak of the Mg2Ni was reported to be located at 852.6 eV.35 The small shift to higher binding energies can be related to the formation of the hydrided form of Mg2Ni. The XPS spectrum of 75%Mg2Ni-CNF-PCT-300 was not suitable for deconvolution but its characteristics indicate that its main peak is consistent with the formation of Mg2NiH4. The other deconvoluted peaks of the main 2p3/2 signal (orange peaks) are located at 856 eV, 855.5 eV, and 855.7 eV for 50%Mg2Ni-CNF-PCT-300, 90%Mg2Ni-CNF-PCT-300, and 100%Mg2Ni-PCT-300, respectively. The origin of these peaks can be related to the presence of unreacted NiCp2 or decomposition of the intermediates. Finally, Fig. 10(d) presents the O 1s peaks of the hydrided materials. All these spectra have in a common peak between 531.5–532.2 eV, corresponding to the usual surface oxygen. An additional peak at 532.5 eV improved the fitting of the 75%Mg2Ni-CNF-PCT-300 material. This peak can also be related to other surface oxygen species rather than the formation of metallic oxides. As a brief general conclusion of the characterization of the as-prepared and hydrided materials by XPS, this technique revealed the complexity of the intermediates and by-products, which are most probably amorphous or present in low concentration and can intervene in the decomposition of the precursors and the hydriding reactions. For example, several metal carbides have been used as catalysts of MgH2 and Mg2NiH4 in the field of hydrogen storage.59,60 Similar effects can occur in the materials reported here.
As a remark on the synthesis and characterization findings, we can mention that the formation of Mg2Ni nanoparticles supported in the CNF can be interesting for hydrogen storage. However, the principal observed limitation is the difficulty of dehydriding. Alternatively, the reversibility observed for the ball-milled 75%Mg2Ni-CNF-MM may be related to the presence of Ni and other species, which can work as a catalyst. Further research must be done to explore the use of catalysts and other supporting materials for improving dehydriding. Developing hydrogen storage materials must be optimized in future to enhance the performance of actual hydrogen storage methods.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4nr01725k |
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