Fei Liab,
Dashuai Wangc,
Henan Dub,
Dan Zhou*d,
Yanming Maae and
Yanhui Liu*ab
aBeijing Computational Science Research Center, Beijing 10000, China. E-mail: yhliu@ybu.edu.cn
bDepartment of Physics, College of Science, Yanbian University, Yanji 133002, China
cKey Laboratory of Physics and Technology for Advanced Batteries (Ministry of Education), College of Physics, Jilin University, Changchun, 130012, China
dLaboratory of Clean Energy Technology, Changchun University of Science and Technology, Changchun 130022, China. E-mail: Zhoudan777@aliyun.com
eState Key Lab of Superhard Materials, Jilin University, Changchun, 130012, China
First published on 22nd February 2017
The solid inner core of Earth is mainly composed of an iron-rich alloy with nickel and some lighter elements like hydrogen, carbon, and oxygen, but the exact composition and chemical reactions are still elusive. Hydrogen has been proposed as the main element responsible for the density deficit observed in the Earth’s inner core. Moreover, the solubility of hydrogen in iron increases considerably with increasing pressure. Here, we systematically investigated global energetically stable structures of FeH4 in the pressure range of 80–400 GPa using a first-principles structural search. A transition from an insulated α-phase to a metallic β-phase and then to a semi-conductive γ-phase was predicted. Interestingly, we find a superconducting state in the β-phase with a transition temperature of 1.70 K at 109.12 GPa. The results are useful for investigating the stable phases and equation of state in the Fe–H system, which are relevant to the Earth’s core.
Under pressure experimental studies are scarce because of technical difficulties. Depending on the experimental conditions, FeH has been synthesized into different close-packed phases (dhcp), hcp, and face-centered cubic, and at least up to 80 GPa the most stable phase has the double hexagonal close-packed structure.7–11 Recently, cubic FeH3 was observed using X-ray diffraction above 86 GPa.12 Moreover, the solubility of hydrogen in iron increases considerably with increasing pressure.13 In a recent theoretical study, FeH4 with space group P21/m has been proposed in a pressure range of 300–400 GPa.13 However, its crystal structure and electronic properties in a broader pressure range need to be confirmed and studied. Therefore, with the help of theoretical calculations, predictions of the possible chemical reactions and structures of the Fe–H system may help to understand the density deficit observed in the Earth’s inner core.
In this work, we present an extensive structure search to identify the crystal structure of FeH4 by using the developed CALYPSO method, which has succeeded in predicting the crystal structures of various systems. Our work shows that FeH4 crystallizes in the cubic P213 (α-phase) structure up until 109.12 GPa and undergoes structural transitions to the orthorhombic Imma (β-phase) structure up until 241.72 GPa, then to the monoclinic P21m (γ-phase) structure. The phonon-mediated superconducting behavior of the β-phase was revealed by exploring the electron–phonon coupling. We hope that our study provides guidance for experimental groups aiming to synthesize novel crystal stoichiometry under high pressure. The present work establishes the comprehensive understanding of the structures and properties of FeH4 under the Earth’s core pressure.
The atomic arrangements of the competing structures are shown in Fig. 2. The optimized structure parameters at related pressures are listed in Table 1. The α-phase has a cubic primitive symmetry, with a = b = c = 4.061 Å (Z = 4) at 80 GPa (Fig. 2(a)). Four Fe atoms occupy the Wyckoff 4a site and sixteen H atoms lie in the 4a and 12b sites in the unit cell. In this structure, each Fe atom is coordinated to six H atoms in a trigonal prismatic environment, connected by a hydrogen bridge. The Fe–H distances are 1.587 Å and 1.526 Å at 80 GPa. In the case of the β-phase, it belongs to an orthorhombic space group, with lattice parameters of a = 2.400 Å, b = 3.225 Å, and c = 7.967 Å at 109.12 GPa (Fig. 2(b)). Four Fe atoms occupy the Wyckoff 4e site and six H atoms lie in the 4e, 8h, and 4b sites in the unit cell. Each Fe atom is coordinated to six H atoms in a unit cell. The Fe–H distances are 1.616 Å and 1.628 Å. In the case of the γ-phase, its equilibrium lattice parameters are a = 2.373 Å, b = 3.107 Å, and c = 3.567 Å, and β = 77.772° at 241.71 GPa (Fig. 2(c)). Two Fe atoms occupy the Wyckoff 2e site and eight H atoms lie in 2e, 2c and 4f sites in the unit cell. Each Fe atom is coordinated to seven H atoms in the unit cell. The Fe–H distances are 1.481 Å, 1.568 Å, and 1.543 Å at 109.12 GPa. In these hydrides, the H–H distance diminishes with pressure, from 1.470 Å in the α-phase to 1.442 Å in the β-phase to 1.203 Å in the γ-phase. However, the 1.0 Å H–H distance for metal hydrogen (at P = 450 GPa) does not appear in FeH4 structures until 400 GPa.28 The coordination number of the Fe atom increases from 4 in the α-and β-phase to 7 in the γ-phase, which is in agreement with the behavior of extended systems under pressure in general. In fact, our simulated γ-phase is consistent with the results in a theoretical study.13 Fig. 3 shows the simulated X-ray diffraction data of these structures, indicating that their structures are different from each other.
Lattice parameters (Å) | Atoms | x | y | z | |
---|---|---|---|---|---|
α-Phase | a = 4.061 | Fe (4a) | 0.5979 | 0.5979 | 0.5979 |
b = 4.061 | H (4a) | 0.2263 | 0.2263 | 0.2263 | |
c = 4.061 | H (12b) | 0.7776 | 0.0491 | 0.1101 | |
β-Phase | a = 2.400 | Fe (4e) | 1.0000 | 0.2500 | 0.1153 |
b = 3.225 | H (4b) | 0.5000 | 0.0000 | 0.0000 | |
c = 7.967 | H (8h) | 0.0000 | 0.9680 | 0.3002 | |
H (4e) | 0.0000 | 0.7500 | 0.1019 | ||
γ-Phase | a = 2.373 | Fe (2e) | 0.5516 | 0.2500 | 0.2505 |
b = 3.107 | H (2c) | 0.0000 | 0.0000 | 0.5000 | |
c = 3.567 | H (2e) | 0.4388 | 0.2500 | 0.6871 | |
β = 77.772° | H (4f) | 0.8672 | 0.0324 | 0.8780 |
To analyze the electronic properties of the identified stable structures, we calculate their energy band structures considered in the standard PBE-GGA functional for crystalline FeH4 in Fig. 4(a–c). The calculated PDOSs (projected densities of states) for the β-phase are shown in Fig. 4(d). For the α-phase, it is an insulator with a larger indirect band gap of 2.64 eV. In this structure, the band gaps decrease with increasing pressure when the molar volume decreases – when the van der Waals gap reduces, the orbital overlap across the gap is enhanced and this would reduce the energy separation between bonding and anti-bonding interactions.30,31 In Fig. 4(d), between −3 to 1.5 eV, a significant hybridization of Fe 3d and H s for the β-phase is shown. It must also be mentioned that H s has been extended ten times. We employ Bader charge analysis, which provides a description of electron transfer, to quantify the amount of charge belonging to each atom at different pressure points. The calculated charge values are 7.1335 (1.2166), 7.228 (1.1921) and 7.2061 (1.1985) electrons for Fe(H) for the α-, β- and γ-phase, respectively. This result reveals that the charge states of Fe and H atoms change with pressure-induced transition. However, the net charges on Fe and H atoms are less than the nominal charges on the ions (+8 for Fe and −1 for H). Accordingly, in FeH4, the bond between Fe and H atoms shows evident ionic character and a little covalent bond exists between Fe and H atoms at the same time.
The predicted overlap between conduction and valence bands reveals that the β-phase is metallic, while a weak overlap of conduction and valence bands occurs in the γ-phase. It is known that standard PBE-GGA usually underestimates the band gap. Therefore, we have employed the HSE hybrid functional that has been widely considered as providing a better description of the electronic properties (especially the band position).32–34 For the β structure, the band still crosses over the Fermi level at 109.12 GPa. It is interesting to note that the predicted γ-phase is a semi-conductor, as illustrated by the HSE corrections with a band gap of 0.4 eV.
Metallic high-pressure phases of hydrogen-rich compounds are promising high-temperature superconductors.35–41 Interestingly, the band structure of the β-phase crossing the Fermi level along the R–M–Γ direction is quite flat, and a narrow energy window located at the Fermi level results in a large electronic density of states near the Fermi energy. The corresponding restricted conduction electrons near the band gap possess a large effective mass with their group velocities approaching zero. Above all, such flat bands with highly mobile and localized electrons should provide the strong electron–phonon coupling necessary for superconductivity. To explore the superconducting properties, we calculated the electron–phonon coupling parameter, λ(ω), the logarithmic average phonon frequency, ωlog, and the electronic DOS at the Fermi level, N(Ef), for the β-phase, at 109.12 GPa in Fig. 5. Note that the low-frequency vibrations which are mainly associated with the Fe atoms due to their relatively higher atomic mass, provide a contribution of 25% of the total EPC parameter, while the phonon high-frequencies between 15 and 60 THz associated with the H atoms account for nearly 75% of λ(ω). Therefore, it is suggested that H atoms play a significant role in the superconductivity of FeH4. According to our calculations, λ(ω) reaches 0.36, and ωlog is 756.33 K, so the estimated Tc within the Allen–Dynes modified McMillan equation38 becomes 1.70 K, considering the typical Coulomb pseudopotential parameter, μ* = 0.1. It should be noted that a recent theoretical prediction of GeH4 and SnH4 gave a much larger Tc of 102 K and 62 K, respectively, where the “H2” unit has been suggested to be mainly responsible for the EPC parameter.42,43 In our predicted structure of FeH4, the relatively small Tc stems from a missing H2 unit.
Fig. 5 The calculated phonon dispersion (left), Eliashberg phonon spectral function, α2F(ω)/ω, partial electron–phonon integral, λ(ω), and site-projected phonon DOS of the β-phase (right). |
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