Abstract
This study presents a computational investigation of X4H15 compounds (where X represents a metal) as potential superconductors at ambient conditions or under pressure. Through systematic density functional theory calculations and electron–phonon coupling analysis, it is demonstrated that electronic structure engineering via hole doping dramatically enhances the superconducting properties of these materials. While electron‐doped compounds with X4 + cations (Ti, Zr, Hf, Th) exhibit modest transition temperatures of 1–9 K, hole‐doped systems with X3 + cations (Y, Tb, Dy, Ho, Er, Tm, Lu) show remarkably higher values of ≈50 K at ambient pressure. Superconductivity in hole‐doped compounds originates from stronger coupling between electrons and both cation and hydrogen phonon modes. Although pristine X3 + 4H15 compounds are thermodynamically unstable, a viable synthesis route via controlled hole doping of the charge‐compensated YZr3H15 compound is proposed. The calculations predict that even minimal concentrations of excess Y can induce high‐temperature superconductivity while preserving structural integrity. This work reveals how strategic electronic structure modulation can optimize superconducting properties in hydride systems, establishing a promising pathway toward practical high‐temperature conventional superconductors at ambient pressure.
Keywords: conventional superconductors, DFT calculations, hydride, hole‐doping, superconductivity
Hole doping in X4H15 hydrides significantly enhances superconductivity, with X3 + compounds reaching T c values near 50 K due to strong electron–phonon coupling. A viable route is proposed by doping thermodynamically unstable 15 to control the charge‐compensated YZr3H15 compound. This work demonstrates how electronic structure modulation can enable high‐T c superconductivity under ambient pressure.

1. Introduction
Hydride superconductors have attracted significant attention due to their potential for achieving high‐temperature superconductivity, particularly in high‐pressure synthesized binary hydrides, such as H3S (203 K, 155 GPa)[ 1 , 2 , 3 ] and LaH10 (250–260 K, 170 GPa),[ 4 , 5 , 6 , 7 ] and ternary hydrides, such as (La, Y)H10 (253 K at 183 GPa),[ 8 ] (La, Ca)H10 (247 K at 173 GPa),[ 9 ] and (La, Al)H10 (223 K at 164 GPa).[ 10 ] These structures exhibit remarkably high superconducting transition temperature (T c), yet their stabilization pressures exceed 150 GPa, posing a significant barrier to practical applications. Consequently, researchers have shifted their focus toward identifying hydrides that maintain stability under relatively low‐pressure conditions or even at ambient temperatures, with the goal of discovering practical, novel superconductors.
Among these systems, the X4H15 compounds (where X = Zr, Hf, Th) represent a captivating class of materials, requiring relatively moderate pressures compared to other hydride superconductors. Th4H15, first synthesized and characterized in the 1970s, exhibits a transition temperature (T c) of 7.5–8 K at ambient pressure, establishing it as a pioneering example of hydride superconductivity.[ 11 , 12 ] The Th sublattice in Th4H15 adopts a cI16 structure, characterized as a distorted 2 × 2 × 2 supercell of a body‐centered cubic (bcc) sublattice.[ 12 ] The hydrogen atoms in Th4H15 form an intricate network, incorporating both interstitial and framework hydrogen. This distinctive hydrogen arrangement, with multiple interstitial site occupations, profoundly influences the electronic and vibrational properties, thereby controlling superconductivity. Subsequently, Hf4H15 and Zr4H15 were successfully synthesized with analogous structures,[ 13 , 14 ] confirming the robustness and versatility of this hydride class. Experimental investigations reveal that Hf4H15 achieves a T c of 4.5 K at 23 GPa,[ 13 ] while Zr4H15 demonstrates superconductivity with a T c of 4 K at 40 GPa.[ 14 ] Computational studies have provided crucial insights into the stability and electronic properties of these systems. Theoretical calculations for Hf4H15 predict superconductivity with T c ranging from 0.8 to 2.1 K at 200 GPa, maintaining structural stability between 100 and 200 GPa.[ 15 ] Similarly, simulations for Zr4H15 predict a T c of 0.2–0.8 K at 40 GPa, with stability in the 50–100 GPa range.[ 14 ]
The uniqueness of the X4H15 structure resides in its high hydrogen content and distinctive electronic properties, positioning it as an ideal candidate for investigating superconductivity in low‐pressure or ambient‐pressure hydrides. In this work, we present a comprehensive computational investigation of the X4H15 family, methodically exploring potential compounds where X spans the periodic table. Our study integrates thermodynamic stability analysis with electron‐phonon coupling calculations to predict superconducting properties. The objective is to elucidate the fundamental mechanisms driving superconductivity and develop optimization strategies for achieving higher T c. Our investigation reveals that hole doping emerges as a remarkably effective approach for enhancing superconductivity. By introducing hole carriers, selective doping strategically modulates the electronic density of states (DOS) near the Fermi level and significantly strengthens electron‐phonon coupling, offering a powerful new paradigm for optimizing the superconducting properties of hydrides.[ 16 , 17 , 18 , 19 ]
We remark that previous theoretical studies have demonstrated that hole doping in hydrides such as CaYH12,[ 20 ] Ca(BH4)2 [ 21 ] can strongly increase T c. This enhancement primarily stems from critical modifications in the DOS near the Fermi level and intensification of phonon softening effects induced by hole doping, which synergistically amplify electron–phonon coupling. Furthermore, hole doping not only potentially triggers new superconducting phases but also substantially reduces the pressure threshold required for achieving high‐temperature superconductivity, hence offering a viable pathway for exploring high‐T c materials under ambient or near‐ambient conditions.[ 22 , 23 ] Experimentally, significant advancements have been made in realizing hole doping through elemental substitution or the introduction of vacancy defects. For instance, in the LaH10 system, partial substitution of La with low‐valence elements such as Be effectively introduces hole carriers, optimizing electron‐phonon coupling and enhancing superconducting performance.[ 24 ] Additionally, hole doping in hydrogen storage materials like Mg(BH4)2 has successfully induced an insulator‐to‐metal transition, accompanied by an exceptionally high DOS near the Fermi level, resulting in a T c as high as 140 K.[ 25 ]
2. Results and Discussion
The compound X4H15 crystallizes in the cubic system with space group (#220) (see Figure 1a). The X atoms exclusively occupy the 16c Wyckoff positions with full occupancy, while the hydrogen atoms distribute across two distinct crystallographic sites: the general 48e positions and the more symmetric 12a positions. This arrangement yields a total of 16 metal X atoms and 60 H atoms per conventional unit cell (4 formula units). The metal atoms in the conventional cell can be seen following a distorted bcc configuration. Each X atom is coordinated to 12 H atoms forming a distorted icosahedron. Neighboring icosahedra share facets formed by three H atoms. The strategic positioning of hydrogen atoms around the X centers creates well‐defined channels for electron transport and phonon propagation, playing a decisive role in determining the superconducting properties of these materials.
Figure 1.

The structures of X4H15 with space group at a) 0 GPa and b) 80 GPa. Blue, pink, and purple spheres denote the X atoms at 16c, H atoms at 48e, and H atoms at 12a Wyckoff positions, respectively.
We can assume the ‐1 oxidation state of hydrogen, which is typical of hydrides, this assumption is supported by calculated Bader charges for Zr4H15 and Y4H15. The H atoms exhibit charges ranging from –0.45 to –0.49, while the cations Zr and Y carry charges of ≈+1.78 and +1.72, respectively. Although the charge transfer deviates from the idealized one‐electron transfer from cation to hydrogen, these values are typical for metal hydrides with hydrogen in the –1 oxidation state.[ 26 , 27 ]
Achieving charge neutrality with the X4H−115 stoichiometry proves impossible, as pristine X4H15 would necessitate an oxidation state of +3.75 for the X atom. The three experimentally confirmed systems incorporate X atoms with oxidation state +4, resulting in one excess electron per formula unit relative to charge compensation. Conversely, a +3 cation generates three holes, while other oxidation states produce an untenable quantity of electrons or holes that would likely destabilize the system, for example Sr4H15 and Ba4H15 (that have seven holes) deform considerably to a structure without any symmetry after geometry optimization. Consequently, it is logical that all X4H15 systems exhibiting semiconducting behavior in our calculations (B4H15, Cd4H15, N4H15, Tl4H15, Bi4H15, C4H15, O4H15, Si4H15, Cu4H15, Os4H15, Ru4H15, and La4H15) relax to crystal structures that deviate substantially from the prototypical Th4H15 arrangement.
A number of X4H15 are magnetic, which hinders conventional superconductivity, specifically the compounds with X = K, Mn, Tc, Cr, V, Ce, Re, Bi, Gd, U, Pu, Np. Of the remaining 35 compounds, that are metallic and non‐magnetic, only Zr4H15, Hf4H15, and Th4H15 are on the convex hull of stability. Note that these three compounds have been synthesized experimentally, in excellent agreement with our results. Up to 100 meV atom−1 of the convex hull we still find Np4H15 (26 meV atom−1), Ce4H15 (37 meV atom−1), Pu4H15 (81 meV atom−1), K4H15 (91 meV atom−1), and Ti4H15 (95 meV atom−1). We note that the convex hull in this work were calculated using the Alexandria database.[ 28 , 29 ]
A possible way to improve the thermodynamic stability of this compounds is by enforcing charge compensation. To demonstrate this concept, we constructed YZr3H15 by substituting one Zr4 + in Zr4H15 with Y3 +. This turns out to be a very stable compound, positioned merely 5 meV atom−1 from the convex hull of stability, even if Y4H15 is 233 meV atom−1 above the hull. While hull distances suggest YZr3H15 is less stable than Zr4H15 and Hf4H15, formation energies reveal the opposite: YZr3H15 (–0.466 eV atom−1) is more stable than Zr4H15 (–0.429 eV atom−1) or Y4H15 (–0.365 eV atom−1). This apparent contradiction arises because Y–H binaries are more stable than Zr–H binaries (see phase‐diagrams in the Supporting Information), increasing the distance to the hull of the ternary compound. Therefore, YZr3H15 is indeed more stable than Zr4H15 and Hf4H15, but this stability is offset by the higher stability of YH3.
As anticipated, this compound behaves as a semiconductor with an indirect band gap of ≈1.1 eV within the PBE approximation (see Figure 2a). The valence band exhibits triple degeneracy at Γ, with one band displaying large hole mass along specific directions in the Brillouin zone. This characteristic generates a steep increase in the electronic density of states immediately below the valence band maximum. These bands predominantly comprise hydrogen states hybridized with the cation states. In contrast, the conduction bands manifest primarily Zr character, with minimal contributions from both Y and H. Based on these fundamental electronic structure characteristics, we can readily anticipate that hole doping would prove substantially more effective than electron doping in facilitating conventional superconductivity in these materials.
Figure 2.

Electronic band structure and density of states (DOS) for representative compounds: a) charge‐compensated YZr3H15, b) electron‐doped Zr4H15, and c) hole‐doped Y4H15. The Fermi level is set at 0 eV.
We begin our discussion on superconductivity with compounds where X = Ti, Zr, Hf, and Th exists in the +4 oxidation state. This configuration yields one excess electron per formula unit occupying the conduction band. The electronic band structure of Zr4H15, illustrated in Figure 2, exemplifies a degenerate semiconductor, exhibiting striking similarities to that of the semiconducting compound YZr3H15, presented in Figure 2a (note that the different symmetry points and path in the Brillouin zone result from the reduced symmetry of the latter system). The phonon band structure, depicted in Figure 3a, demonstrates characteristics typical of hydrides with heavy cations, where acoustic and low‐lying optical modes consist exclusively of cation vibrations, while hydrogen governs the higher‐energy modes. The maximum phonon frequency exceeds 2000 K. Nevertheless, despite the Fermi energy residing at a pronounced peak in the density of states, this compound demonstrates an unexpectedly small electron–phonon coupling constant (λ), resulting in exceedingly modest superconducting transition temperatures (see Table 1 ). Analogous behavior manifests in other X4 + materials. The calculated T c values for Zr and Hf compounds align closely with experimental measurements under pressure.[ 13 , 14 ] However, the predicted value for Th4H15 significantly underestimates the experimental observation (1.2 K vs the experimental 7–8 K.[ 11 , 12 ])
Figure 3.

Phonon band structure, phonon density of states and Eliashberg spectral function α2 F(ω) for representative compounds: a) electron‐doped Zr4H15 and b) hole‐doped Y4H15. The stronger coupling with high‐frequency hydrogen modes in the hole‐doped compound is evident.
Table 1.
Summary of the X4H15 compounds that are dynamically stable at zero pressure. We show the oxidation state of the X cation, the distance above the convex hull of stability (E hull in eV atom−1), the superconducting transition temperature calculated with the Allen‐Dynes correction[ 30 ] to the McMillan formula[ 31 ] with μ* = 0.1 ( in K), the electron‐phonon coupling constant λ, average of electron‐phonon coupling matrix elements squared 〈g 2〉 (in eV2),[ 32 ] the logarithmic average of the phonon frequency (ωlog in K), the total density of electronic states are Fermi level (TDOS in states eV−1 cell−1), and the partial density of H and X states ate the Fermi level (in states eV−1 cell−1).
| Compound | oxi. state | E hull |
|
λ | 〈g 2〉 | ωlog | TDOS | PDOSH | PDOSX | |
|---|---|---|---|---|---|---|---|---|---|---|
| Y4H15 | +3 | 0.233 | 53.1 | 1.32 | 0.89 | 474 | 5.38 | 3.45 | 1.87 | |
| Tb4H15 | +3 | 0.232 | 48.6 | 1.30 | 1.58 | 440 | 5.14 | 3.28 | 1.83 | |
| Dy4H15 | +3 | 0.231 | 48.9 | 1.27 | 1.61 | 457 | 5.05 | 3.20 | 1.81 | |
| Ho4H15 | +3 | 0.230 | 48.9 | 1.24 | 1.63 | 475 | 4.97 | 3.14 | 1.80 | |
| Er4H15 | +3 | 0.228 | 49.3 | 1.23 | 1.66 | 482 | 4.90 | 3.08 | 1.79 | |
| Tm4H15 | +3 | 0.227 | 50.4 | 1.23 | 1.70 | 495 | 4.83 | 3.02 | 1.78 | |
| Lu4H15 | +3 | 0.225 | 51.3 | 1.19 | 1.75 | 523 | 4.70 | 2.92 | 1.75 | |
| Th4H15 | +4 | 0.000 | 1.2 | 0.38 | 0.36 | 368 | 15.24 | 0.46 | 14.40 | |
| Ti4H15 | +4 | 0.095 | 9.2 | 0.52 | 0.13 | 625 | 9.82 | 0.49 | 9.15 | |
| Zr4H15 | +4 | 0.000 | 2.9 | 0.41 | 0.25 | 607 | 7.84 | 0.51 | 7.16 | |
| Hf4H15 | +4 | 0.000 | 4.8 | 0.47 | 0.57 | 476 | 7.33 | 0.53 | 6.65 | |
| Nb4H15 | +5 | 0.129 | 34.4 | 1.28 | 0.40 | 319 | 9.49 | 0.63 | 8.64 |
In contrast, Nb4H15 containing Nb5 +, introduces five additional electrons into the conduction band. This substantial electron doping profoundly transforms the electronic structure, although the fundamental band architecture of the hypothetical charge‐compensated compound remains identifiable. The density of states at the Fermi level for this +5 compound is markedly elevated compared to its +4 counterparts, yielding electron‐phonon coupling constants exceeding unity (λ > 1) and correspondingly enhanced T c values. Notably, the majority of coupling originates from the low‐lying niobium phonon modes, rather than from the high‐energy hydrogen vibrations, as demonstrated in SI #6 in Supporting Information.
The most intriguing results emerge for compounds containing trivalent metals: Y4H15, Tb4H15, Dy4H15, Ho4H15, Er4H15, Tm4H15, and Lu4H15. These systems, incorporating a +3 cation, generate three holes per formula unit in the valence band. All these compounds exhibit extraordinarily similar electronic and phononic band structures, culminating in nearly identical superconducting properties. The electronic band‐structure of Y4H15 is illustrated in Figure 2c. The resemblance to the charge‐compensated compound remains unmistakable, with the Fermi level positioned precisely on a prominent peak in the density of states. Once again, the low‐energy phonon states (see Figure 3) originate from the heavy cation, while the hydrogen modes segregate into distinct manifolds. The lowest energy and the two highest hydrogen manifolds involve vibrations of the atoms in both the 12a and 48e Wyckoff positions, while the remaining contains essentially vibrations of the hydrogens in the 48e positions. Due to the intricate geometry of these compounds, further categorizing these vibrations proves challenging; nevertheless, spectral analysis reveals that the low‐energy manifold predominantly exhibits torsional character, while the highest frequency modes correspond to hydrogen bond stretching vibrations. In this case, not only do the cation modes couple strongly to electrons, but the hydrogen modes contribute significantly as well, resulting in a substantial electron‐phonon coupling constant (λ = 1.3) and an exceptional superconducting transition temperature of ≈50 K (see Table 1).
The consistent behavior across diverse rare earth elements suggests that the superconducting properties are predominantly governed by common electronic structure features rather than the specific chemical identity of the metal. This fundamental observation receives further corroboration from our phonon calculations, which reveal strikingly similar phonon dispersions and electron–phonon coupling distributions across all trivalent metal compounds (see Figure 3 and Supporting Information).
Our comprehensive analysis spanning multiple compounds demonstrates that hole doping proves more effective than electron doping for enhancing superconducting properties in X4H15 systems. The λ values for hole‐doped compounds consistently exceed those of electron‐doped systems by a substantial margin, even when the total DOS at the Fermi level is comparatively lower (see Table 1). The profound contrast between hole‐doped and electron‐doped systems becomes evident, with the former exhibiting T c values that surpass the latter by an order of magnitude. The electron‐phonon coupling parameter λ can also be expressed as λ = N(E F)〈g 2〉/M〈ω2〉,[ 32 ] where N(E F), 〈g 2〉, 〈ω2〉, and M are the electronic density of states at the Fermi level, the average over the Fermi surface of electron‐phonon coupling matrix elements squared, the average of the phonon frequencies squared, and the atomic mass, respectively. As shown in Table 1, it happens that the hole doping 15 compounds have larger 〈g 2〉 values, therefore the increase of T c should mainly be attributed to stronger electron‐phonon coupling instead of an increase of N(E F).
To understand how these materials behave under pressure, we performed calculations of the superconducting properties of X4H15 compounds with varying pressure from –10 to 80 GPa, (see Figure 4 ). From the figure, the distinctive behavior of compounds depending on the oxidation state of the cation becomes immediately evident. For the +3 metals, λ decreases precipitously with pressure, while ωlog remains relatively constant, resulting in a monotonic decrease of T c. This phenomenon can be attributed to the softening of a phonon mode that eventually becomes imaginary at pressures above 10–20 GPa. The compounds subsequently undergo a structural phase transition (see Figure 1b) into a high‐pressure phase that maintains the same space group, but with cations reconfiguring into an undistorted bcc sublattice. In this structure, the electron‐phonon coupling decreases with pressure, while ωlog increases, leading to an enhancement of the transition temperature with pressure. For the +4 metals, λ diminishes to values substantially below 0.5, while ωlog increases to values approaching 1000 K, resulting in a net reduction of T c with pressure. Finally, for Nb, λ exhibits a minimum at ≈5 GPa, while ωlog reaches a maximum at ≈40 GPa, yielding a monotonically increasing T c that attains a value exceeding 40 K at 80 GPa.
Figure 4.

Superconducting critical temperature (T c), electron–phonon coupling constant (λ), and the logarithmic average of the phonon frequency (ωlog) as a function of pressure. The filled and empty symbol represent the low‐ and high‐pressure structures (See Figure 1). For a certain pressure we omit the systems that are not dynamically stable. Note for Yb only PBE pseudopotential is available, for the sake of consistency we do not plot the curve of Yb4H15.
We must emphasize that while 15 compounds demonstrate promising superconducting properties, they lack thermodynamic stability at ambient pressure. Our calculations reveal that these compounds reside ≈230 meV atom−1 above the convex hull of stability, and this instability can be directly attributed to the charge imbalance and the resulting electronic structure, which favors decomposition into more stable phases. As anticipated, the most probable decomposition pathway involves the charge‐compensated XH3 binary together with excess H2. While the formation enthalpy calculations indicate that these compounds become significantly more stable under pressure (see Supporting Information), a comprehensive assessment of their thermodynamic stability would require detailed phase diagram studies that are beyond the scope of this work.
While high‐pressure synthesis represents one possible route for these compounds, we propose a potentially more direct approach. Our strategy involves initiating with YZr3H15, which our calculations indicate lies remarkably close to thermodynamic stability (5 meV atom−1 above the convex hull) and exhibits chemical plausibility due to its charge‐compensated nature. Furthermore, cation site disorder will enhance stability through configurational entropy contributions. By synthesizing this compound with excess Y, one could effectively introduce hole doping while preserving structural integrity. As the DOS increases dramatically at the onset of valence states (see Figure 2), even modest amounts of excess Y might suffice to induce hole‐doped superconductivity in this system. Our band structure calculations demonstrate that removing merely 0.1–0.2 electrons per formula unit (equivalent to 5–10% Y excess) could shift the Fermi level into the region of elevated DOS at the top of the valence band.
To rigorously evaluate this concept, we constructed ordered cells with Y2Zr2H15 and Y3ZrH15 stoichiometry, for which the distance to the convex hull at 0 GPa are 59 and 135 meV atom−1, respectively. While these models cannot comprehensively capture the effects of substitutional doping in YZr3H15 due to the absence of disorder and the relatively high doping concentration, they provide critical insights into the potential behavior of such systems. The calculated electronic structure exhibits distinct metallic character with substantial DOS at the Fermi level, confirming the efficacy of this doping strategy. Furthermore, our phonon calculations for Y2Zr2H15 and Y3ZrH15 reveal no imaginary modes, unequivocally demonstrating dynamic stability. The electron‐phonon coupling constant for this compound is calculated to be ≈λ = 0.8 and 1.1. The T c of these systems show an intermediate behavior with respect to the binary compounds, with T c increasing with the amount of Y in the material. This intermediate behavior persists under applied pressure (as shown in Supporting Information).
In summary, our comprehensive computational investigation reveals that the superconducting properties of X4H15 compounds are profoundly influenced by their electronic configuration, with hole doping emerging as an exceptionally promising pathway to achieve high transition temperatures. The proposed strategy of introducing controlled hole doping in thermodynamically stable, charge‐compensated compounds represents a practical approach for the experimental realization of these promising superconducting materials.
Furthermore, our findings demonstrate that the underlying structural stability of these compounds is intimately connected to their electronic configuration. Charge‐compensated systems exhibit remarkable thermodynamic stability, while both electron and hole doping introduce varying degrees of instability that may necessitate high‐pressure synthesis conditions.
The extraordinary consistency in superconducting properties across different trivalent metal compounds (Y, Dy, Er, Ho, Lu, Tb, Tm) strongly indicates that the hole‐doping mechanism operates independently of the specific rare earth element. This universality reveals a fundamental electronic structure feature that could be systematically exploited in the rational design of new superconducting hydrides.
Our results carry significant implications for the broader field of hydride superconductivity. First, they underscore the critical importance of electronic structure engineering for optimizing superconducting properties. Second, they conclusively demonstrate that partial substitution constitutes an effective strategy for introducing carriers while maintaining structural stability. Finally, they suggest that other structurally related hydride systems could potentially benefit from analogous doping approaches.
3. Experimental Section
Calculations were performed of the entire family of X4H15 compounds where X spans the periodic table from Be to Bi, excluding rare‐gases. Geometry relaxations and total energy calculations were performed using the vasp code[ 33 , 34 ] with the Perdew–Burke–Ernzerhof approximation[ 35 ] to the exchange‐correlation functional. To sample the Brillouin zones, a 3× 3 ×3 Γ‐centred k‐point grid was used. Spin‐polarised calculations were initiated from a ferromagnetic configuration. The projector augmented wave (PAW) setup[ 36 , 37 ] within vasp version 5.2 was utilized, applying a cutoff of 520 eV. We established the convergence criteria of the forces to be less than 0.005 eV Å−1.
Distances to the convex hull were calculated against the convex hull of the Alexandria database.[ 28 , 29 ] It is remarked that this represents the largest convex hull freely available, substantially more extensive than that of the Materials Project database.[ 38 ] All parameters, including pseudopotentials, were configured to ensure compatibility with the data available in the Alexandria database.[ 28 , 29 ]
Phonon calculations were executed using version 7.1 of quantum espresso [ 39 , 40 ] with the Perdew–Burke–Ernzerhof functional for solids (PBEsol)[ 35 ] generalized gradient approximation. The PBEsol pseudopotentials[ 35 ] was employed from the pseudodojo project,[ 41 ] specifically the stringent, scalar‐relativistic norm‐conserving set. Geometry optimizations were conducted using a uniform Γ‐centered 4 × 4 × 4 k‐point grid. Convergence thresholds for energies, forces, and stresses were established at 1 × 10−8 a.u., 1 × 10−6 a.u., and 5 × 10−2 kbar, respectively. For the electron–phonon coupling calculations, a double‐grid technique, utilizing a 8 × 8 × 8 k‐grid as the coarse grid, and a 16 × 16 × 16 as the fine grid was implemented. For the q‐sampling of phonons, a 2 × 2 × 2 q‐point grid was employed. The double δ‐integration to obtain the Eliashberg function was performed with a Methfessel–Paxton smearing of 0.05 Ry.
Conflict of Interest
The authors declare no conflict of interest.
Supporting information
Supporting Information
Acknowledgements
K.G. acknowledges financial support from the China Scholarship Council (202208320112). M.A.L.M. was supported by a grant from the Simons Foundation (SFI‐MPS‐NFS‐00006741‐12, P.T.) in the Simons Collaboration on New Frontiers in Superconductivity and by the Keele and the Klaus Tschira foundations as a part of the SuperC collaboration. T.F.T.C. acknowledges the financial support from FCT ‐ Fundaçào para a Ciência e Tecnologia, I.P. through the projects UIDB/04564/2020 and CEECINST00152/2018/CP1570/CT0006, with DOI identifiers 10.54499/UIDB/04564/2020 and 10.54499/CEECINST/00152/2018/CP1570/CT0006 respectively, and computing resources provided by the project Advanced Computing Project 2023.14294.CPCA.A3, platform Deucalion. W.C., H.C.W and M.A.L.M. acknowledge the funding from the Sino‐German Mobility Programme under Grant No. M‐0362. The authors thank the Gauss Centre for Supercomputing e.V. (www.gauss‐centre.eu) for funding this project by providing computing time on the GCS supercomputer SUPERMUC‐NG at the Leibniz Supercomputing Centre (www.lrz.de) under the project pn25co. H.C.W and M.A.L.M. would like to thank the NHR Centre PC2 for providing computing time on the Noctua 2 supercomputers.
Open access funding enabled and organized by Projekt DEAL.
Gao K., Cui W., Cerqueira T. F. T., Wang H.‐C., Botti S., and Marques M. A. L., “Enhanced Superconductivity in X4H15 Compounds via Hole‐Doping at Ambient Pressure.” Adv. Sci. 12, no. 39 (2025): e08419. 10.1002/advs.202508419
Contributor Information
Wenwen Cui, Email: wenwencui@jsnu.edu.cn.
Miguel A. L. Marques, Email: miguel.marques@rub.de.
Data Availability Statement
The data that support the findings of this study are available in the supplementary material of this article.
References
- 1. Li Y., Hao J., Liu H., Li Y., Ma Y., J. Chem. Phys. 2014, 140, 174712. [DOI] [PubMed] [Google Scholar]
- 2. Duan D., Liu Y., Tian F., Li D., Huang X., Zhao Z., Yu H., Liu B., Tian W., Cui T., Sci. Rep. 2014, 4, 6968. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 3. Drozdov A., Eremets M., Troyan I., Ksenofontov V., Shylin S. I., Nature 2015, 525, 73. [DOI] [PubMed] [Google Scholar]
- 4. Liu H., Naumov I. I., Hoffmann R., Ashcroft N., Hemley R. J., Proc. Natl. Acad. Sci 2017, 114, 6990. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 5. Peng F., Sun Y., Pickard C. J., Needs R. J., Wu Q., Ma Y., Phys. Rev. Lett. 2017, 119, 107001. [DOI] [PubMed] [Google Scholar]
- 6. Drozdov A., Kong P., Minkov V., Besedin S., Kuzovnikov M., Mozaffari S., Balicas L., Balakirev F., Graf D., Prakapenka V., Greenberg E., Knyazev D. A., Tkacz M., Eremets M. I., Nature 2019, 569, 528. [DOI] [PubMed] [Google Scholar]
- 7. Somayazulu M., Ahart M., Mishra A. K., Geballe Z. M., Baldini M., Meng Y., Struzhkin V. V., Hemley R. J., Phys. Rev. Lett. 2019, 122, 027001. [DOI] [PubMed] [Google Scholar]
- 8. Semenok D. V., Troyan I. A., Ivanova A. G., Kvashnin A. G., Kruglov I. A., Hanfland M., Sadakov A. V., Sobolevskiy O. A., Pervakov K. S., Lyubutin I. S., Glazyrin K. V., Giordano N., Karimov D. N., Vasiliev A. L., Akashi R., Pudalov V. M., Oganov A. R., Mater. Today 2021, 48, 18. [Google Scholar]
- 9. Chen S., Guo J., Wang Y., Wu X., Chen W., Huang X., Cui T., Phys. Rev. B 2024, 109, 224510. [Google Scholar]
- 10. Chen S., Qian Y., Huang X., Chen W., Guo J., Zhang K., Zhang J., Yuan H., Cui T., Natl. Sci. Rev. 2023, 11, nwad107. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 11. Satterthwaite C., Toepke I., Phys. Rev. Lett. 1970, 25, 741. [Google Scholar]
- 12. Satterthwaite C., Peterson D., J. Less‐Common Met. 1972, 26, 361. [Google Scholar]
- 13. Kuzovnikov M. A., Tkacz M., J. Phys. Chem. C 2019, 123, 30059. [Google Scholar]
- 14. Xie H., Zhang W., Duan D., Huang X., Huang Y., Song H., Feng X., Yao Y., Pickard C. J., Cui T., J. Phys. Chem. Lett. 2020, 11, 646. [DOI] [PubMed] [Google Scholar]
- 15. Xie H., Yao Y., Feng X., Duan D., Song H., Zhang Z., Jiang S., Redfern S. A., Kresin V. Z., Pickard C. J., Cui T., Phys. Rev. Lett. 2020, 125, 217001. [DOI] [PubMed] [Google Scholar]
- 16. Wang C., Liu S., Jeon H., Yi S., Bang Y., Cho J.‐H., Phys. Rev. B 2021, 104, L020504. [Google Scholar]
- 17. Rudenko A. N., Badrtdinov D. I., Abrikosov I. A., Katsnelson M. I., Phys. Rev. B 2024, 109, 014502. [Google Scholar]
- 18. Rosner H., Kitaigorodsky A., Pickett W. E., Phys. Rev. Lett. 2002, 88, 127001. [DOI] [PubMed] [Google Scholar]
- 19. Zhu L., Liu H., Somayazulu M., Meng Y., Guńka P. A., Shiell T. B., Kenney‐Benson C., Chariton S., Prakapenka V. B., Yoon H., Horn J. A., Paglione J., Hoffmann R., Cohen R. E., Strobel T. A., Phys. Rev. Res. 2023, 5, 013012. [Google Scholar]
- 20. Liang X., Bergara A., Wang L., Wen B., Zhao Z., Zhou X.‐F., He J., Gao G., Tian Y., Phys. Rev. B 2019, 99, 100505. [Google Scholar]
- 21. Di Cataldo S., Boeri L., Phys. Rev. B 2023, 107, L060501. [Google Scholar]
- 22. Ding H.‐B., Niu R., Li S.‐A., Liu Y.‐M., Chen X.‐J., Lin H.‐Q., Zhong G.‐H., Adv. Sci. 2024, 11, 2408275. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 23. Chen Q., Yang X., Yang X., Chen J., Shen C., Zhang P., Li Y., Tao Q., Xu Z.‐A., Front. Phys. 2017, 12, 1. [Google Scholar]
- 24. Song Y., Bi J., Nakamoto Y., Shimizu K., Liu H., Zou B., Liu G., Wang H., Ma Y., Phys. Rev. Lett. 2023, 130, 266001. [DOI] [PubMed] [Google Scholar]
- 25. Liu X., Zhang L., Wang M., Huang X., Liu L., Jia Y., Mater. Today Phys. 2024, 40, 101299. [Google Scholar]
- 26. Matar S. F., Prog. Solid State Chem. 2010, 38, 1. [Google Scholar]
- 27. Mizoguchi H., Park S.‐W., Hosono H., J. Am. Chem. Soc. 2021, 143, 11345. [DOI] [PubMed] [Google Scholar]
- 28. Schmidt J., Pettersson L., Verdozzi C., Botti S., Marques M. A. L., Sci. Adv. 2021, 7, eabi7948. [DOI] [PMC free article] [PubMed] [Google Scholar]
- 29. Schmidt J., Hoffmann N., Wang H.‐C., Borlido P., Carriço P. J., Cerqueira T. F., Botti S., Marques M. A., Adv. Mater. 2023, 35, 2210788. [DOI] [PubMed] [Google Scholar]
- 30. Allen P. B., Dynes R., Phys. Rev. B 1975, 12, 905. [Google Scholar]
- 31. McMillan W. L., Phys. Rev. 1968, 167, 331. [Google Scholar]
- 32. Hopfield J. J., Phys. Rev. 1969, 186, 443. [Google Scholar]
- 33. Kresse G., Furthmüller J., Comput. Mater. Sci. 1996, 6, 15. [Google Scholar]
- 34. Kresse G., Furthmüller J., Phys. Rev. B 1996, 54, 11169. [DOI] [PubMed] [Google Scholar]
- 35. Perdew J. P., Ruzsinszky A., Csonka G. I., Vydrov O. A., Scuseria G. E., Constantin L. A., Zhou X., Burke K., Phys. Rev. Lett. 2008, 100, 136406. [DOI] [PubMed] [Google Scholar]
- 36. Blöchl P. E., Phys. Rev. B 1994, 50, 17953. [DOI] [PubMed] [Google Scholar]
- 37. Kresse G., Joubert D., Phys. Rev. B 1999, 59, 1758. [Google Scholar]
- 38. Jain A., Ong S. P., Hautier G., Chen W., Richards W. D., Dacek S., Cholia S., Gunter D., Skinner D., Ceder G., Persson K. A., APL Mater. 2013, 1, 011002. [Google Scholar]
- 39. Giannozzi P., Baroni S., Bonini N., Calandra M., Car R., Cavazzoni C., Ceresoli D., Chiarotti G. L., Cococcioni M., Dabo I., Corso A. D., de Gironcoli S., Fabris S., Fratesi G., Gebauer R., Gerstmann U., Gougoussis C., Kokalj A., Lazzeri M., Martin‐Samos L., Marzari N., Mauri F., Mazzarello R., Paolini S., Pasquarello A., Paulatto L., Sbraccia C., Scandolo S., Sclauzero G., Seitsonen A. P., et al., J. Phys.: Condens. Matter 2009, 21, 395502. [DOI] [PubMed] [Google Scholar]
- 40. Giannozzi P., Andreussi O., Brumme T., Bunau O., Nardelli M. B., Calandra M., Car R., Cavazzoni C., Ceresoli D., Cococcioni M., Colonna N., Carnimeo I., Dal Corso A., de Gironcoli S., Delugas P., DiStasio Jr R. A., Ferretti A., Floris A., Fratesi G., Fugallo G., Gebauer R., Gerstmann U., Giustino F., Gorni T., Jia J., Kawamura M., Ko H.‐Y., Kokalj A., Küçükbenli E., Lazzeri M., et al., J. Phys.: Condens. Matter 2017, 29, 465901. [DOI] [PubMed] [Google Scholar]
- 41. van Setten M., Giantomassi M., Bousquet E., Verstraete M., Hamann D., Gonze X., Rignanese G.‐M., Comput. Phys. Commun. 2018, 226, 39. [Google Scholar]
Associated Data
This section collects any data citations, data availability statements, or supplementary materials included in this article.
Supplementary Materials
Supporting Information
Data Availability Statement
The data that support the findings of this study are available in the supplementary material of this article.
