First-principles investigation of the effects of Ni and Y co-doped on destabilized MgH2

Gaili Sunab, Yuanyuan Lib, Xinxin Zhaoa, Jianbao Wua, Lili Wang*a and Yiming Mi*ab
aCollege of Fundamental Studies, Shanghai University of Engineering Science, Shanghai 201620, China. E-mail: llwang@sues.edu.cn; yimingmi@sues.edu.cn
bCollege of Chemistry and Chemical Engineering, Shanghai University of Engineering Science, Shanghai 201620, China

Received 13th November 2015 , Accepted 15th February 2016

First published on 15th February 2016


Abstract

The Ni and Y co-doping effect on the structural stabilities and dehydrogenation properties of destabilized MgH2 was studied by first-principles calculations. Ni and Y dopants prefer to occupy the Mg3 and Mg2 positions due to the minimal total electronic energy. The formation enthalpy was used to evaluate the stability of the doped MgH2 systems. Most Ni and Y co-doped MgH2 systems are more stable than Ni single-doping. In particular, the case of x = 20% (Mg8Ni8Y2H36) exhibits the highest stability. During the dehydrogenation process, the Ni and Y co-doped MgH2 system possesses promising dehydrogenation properties compared with pure Ni doping, which can be attributed to the relatively lower hydrogen desorption enthalpies. The electronic structures show that hybridization of the dopants with Mg and H atoms can strongly weaken the Mg–H interactions, which effectively improve the dehydrogenation properties of the Ni and Y co-doped MgH2 system.


1. Introduction

Metal hydrides with a high hydrogen storage capacity and demonstrated cycling capability,1–4 are considered to be some of the most promising hydrogen storage media for automotive applications. Among these hydrogen storage materials, magnesium hydride (MgH2) has been investigated extensively in the last two decades due to its high hydrogen storage capacity of 7.6 wt% and good reversibility,5–7 together with the cheap cost and light weight of magnesium.8,9 Unfortunately two technical obstacles limit the practical application of MgH2: (i) the high thermodynamic stability, which is responsible for the high dehydrogenation temperature requirement of 573 K at 1 bar H2.10,11 (ii) The poor kinetics in the hydrogenation and dehydrogenation reaction, which can be attributed to the low dissociation rate of H2 on the metallic Mg surface, strong Mg–H bonding in magnesium hydride, and slow hydrogen diffusion ability in MgH2.10–12

To overcome these limitations in MgH2, various efforts have been made in the design of Mg-based hydrogen storage materials. On the one hand, reducing the gain size is an effective way to improve the thermodynamic behavior of MgH2 by shortening the diffusion length, introducing defects and increasing the surface areas.13,14 Theoretical calculations predicted that the reaction enthalpy of MgH2 nanoparticles is reduced compared with the bulk material only when the particles are smaller than 2 nm and contain <50 Mg atoms.15,16 However, this property is not straightforward for practical applications because it is extremely difficult to prepare nanoparticles of this size and keep the stabilities of these nanoparticles after repeated hydrogenation/dehydrogenation cycles.17 On the other hand, introducing catalysts such as transition metals and transition metal oxides will improve the hydrogen adsorption/desorption kinetics and thermodynamic properties of MgH2. It has been revealed that doping MgH2 with transition metals can improve its hydrogen adsorption/desorption kinetics as well as its thermodynamic properties. Many transition metals (TM) such as Ni, Ti, V, Zr, Fe, Ru, Co, Y, Rh, Pd, Cu, Ag and Nb, have been used as additives for MgH2.18–24 Ren et al. found that the V dopant can significantly reduce the dehydrogenation temperature and improve the kinetics of MgH2.20 Computational studies by Takahashi et al. used density functional theory (DFT) to investigate the hydrogenation and dehydrogenation mechanism of Nb, NbO and Nb2O5 doped on MgH2, and found that these dopants have a significant catalytic effect on the dehydrogenation of MgH2.21,22 Dai et al. carried out first principles calculations based on DFT to show that Ni can improve the dehydrogenation properties of MgH2 by the weakened Mg–H bond.10 Very recently, Hudson et al. discovered that graphene decorated Fe clusters dramatically improved the kinetics of MgH2, and they showed that non-transition metals like graphene can be used as a catalyst for the MgH2 system.24

Previous studies25–28 demonstrated that multiple transition metal additions generally have a better effect in improving the hydrogenation performance of MgH2 than addition of a single transition metal. It was found that co-doped MgH2 showed excellent hydrogen absorption/desorption kinetics, especially in the latter process, since it reduced the activation energies of both processes and weakened the Mg–H bonds. Zaluska et al. reported that the best storage kinetic results are contributed by a combination of the transition metals, such as V + Zr or Mn + Zr.25 Another promising material is the Mg–Ni–Y alloy, which can reach an invertible hydrogen storage capacity of up to 5.3 wt% H2. The rates of hydrogenation and dehydrogenation are up to 1 wt% H per min at a temperature of 250 °C, with a remaining nanocrystalline structure even after several cycles of H2 uptake and release.26 Li et al. investigated Mg alloyed 20 wt% Ni–Y and observed high gravimetric hydrogen storage densities and excellent hydrogen sorption kinetics. At 293 K and 473 K under 3.0 MPa H2, it can absorb 4.16 and 5.59 wt% hydrogen, respectively. It can also desorb 4.75 wt% hydrogen in 15 min at 573 K under 0.1 MPa H2.27 Zhou et al. observed that Al and Y co-doped MgH2 can weaken Mg–H bonds and promote hydrogen dissociation and desorption.28 Moreover, the exact mechanism of Ni combined with Y as a catalyst in the enhancement of hydrogen storage properties of MgH2 is not completely understood. Therefore, it is necessary to develop a systematic investigation of the synergistic effects of Ni with Y on improving the hydrogen storage properties of MgH2.

In this paper we performed a systematic study on the collaborative effects of Ni and Y co-doped with destabilized MgH2 using first-principles calculations. The preferential sites of Ni and Y dopants on MgH2 were determined by the lowest total electronic energy. The formation enthalpies and hydrogen desorption enthalpies were used to study the dopants’ influence on the structural stability and dehydrogenation properties of MgH2. Electronic structures were analyzed to identify the intrinsic mechanisms of the dopants’ influence on the bonding and dehydrogenation properties of the destabilized MgH2 matrix.

2. Computational methods

Energy and electronic structure calculations were performed under the framework of density functional theory (DFT) via the Vienna Ab initio Simulation Package (VASP) code.29,30 The projector augmented wave (PAW) method was used to spin out the valence electron density; the generalized gradient approximation (GGA) in the scheme of Perdew–Wang 91 (PW91) was adopted for the exchange–correlation functional.31,32 For the plane wave basis set a cutoff energy of 350 eV was used throughout. The model of the co-doped MgH2 with Ni and Y was simulated by 3 × 3 × 1 and 3 × 3 × 3 supercells. The Brillouin-zone samples were 3 × 3 × 7 and 3 × 3 × 3 Monkhorst–Pack k-point meshes for the supercells above, respectively. The electronic structures were defined as self-consistent if the differences between two consecutive energies and forces were less than 10−7 eV and 0.01 eV Å−1.

3. Results and discussion

3.1. Calculation models and site preference

MgH2 has a tetragonal structure (P42/mnm, group no. 136) with experimentally measured lattice parameters of a = 4.501 Å and c = 3.010 Å.30 Two Mg atoms occupy the 2a (0, 0, 0) site and four H atoms occupy the 4f (0.303, 0.303, 0) site. In a previous work, we calculated that the lattice parameters for a unit cell of MgH2 are a = 4.477 Å and c = 2.989 Å, which are very close to the experimental34 and other theoretical results.33,35,36 The model of MgH2 was built from a 3 × 3 × 1 supercell and computed using those bulk parameters. The 3 × 3 × 1 supercell (see Fig. 1) contained a total of 54 atoms with four non-equivalent positions for Mg and six non-equivalent positions for H. The optimal atomic positions of Mg and H atoms are in good agreement with the theoretical data.28
image file: c5ra23996f-f1.tif
Fig. 1 Top (a) and side (b) views of the MgH2 3 × 3 × 1 supercell model. Mg1, Mg2, Mg3 and Mg4 denote the four non-equivalent positions for Mg, respectively.

In order to find the optimum geometry and doping sites of dopants (Ni and Y) in MgH2, each of the four non-equivalent positions of Mg were substituted by Ni in order. The calculated total electronic energies of the Ni doped system are shown in Fig. 2(a). These results suggest that the Ni atom prefers to stay in the Mg3 position, due to the minimal total electronic energy. The new compounds are denoted as (Mg, Ni)H2. Then, Mg is substituted by Y in the other three non-equivalent positions (Mg1, Mg2 and Mg4) of the (Mg, Ni)H2 compound. The calculated total electronic energies are shown in Fig. 2(b). The Y atom is likely to substitute in the Mg2 position due to its lowest total electronic energy. The new compounds are denoted as (Mg, Ni, Y)H2. Adopting the same method, we also calculate the total electronic energies of different doping sites of dopants (Ni and Y) in the MgH2 3 × 3 × 3 supercell. The calculated total electronic energies of these doping systems are shown in Fig. 2(c) and (d). Ni and Y prefer to occupy the Mg3 and Mg2 positions in the 3 × 3 × 3 supercell, respectively. The calculated results of the 3 × 3 × 3 supercell are consistent with the results of the 3 × 3 × 1 supercell; we have chosen the latter results in the following calculations due to the 3 × 3 × 1 supercell model having a higher calculation efficiency.


image file: c5ra23996f-f2.tif
Fig. 2 The total electronic energy for: (a) doping MgH2 (3 × 3 × 1 supercell) with Ni in four non-equivalent positions of Mg; (b) doping (Mg, Ni)H2 (3 × 3 × 1 supercell) with Y in the other non-equivalent positions of Mg; (c) doping MgH2 (3 × 3 × 3 supercell) with Ni in four non-equivalent positions of Mg; (d) doping (Mg, Ni)H2 (3 × 3 × 3 supercell) with Y in the other non-equivalent positions of Mg.

In order to systematically investigate the role of Ni and Y co-doping on the structural stability of MgH2, we studied the substitution of Mg2 by Y in different doping concentrations. We chose eight doping concentrations of x = 0, 10%, 13%, 20%, 27%, 30%, 33% or 40% in (Mg, Ni)H2, which meant substituting n = 0, 1, 1.3, 2, 2.7, 3, 3.3 or 4 out of 10 Mg atoms in Mg10−nNi8YnH36. For the case of 1.3, 2.7 or 3.3 out of 10 Mg atoms in Mg10−nNi8YnH36, we performed an equivalent treatment by replacing 4, 8 or 10 of 30 Mg atoms in the (Mg, Ni)H2 (3 × 3 × 3) supercell to achieve the doping level of x = 13%, 27% or 33% in (Mg, Ni)H2. The chosen method of preferential positions in different concentrations is consistent with that used in the former.

The favorability of single-doping and co-doping in MgH2 can be identified by the substitution energies (Esub), which were calculated via the following definition:37–39

 
Esub = 1/54[Et(Mg10−nNi8MnH36) − Et(Mg18H36) − 8Eb(Ni) − nEb(Y) + (8 + n)Eb(Mg)] (1)
where Et(M) refers to the total energies of hydrides in the supercells. Eb represents the total energies per atom in the bulk structure. The obtained substitution energies of the doped materials with different Y concentrations are presented in Fig. 3. It can be seen that Ni and Y co-doped MgH2 systems have a lower substitution energy value compared with the Ni single doped system, except for the doping concentrations of x = 10% (Mg9Ni8YH36) and 33% (Mg6.8Ni8Y3.3H36). Compared with the Ni single-doped system, the substitution energy of Mg9Ni8YH36 and Mg6.8Ni8Y3.3H36 are slightly increased by about 2.6% and 2.9%, respectively. Furthermore, the lowest substitution energy value is located at a doping concentration of x = 20% (Mg8Ni8Y2H36), which is lower than that of the Ni single-doping by 65.9%. From an energy point of view, the smaller substitution energy corresponds to a more favorable substitution doping. Hence, most of the co-doping of Ni and Y into MgH2 is more energetically favorable than the single-doping. In particular, x = 20% (Mg8Ni8Y2H36) is the most energetically favorable doping.


image file: c5ra23996f-f3.tif
Fig. 3 The calculated substitutional energies (Esub) of the doped hydrides with different Y concentrations of x = 0, 10%, 13%, 20%, 27%, 30%, 33% or 40%.

3.2. Stability and dehydrogenation properties

Commonly, the structural stability of a crystal can be evaluated by its formation enthalpy ΔHform. A negative formation enthalpy indicates that the crystal can exist stably. Besides, a lower formation enthalpy suggests a stronger stability.40 In order to investigate the stability of Ni and Y doping on the MgH2 system, the formation enthalpies ΔHform are calculated by using eqn (2):28,40,41
 
ΔHform = 1/54[Et(Mg10−nNi8YnH36) − 8Es(Ni) − nEb(Y) − (10 − n)Eb(Mg) − 18E(H2)] (2)
where Et(M) refers to the total energies of hydrides in supercells. Eb represents the total energies per atom in the bulk structure. The total energy of the free H2 molecule, E(H2), was computed as −6.77 eV using a 8 Å3 cubic cell, consistent with other theoretical results.28,47 The calculated formation enthalpy of the doped hydrides with different Y concentrations are presented in Fig. 4. The formation enthalpies of these eight compounds are all found to be negative, which indicates they can exist stably. Ni and Y co-doped MgH2 systems have a lower formation enthalpy value compared with the Ni single-doped system, except for the doping concentrations of x = 10% (Mg9Ni8YH36) and 33% (Mg6.8Ni8Y3.3H36). Compared with the Ni single-doped system, the formation enthalpy of Mg9Ni8YH36 and Mg6.8Ni8Y3.3H36 are increased by about 6.5% and 17.8%, respectively. Furthermore, x = 20% (Mg8Ni8Y2H36) has the lowest enthalpy value, which is lower than that of Ni single-doping by 172.6%. This trend is consistent with the calculated results of the substitution energy. Hence, the doping of Ni combined with Y into MgH2 exhibits a higher stability than Ni single-doping. In particular, the doping concentration of x = 20% (Mg8Ni8Y2H36) exhibits the highest stability.

image file: c5ra23996f-f4.tif
Fig. 4 The calculated formation enthalpies (ΔHform) of the doped hydrides with different Y concentrations of x = 0, 10%, 13%, 20%, 27%, 30%, 33% or 40%.

From the investigation of the substitution energy and the formation enthalpy above, Mg8Ni8Y2H36 is more energetically favorable than other co-doped compounds. Therefore, for the dehydrogenation property and bond and electronic structure of the Ni and Y co-doped system, we are going to investigate the Y doping concentration of x = 20% (Mg8Ni8Y2H36) for the co-doped systems, compared to the Ni single-doping case.

In order to further assess the dehydrogenation abilities of these hydrides, their hydrogen desorption enthalpies, ΔHdes, are calculated by using eqn (3):42,43

 
ΔHdes = [Et(Mg10−nNi8YnH35) + 1/2E(H2)] − Et(Mg10−nNi8YnH36) (3)
where Et(Mg18−nNi8YnH36) represents the total energy of hydrides. Et(Mg10−nNi8YnH35) refers to a pseudostructure in which one H atom is removed from the relaxed Et(Mg18−nNi8YnH36) system. E(H2) is the same as that used in eqn (2).

The obtained hydrogen desorption enthalpy (ΔHdes) in single-doped MgH2 with Ni is 0.71 eV. This enthalpy value is lower than the result in ref. 10, which may be ascribed to the higher dopant content here. Moreover, compared to ΔHdes = 1.5335 eV for pure MgH2,44,45 the hydrogen desorption enthalpy of the single-doped MgH2 system is decreased. After Ni doping, the lower hydrogen desorption enthalpy of the doped MgH2 system leads to an improvement of its dehydrogenation properties. For the best Ni and Y co-doped MgH2 system, the hydrogen desorption enthalpies when moving out one H atom from each of the six non-equivalent positions of the co-doped system are all calculated. The obtained hydrogen desorption enthalpies (ΔHdes) are presented in Fig. 5. It can be observed that the hydrogen desorption enthalpies of the hydride are all significantly decreased in comparison with the Ni single-doped and pure MgH2 systems. Thus, each hydrogen desorption is much easier than in the single-doped case, which indicates that the Ni and Y co-doped system exhibits excellent dehydrogenation properties. Besides, some of the hydrogen desorption enthalpies of the Ni and Y co-doped MgH2 system are lower than those obtained when alloying MgH2 with other catalysts.21,24,28 Based on the calculated results we can conclude that co-doping MgH2 with Ni and Y not only enhances the structural stability of MgH2, but is also beneficial for the improvement of the dehydrogenation properties of MgH2. Although the partial substitution of Mg by Ni and Y has significant synergetic effects on MgH2, a detailed understanding of the influence of dopants on the hydrogen desorption process and kinetics of MgH2 requires further investigation, which will be the subject of our future work.


image file: c5ra23996f-f5.tif
Fig. 5 The calculated hydrogen desorption enthalpies (ΔHdes) when moving out one H atom (H1–H6) for the Y doping concentration of x = 20% (Mg8Ni8Y2H36) in (Mg, Ni)H2.

3.3. Bonding analysis

Table 1 lists the bond distances between metallic elements in undoped and doped MgH2. For undoped MgH2, the bond length of Mg–Mg ranges from 3.50 Å to 4.48 Å with an average length of 3.66 Å. For the Ni single-doped MgH2 system, Mg2 and Mg4 are the nearest neighboring metallic atoms of the dopant Ni and the Mg–Ni bonds are decreased by an average of 3.90 Å. Discounting the radius difference, the bond length of Mg–Ni is longer than the original Mg–Mg, which implies that the Mg–Ni bond is weakened. But the bond length of Mg–Mg is decreased, thus the strength of the Mg–Mg bond is enhanced compared with pure MgH2. For the best co-doped case of Mg8Ni8Y2H36, discounting the radius difference, the distances between the Mg and Ni atoms are decreased in comparison with that of the single-doped system, which indicates that the bond strengths are strengthened. Furthermore, the lengths of the Mg–Y bond and the Y–Ni bond are shorter than the Ni-doped system, thus the bond strengths of Mg–Y and Y–Ni are enhanced. Thus it can be inferred that the dopant Y has a strong alloying trend with the Mg and Ni atoms, which weakens the strength of the Mg–H and Ni–H bonds.
Table 1 Calculated bond distances (Å) between metallic elements in the hydrides
MgH2 Mg1–Mg2 Mg1–Mg3 Mg1–Mg4 Mg2–Mg3 Mg2–Mg4 Mg3–Mg4
3.50 4.48 3.50 3.50 3.50 3.50
Mg10Ni8H36 Mg1–Mg2 Mg1–Ni Mg1–Mg4 Mg2–Ni Mg2–Mg4 Ni–Mg4
3.28 4.34 3.28 3.46 3.21 3.31
Mg8Ni8Y2H36 Mg1–Mg2 Mg1–Ni Mg1–Mg4 Mg2–Ni Mg2–Mg4 Ni–Mg4
3.87 3.81 3.25 3.07 3.13 3.04
Mg1–Y     Y–Ni Y–Mg4  
3.36     3.09 3.40  


Table 2 lists the interaction of metallic and H atoms in undoped and doped MgH2. In this calculation, the bond length of Mg–H ranges from 1.93 Å to 1.94 Å with an average length of 1.93 Å, consistent with the experimental34 and other theoretical results.35,36 For the Ni single-doped MgH2 system, H4, H5 and H6 atoms are the nearest neighboring atoms of the dopant Ni and these atoms move towards Ni, thus the bond lengths of Mg–H (H4–H6) are increased. Meanwhile, the Mg–H (H5, H6) bond lengths are also increased. Hence, the bond strength of Mg–H is weakened. For Ni and Y co-doped MgH2 (Mg8Ni8Y2H36), the nearest neighboring H (H4–H5) atoms of Ni further move towards the Ni, thus the Mg–H (H4–H5) bonds further weaken their strength. However the Ni–H6 bond is a little bit weakened. H1, H3 and H6 atoms are the nearest neighboring atoms of the dopant Y, in comparison with the single-doped system the bond length of Y–H (H1–H6) is markedly increased. The length of the Mg–H bonds are all increased, which means that the strength of the Mg–H bonds are all weakened. Therefore, the dopant Y can further weaken the Mg–H bond.

Table 2 Calculated bond distances (Å) between the metallic and H atoms in the hydrides
Mg10Ni8H36 Mg1–H1 1.80 Mg2–H1 1.84 Ni–H4-1 1.78 Mg4–H2 1.79
Mg1–H2 1.84 Mg2–H3 1.80 Ni–H4-2 1.62 Mg4–H3 1.77
  Mg2–H6 2.25 Ni–H5 1.66 Mg4–H5 1.95
  Mg2–H1 3.46 Ni–H6 1.68  
Mg8Ni8Y2H36 Mg1–H1 1.83 Mg2–H3 1.88 Ni–H4-1 1.72 Mg4–H2 2.00
Mg1–H2 1.91 Mg2–H6 2.30 Ni–H4-2 1.62 Mg4–H3 1.83
  Y–H1 2.16 Ni–H5 1.59 Mg4–H5 1.99
  Y–H3 2.11 Ni–H6 1.70  
  Y–H6 2.45    


3.4. Electronic structure

Fig. 6(a) shows the total and partial density of states (DOS) of undoped MgH2. The Fermi energy (EF) level is set at zero. The gap between the valence band (VB) and conduction band (CB) is about 4 eV, in good agreement with other calculation results.28,46 The relatively large gap value of the bulk leads to a relatively high formation energy. The VB is mainly dominated by H s states and the CB mainly by Mg s and Mg p states. Analyzing the partial DOS curves, these correspond to the strong ionic bonding interactions between Mg and H atoms. By using the Bader charge analysis in molecule AIM theory,47–49 it is found that the average electron number of the Mg and H atoms is 0.42 and 1.79, respectively, as shown in Table 3. The ionic charges of Mg and H can be represented as Mg1.58+ and H0.79−, indicating the strong ionic character of the Mg–H bond.
image file: c5ra23996f-f6.tif
Fig. 6 Total and partial densities of states (DOS) of (a) undoped MgH2; (b) Mg10Ni8H36; (c) Mg8Ni8Y2H36.
Table 3 Bader charges for undoped and doped MgH2 systems
MgH2 Mg1 Mg2 Mg3 Mg4    
0.43 0.42 0.42 0.42    
H1 H2 H3 H4 H5 H6
1.79 1.79 1.79 1.80 1.79 1.79
Mg10Ni8H36 Mg1 Mg2 Ni Mg4    
0.44 0.41 9.63 0.43    
H1 H2 H3 H4 H5 H6
1.79 1.78 1.81 1.22 1.61 1.32
Mg8Ni8Y2H36 Mg1 Mg2 Y Ni Mg4  
0.44 0.39 9.33 9.66 0.43  
H1 H2 H3 H4 H5 H6
1.76 1.79 1.75 1.23 1.62 1.33


Fig. 6(b) shows the total and partial DOS of the Ni single-doped MgH2 system. In order to plot the partial DOS of all atoms in the same panel with the same scale, the amplitude of the partial DOS of the Ni d orbital was decreased by 10. The total DOS curve shows a remarkable decrease in the band gap of 0 eV, which show clearly metallic characteristics. It can be obviously seen that the Ni d states insert in the middle part and then overlap with the Mg p and H s orbitals separately in a different energy region. The electrons in the Mg p and H s hybridization states are pushed to the Mg p, Ni d and H s hybridization states. The interactions of the Mg–H bond in these regions are weakened. Furthermore, the H s orbitals distributed in the region of −5.5 to −3.1 eV are less overlapped with the Mg s and p orbitals compared to the pure MgH2, which can help to weaken the hybridization of the Mg–H bond. This interpretation is also supported by the Bader charge data. As shown in Table 3, the Bader charges on H (H4–H6) atoms decrease significantly and the Bader charges on Mg (Mg1, Mg4) increase slightly after Ni-doping. Therefore, the electron transfer from H to Mg is obviously weakened.

Fig. 6(c) shows the total and partial DOS of the Ni and Y co-doped MgH2 system; this case corresponds to a Y doping concentration of x = 20% (Mg8Ni8Y2H36). In order to plot the partial DOS of all atoms in the same panel with the same scale, the amplitude of the partial DOS of Ni d and Y d orbitals were decreased by 10 and 5, respectively. The main peaks of the co-doped system slightly move away from the Fermi energy compared with the Ni single-doped MgH2, implying a higher stability of the Ni and Y co-doped system. The Y p and d orbitals overlap with H s, Mg p, and Ni p and d orbitals in the energy region of −6.0 to −2.6 eV. Also, the distributions of the bonding peaks of Y d orbitals are mainly concentrated in the energy region of 1.2 to 5.1 eV and overlap well with the Mg s and p orbitals. These behaviors indicate that the Y atom has a strong bonding interaction with H, Mg and Ni atoms and decreases the Mg–H p–s mixing. In addition, the drop in magnitude of the bonding peaks of H s and Mg s and p orbitals is more than that of the Ni single-doping, which means that the Mg–H bond is further weakened in the co-doped system. Similar to the Ni single-doped system, this interpretation is also supported by the Bader charge data. The number of electrons around H (H1, H3) atoms in the co-doped system is decreased compared with Ni single-doped MgH2, which implies that the electron transfer from H to Mg is further weakened. Thus, the Mg–H hybridizations are significantly weakened by Ni and Y co-doping.

4. Conclusion

In summary, first-principles calculations were preformed to study the structural stabilities and dehydrogenation properties of destabilized MgH2 co-doped with Ni and Y. According to the minimal total electronic energy, the Ni and Y prefer to substitute in the Mg3 and Mg2 position, respectively. The substitution energies and formation enthalpies of different Y doping concentrations of hydrides were estimated. They show that most of the Ni and Y co-doped MgH2 systems are more stable than Ni single-doping. Especially, the Y doping concentration of x = 20% (Mg8Ni8Y2H36) has the most energetic stability. Moreover, these calculations also give insight into the hydrogen desorption enthalpies (ΔHdes) of this cases. The Ni and Y co-doped MgH2 system has the lowest ΔHdes value of 0.11 eV. Due to the relatively lower hydrogen desorption enthalpy, the Ni and Y co-doped MgH2 system possesses promising dehydrogenation properties. The electronic structures show that the hybridization of dopants with Mg and H atoms together weaken the Mg–H interaction. The electronic structures further demonstrate that the Mg–H bonds are more susceptible to dissociation by Ni and Y co-doping because of the reduced magnitude of the Mg–H hybridization peaks. Therefore, co-doping with Ni and Y effectively improves the dehydrogenation properties of destabilized MgH2.

Acknowledgements

The work was supported by the National Natural Science Fund (No. 11504228) and the Graduated Innovative Research Project of Shanghai University of Engineering Science (No. E1-0903-14-01107-14KY0411).

References

  1. S. Q. Hao and D. S. Sholl, J. Phys. Chem. C, 2012, 116, 2045–2050 CrossRef CAS.
  2. J. J. Tang, X. B. Yang, L. J. Chen and Y. J. Zhao, AIP Adv., 2014, 4, 077101 CrossRef.
  3. J. H. Dai, Y. Song and R. Yang, J. Phys. Chem. C, 2010, 114, 11328–11334 CrossRef CAS.
  4. Y. Zhong, H. Zhu, L. L. Shaw and R. Ramprasad, J. Phys. Chem. C, 2010, 114, 21801–21807 CrossRef CAS.
  5. D. Meggiolaro, G. Gigli, A. Paolone, F. Vitucci and S. Brutti, J. Phys. Chem. C, 2013, 117, 22467–22477 CrossRef CAS.
  6. M. Ismail, N. Juahir and N. S. Mustafa, J. Phys. Chem. C, 2014, 118, 18878–18883 CrossRef CAS.
  7. S. Q. Hao and D. S. Sholl, J. Phys. Chem. Lett., 2010, 1, 2968–2973 CrossRef CAS.
  8. T. Jiang, L. X. Sun and W. X. Li, Phys. Rev. B: Condens. Matter Mater. Phys., 2010, 81, 035416 CrossRef.
  9. Q. Wan, P. Li, J. W. Shan, F. Q. Zhai, Z. L. Li and X. H. Qu, J. Phys. Chem. C, 2015, 119, 2925–2934 CrossRef CAS.
  10. J. H. Dai, Y. Song and R. Yang, J. Phys. Chem. C, 2010, 114, 11328–11334 CrossRef CAS.
  11. J. Zhang, D. W. Zhou, P. Peng and J. S. Liu, Phys. B, 2008, 403, 4217–4223 CrossRef CAS.
  12. J. J. Tang, X. B. Yang, M. Chen, M. Zhu and Y. J. Zhao, J. Phys. Chem. C, 2012, 116, 14943–14949 CrossRef CAS.
  13. M. Chen, X. B. Yang, J. Cui, J. J. Tang, L. Y. Gan, M. Zhou and Y. J. Zhao, Int. J. Hydrogen Energy, 2012, 37, 309–317 CrossRef CAS.
  14. J. J. Liu, J. Tyrrell, L. Cheng and Q. F. Ge, J. Phys. Chem. C, 2013, 117, 8099–8104 CrossRef CAS.
  15. R. W. Wagemans, J. H. van Lenthe, P. E. de Jongh, A. Josvan Dillen and K. P. de Jong, J. Am. Chem. Soc., 2005, 127, 16675–16680 CrossRef CAS PubMed.
  16. K. C. Kim, B. Dai, J. K. Johnson and D. S. Sholl, Nanotechnology, 2009, 20, 204001 CrossRef PubMed.
  17. S. Cheung, W. Q. Deng, A. C. T. van Duin and W. A. Goddard, J. Phys. Chem. A, 2005, 109, 851–859 CrossRef CAS PubMed.
  18. H. C. Wang, D. H. Wu, L. T. Wei and B. Y. Tang, J. Phys. Chem. C, 2014, 118, 13607–13616 CrossRef CAS.
  19. M. Pozzo and D. Alfè, Int. J. Hydrogen Energy, 2009, 34, 1922–1930 CrossRef CAS.
  20. C. Ren, Z. Z. Fang, C. S. Zhou, J. Lu, Y. Ren and X. Y. Zhang, J. Phys. Chem. C, 2014, 118, 21778–21784 CrossRef CAS.
  21. K. Takahashi, S. Isobe and S. Ohnuki, J. Alloys Compd., 2013, 58, S25–S28 CrossRef.
  22. K. Takahashi, S. Isobe and S. Ohnuki, Langmuir, 2013, 29, 12059–12065 CrossRef CAS PubMed.
  23. Y. Mina, H. W. Hanno and Z. Y. Zhang, Phys. Rev. B: Condens. Matter Mater. Phys., 2011, 83, 045413 CrossRef.
  24. M. S. L. Hudson, K. Takahashi, A. Ramesh, S. Awasthi, A. K. Ghosh, P. Ravindran and O. N. Srivastava, Catal. Sci. Technol., 2015, 6, 261–268 Search PubMed.
  25. A. Zaluska, L. Zaluski and J. O. Strom-Olsen, J. Alloys Compd., 1999, 288, 217–225 CrossRef CAS.
  26. S. Kalinichenkaa, L. Röntzschb and B. Kiebacka, Int. J. Hydrogen Energy, 2009, 34, 7749–7755 CrossRef.
  27. Z. N. Li, X. P. Liu, L. J. Jiang and S. M. Wang, Int. J. Hydrogen Energy, 2007, 32, 1869–1874 CrossRef CAS.
  28. S. C. Zhou, R. K. Pan, T. P. Luo, D. H. Wu, L. T. Wei and B. Y. Tang, Int. J. Hydrogen Energy, 2014, 39, 9254–9261 CrossRef CAS.
  29. G. Kresse and J. Hafner, Phys. Rev. B: Condens. Matter Mater. Phys., 1993, 47, 558–561 CrossRef CAS.
  30. G. Kresse and J. Furthmüler, Phys. Rev. B: Condens. Matter Mater. Phys., 1996, 54, 11169–11187 CrossRef CAS.
  31. P. E. Blöchl, Phys. Rev. B: Condens. Matter Mater. Phys., 1994, 50, 17953–17979 CrossRef.
  32. J. P. Perdew and Y. Wang, Phys. Rev. B: Condens. Matter Mater. Phys., 1992, 45, 13244–13249 CrossRef.
  33. E. Callini, L. Pasquini, T. R. Jensen and E. Bonetti, Int. J. Hydrogen Energy, 2013, 38, 12207–12212 CrossRef CAS.
  34. S. Ono, Y. Ishido, K. Imanari, T. Tabata, Y. Cho and R. Yamamoto, J. Less-Common Met., 1982, 88, 57–61 CrossRef CAS.
  35. Y. Bouhadda, A. Rabehi and S. Bezzari-Tahar-Chaouche, Journal des Energies Renouvelables, 2007, 10, 545–550 Search PubMed.
  36. M. Bortz, B. Bertheville, G. Böttger and K. Yvon, J. Alloys Compd., 1999, 287, L4–L6 CrossRef CAS.
  37. L. W. Huang, O. Elkedim, M. Nowak, R. Chassagnon and M. Jurczyk, Int. J. Hydrogen Energy, 2012, 37, 14248–14256 CrossRef CAS.
  38. Y. Song, W. C. Zhang and R. Yang, Int. J. Hydrogen Energy, 2009, 34, 1389–1398 CrossRef CAS.
  39. Y. Song, Z. X. Guo and R. Yang, Phys. Rev. B: Condens. Matter Mater. Phys., 2004, 69, 094205 CrossRef.
  40. T. Fischer and J. Almlof, J. Phys. Chem., 1992, 96, 9768–9774 CrossRef CAS.
  41. B. Y. Tang, N. Wang, W. Y. Yu, X. Q. Zeng and W. J. Ding, Acta Mater., 2008, 279, 192–200 Search PubMed.
  42. J. H. Dai, Y. Song, B. Shi and R. Yang, J. Phys. Chem. C, 2013, 117, 25374–25380 CrossRef CAS.
  43. B. Shi and Y. Song, Int. J. Hydrogen Energy, 2013, 38, 6417–6424 CrossRef CAS.
  44. J. H. Dai, Y. Song and R. Yang, Int. J. Hydrogen Energy, 2011, 36, 12939–12949 CrossRef CAS.
  45. A. J. Du, S. C. Smith and G. Q. Lu, J. Phys. Chem. C, 2007, 111, 8360–8365 CrossRef CAS.
  46. J. Zhang, Y. N. Huang, C. Mao and P. Peng, J. Alloys Compd., 2012, 538, 205–211 CrossRef CAS.
  47. R. F. W. Bader, Chem. Rev., 1991, 91, 893–928 CrossRef CAS.
  48. G. Henkelman, A. Arnaldsson and H. Jónsson, Comput. Mater. Sci., 2006, 36, 354–360 CrossRef.
  49. E. Sanville, S. D. Kenny, R. Smith and G. Henkelman, J. Comput. Chem., 2007, 28, 899–908 CrossRef CAS PubMed.

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