FORM OF SILICON AND METHOD OF MAKING THE SAME
20170355605 ยท 2017-12-14
Assignee
Inventors
- Timothy A. Strobel (Washington, DC)
- Duck Young Kim (Washington, DC)
- Oleksandr O. Kurakevych (Washington, DC)
Cpc classification
International classification
Abstract
The invention relates to a new phase of silicon, Si.sub.24, and a method of making the same. Si.sub.24 has a quasi-direct band gap, with a direct gap value of 1.34 eV and an indirect gap value of 1.3 eV. The invention also relates to a compound of the formula Na.sub.4Si.sub.24 and a method of making the same. Na.sub.4Si.sub.24 may be used as a precursor to make Si.sub.24.
Claims
1-9. (canceled)
10. A compound of the formula Si.sub.24.
11-12. (canceled)
13. The compound of claim 10 having an indirect band gap of 1.3 eV and a direct band gap of 1.34 eV.
14-16. (canceled)
17. The compound of claim 10 wherein the sodium concentration is less than 0.1 atom %.
18. The compound of claim 10 wherein the structure is nanoporous.
Description
DESCRIPTION OF THE DRAWINGS
[0016] The invention is more fully described by reference to the accompanying drawings wherein:
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DETAILED DISCUSSION
[0041] Applicants first describe certain silicon clathrates and new and unexpected methods of making such compounds.
[0042] Silicon clathrates (1) (or simply clathrates throughout this application) are analogues to the water-based clathrate hydrates,(2) often crystallizing as high-symmetry cubic structures. Si atoms within these compounds take on an sp.sup.3 hybridization state to form a covalent network of polyhedral cavities that host appropriately sized guest atoms. The alkali and alkaline earth metals can be intercalated into these cages that extend in three dimensions. The cubic structure I (sI, Pm
[0043] Most known silicon clathrates have been synthesized at ambient pressure or under deep vacuum using ZintI compounds as precursors or through different types of chemical reactions (1, 6) Up to now, chemical decomposition (arc-remelting or heating in vacuum/Ar atmosphere) remains the principal method for NaSi clathrate synthesis (6, 10, 11). Later, chemical oxidation was proposed as an alternative route (12), as well as spark plasma treatment of the Na.sub.4Si.sub.4 precursor. Although single crystals of some Si clathrates can be grown by the techniques just mentioned (10, 13), the equilibrium synthesis from a melt remains a challenging task for well-controlled crystal growth. The knowledge of thermodynamic stability domains in terms of composition, temperature, and pressure is, therefore, of primary importance.
[0044] The generalized thermodynamic stabilities of silicon clathrate phases are not clear. Guest-free Si clathrates have been predicted to be stable only at negative pressures below 3 GPa (14, 15), (a direct analogy may be drawn between the negative pressure stability of empty silicon and water-based clathrates). While some Ba- and halogen-based silicon clathrates can be synthesized at high pressure (16, 17), ab initio results on the high-pressure stability of NaSi clathrates suggest that these phases are thermodynamically unstable with respect to decomposition at high-pressure conditions (10), Thus, the p-T domains for thermodynamic stability and the possibility for equilibrium crystal growth need clarification.
[0045] At present, the phase equilibria for the NaSi system remain the least understood as compared with other clathrate systems (e.g., BaSi). Sodium is the lightest metal that is known to intercalate the Si cages alone, and its understanding may lead, for example, to the synthesis of Li-, Mg-, and Be-bearing clathrates. The experimentally established binary phase diagram at ambient pressure contains only one congruently melting compound of Na and Si, sodium silicide (Na.sub.4Si.sub.4), and clathrate formation has not been observed under (quasi-) equilibrium conditions (18). In situ study of NaSi clathrate growth under high-temperature, high-vacuum conditions allows one to conclude that its formation is principally determined by mutual structural relationships of phases and dynamic phenomena (e.g., sodium volatility), rather than thermodynamic stability of corresponding phases (19).
[0046] Contrary to Ba-based clathrates (20), high-pressure synthesis has not been explored so far for the NaSi system. The remarkable negative values of atomic V of clathrate formations (1.5-2.5 cm.sup.3/mol; Table 1, below), compared with the elemental constituents, suggests that high pressure should facilitate their formation. High pressure (HP) synthesis is the most reliable method for elaboration and properties control of high-pressure phases, such as diamond (21, 22), cubic boron nitride (23, 24), and boron-rich compounds (25). The quasi-equilibrium growth of HP phases from solvents allows production of high-purity single crystals of a given habit and high-quality powders.
TABLE-US-00001 TABLE 1 Mean Atomic Volumes of Formation V.sub.at .sub.f of sodium clathrates (cm.sup.3/mol) Clathrate <V.sub.at>.sup.clathrate <V.sub.at>.sup.Na+Si V.sub.at.sub.f Na.sub.24Si.sub.136 12.03 13.81 1.78 Na.sub.8Si.sub.46 11.83 13.79 1.96 NaSi.sub.6 11.35 13.72 2.37
[0047] This application discloses experimental and theoretical results that unambiguously indicate that Na clathrates are thermodynamically stable high-pressure phases. Stoichiometric sodium clathrates of structure I (Na.sub.8Si.sub.46) and a new metallic clathrate compound Na.sub.4Si.sub.24 were synthesized directly from the elements, allowing for new opportunities for melt-based growth under equilibrium conditions. Over the range of conditions studied, the Na.sub.24Si.sub.136 clathrate (sII) only forms as an intermediate compound prior to crystallization of the sI phase.
[0048] Sodium clathrates were prepared from elemental Na/Si mixtures (20 mol % Na, i.e., 5% excess as compared with stoichiometric sI and sII clathrates). The initial mixture was ground for 1 hour in a porcelain mortar contained within a glovebox under a high-purity Ar atmosphere. The mixtures were loaded into double-walled capsules, the inner one from Ta and the outer one from Au (see
TABLE-US-00002 TABLE 2 Experimental conditions of High Pressure synthesis and phase composition of the resulting washed sample Phase composition Run Experimental conditions Si sl SII Na.sub.4Si.sub.24 Ta or Au Ta.sub.xSi.sub.y Quenching experiments PL695 6 GPa, 675/1075 K S M W 0.5/1.5 h PL702 6 GPa, 675/1075 K S M M 0.5/3.5 h PL703 6 GPa, 675/1075 K S M M 0.5/1.5 h PL704 3 GPa, 675/1075 K W W S 0.5/11.5 h PL705a 6 GPa, 675/975 K S M 0.5/3.5 h Slow-cooling experiments PL706 6 GPa, 675/1125 K W S 0.5/5.5 h PL708 3 GPa, 675/975 K W S 0.5/5.5 h PL713 8 GPa, 675/1075 K W S 0.5/5.5 h SamiPC1 1 GPa, 1075 K S M 24 h PC1015 2 GPa, 1125 K M W 6 h(33 at % Na) PC1028 1.2 GPa, 875 K M 2 h(33 at % Na) PC1037 2 GPa, 925 K, 2 h S M M PC1047b 2 GPa, 1025 K, 2 h S M Direct transformations. PC1047a 2 GPa, 1025 K S M 2 h(Na.sub.8Si.sub.46) * If not mentioned otherwise, the initial Na/Si mixtures contained 20 at % of Na. S (strong) - predominant phase, M (medium) - one of major phases, W (weak) - secondary phase/contamination. The format is: Preheating temperature (or time)/Heating temperature (or time).
[0049] As shown in
[0050] Powder X-ray diffraction (PXRD) from samples recovered between 2 and 6 GPa revealed the formation of sI clathrate. The presence of a small amount of silicon in the recovered samples likely indicates the peritectic character of the NaSi phase diagram under pressure, with the peritectic reaction L.sub.Na/Si+Si=Na.sub.8Si.sub.46. Two dimensional X-Ray diffraction data indicated the presence of both primary grown clathrate crystals and fine-grained powder formed during eutectic crystallization (see
TABLE-US-00003 TABLE S3 Structural refinement data for Na.sub.8Si.sub.46 and NaSi.sub.6. Different fits for a given structure correspond either to the model of ideal stoichiometry (Fit 1) or to possible non-stoichiometry of Na positions (Fit 2). Both models provide comparable fits indicating near-ideal stoichiometry. A decrease in Na occupancy leads to a decrease in the fitted U.sub.iso value. Na.sub.8Si.sub.46 Fit 1 .sup.2 = 0.260 .Math. 10.sup.2 wRp = 0.0449 (-Bknd) Rp = 0.0305 (-Bknd) Space group: Pm-3n (No 223) Lattice parameter: a = 10.208(1) Atomic coordinates x y z Occupancy U.sub.iso Si1 (6c) 0.25 0.5 0 1 0.012(6) Si2 (16i) 0.184(1) 0.184(1) 0.184 (1) 1 0.012(6) Si3 (24k) 0 0.118(1) 0.308(1) 1 0.012(6) Na4 (2a) 0 0 0 1 0.042(30) Na5 (6d) 0.25 0 0.5 1 0.051(20) Fit 2 .sup.2 = 0.257 .Math. 10.sup.2 wRp = 0.0443 (-Bknd) Rp = 0.0289 (-Bknd) Space group: Pm-3n (No 223) Lattice parameter: a = 10.208(1) Atomic coordinates x y z Occupancy U.sub.iso Si1 (6c) 0.25 0.5 0 1 0.012(6) Si2 (16i) 0.184(1) 0.184(1) 0.184(1) 1 0.012(6) Si3 (24k) 0 0.118(1) 0.308(1) 1 0.012(6) Na4 (2a) 0 0 0 1.0(1) 0.043(30) Na5 (6d) 0.25 0 0.5 0.95(6) 0.032(30) NaSi.sub.6 Fit 1 .sup.2 = 0.866 .Math. 10.sup.2 wRp = 0.0322 (-Bknd) Rp = 0.0500 (-Bknd) Space group: Cmcm (No 63) Lattice parameters: a = 4.106(3), b = 10.563(9), c = 12.243(9) Atomic coordinates x y z Occupancy U.sub.iso Na1 (4c) 0 0.285(5) 0.25 1 0.061(20) Si2 (8f) 0 0.245(3) 0.549(1) 1 0.017(6) Si3 (8f) 0 0.566(2) 0.347(1) 1 0.017(6) Si4 (8f) 0 0.027(2) 0.594(1) 1 0.017(6) Fit 2 .sup.2 = 0.845 .Math. 10.sup.2 wRp = 0.0327 (-Bknd) Rp = 0.0508 (-Bknd) Space group: Cmcm (No 63) Lattice parameters: a = 4.106(3), b = 10.563(9), c = 12.243(9) Atomic coordinates x y z Occupancy U.sub.iso Na1 (4c) 0 0.284(4) 0.25 0.93(6) 0.043(30) Si2 (8f) 0 0.245(3) 0.549(1) 1 0.018(6) Si3 (8f) 0 0.565(2) 0.346(2) 1 0.018(6) Si4 (8f) 0 0.028(2) 0.594(1) 1 0.018(6)
[0051] While sI was always observed between 2 and 6 GPa under quasi-equilibrium conditions of slow cooling (2-10 K.Math.min-1), the rapid quench of the system to ambient temperature (by abruptly switching off the heating power) led to the recovery of both sI and sII phases. Fast and/or lower temperature treatment of the reacting mixture may also occasionally lead to a combination of sII and diamond-Si, without remarkable traces of sI clathrate (see
[0052] When the pressure was increased to 8 GPa, the formation of a novel NaSi compound, Na.sub.4Si.sub.24, was observed. As shown in
[0053] As compared to Ba.sub.4Si.sub.24(31), Sr.sub.4Si.sub.24(32) and Ca.sub.4Si.sub.24(33), the corresponding sodium compound forms at substantially lower pressure: 8 GPa as compared to 11.5 and 10 GPa for BaSi.sub.24 and CaSi.sub.24, respectively. The pressure for Na.sub.4Si.sub.24 formation allows consideration of this phase for a large-volume production, for example, in the toroid-type high-pressure systems,(34) contrary to the alkali-earth metal analogues.
[0054] The electrical resistivity of a polycrystalline piece of 500500 m.sup.2 of Na.sub.4Si.sub.24 was measured as a function of temperature by the standard four-electrode technique, using a Physical Property Measurement System (PPMS: Quantum Design, Inc.). Overall, Na.sub.4Si.sub.24 exhibits metallic behavior, with the electrical resistivity decreasing with decreasing temperature (see
[0055] The observed minimum at about 75 K on the resistivity curve for Na.sub.4Si.sub.24 might be caused by the particularities of the electronic band structure and by an unknown scattering process. The present results suggest that the resistivity increase in Na.sub.4Si.sub.24 at very low temperatures (formal value of .sub.300K/.sub.2K for Na.sub.4Si.sub.24 is 6) is not due to structural defects, intergrain boundaries, or an experimental artifact (the low-temperature resistivity curve of sI does not show such behavior,
[0056] While the formation of sI clathrate and Na.sub.4Si.sub.24 directly from the elements indicates high-pressure thermodynamic stability of these phases, the inventors performed density functional theory (DFT) calculations (38) in order to further elucidate the nature of their stability. Geometry optimizations were performed within the framework of the generalized gradient approximation (GGA) with the Perdew-Burke-Ernzerhof (PBE) parametrization (39) for the exchange-correlation functional implemented in Quantum Espresso. For Brillouin zone integration, the inventors used the Monkhorst-Pack scheme(40) and checked convergence of ground-state calculations with uniformly increasing k-point meshes for each structure. The inventors used a plane-wave basis set cutoff of 60 Ry and generated a 888 k-point grid meshed for a Brillouin zone integration (41). Calculations of phonons of Na.sub.4Si.sub.24 were performed with density functional perturbation theory with a uniform 444 mesh.
[0057] Density functional theory (DFT) calculations reveal that Na.sub.4Si.sub.4, sI, sII, and Na.sub.4Si.sub.24 are all stable against decomposition into the elements at high-pressure conditions (see
[0058] Density functional theory calculations suggest that sII clathrate is the stable ground state from 0 to 4 GPa, yet experiments performed below 2 GPa resulted in the recrystallization of Si. At ambient pressure, the inventors calculate sII to be more stable than Na.sub.4Si.sub.4+Si by 2.5 meV/atom, whereas sII is more stable than sI-Si by 5.2 meV/atom. At 4.2 GPa, the inventors calculate sI to become more stable than sII. The absence of sII in quasi-equilibrium experiments and the lack of this clathrate phase on the ambient-pressure binary NaSi phase diagram are in apparent disagreement with our calculations; however, enthalpy differences between these compounds are small. Finite temperature effects and kinetic barriers across the various phases may contribute to the differences observed. Nevertheless, the observation of sII in rapid-quench experiments certainly verifies the seemingly isoenthalpic nature of these phases.
[0059] The results open new perspectives for high-pressure synthesis and properties control of new advanced materials. The high-pressure thermodynamic stability of NaSi clathrate phases allows for a melt-based synthesis approach, which could be very useful for compositional control in mixed phases (e.g., Na+Ba, etc.), high-quality single crystals, and for precise tuning of the occupancy ratios. All phases formed in this pressure domain allow for larger-volume scaling of materials (from 40 cm.sup.3 for cubic sI at 3 GPa to 1 cm.sup.3 for the orthorhombic Eu.sub.4Ga.sub.8Ge.sub.16 structure at 8 GPa). The consistency of experimental results with ab initio calculations may justify the future application of this approach to the prediction of new covalent sp.sup.3 intercalation compounds (e.g., carbon-rich compounds). Finally, the results reveal the existence of multiple chemical mechanisms that allow for synthesis of high-pressure phases without pressure. Since the NaSi clathrates are stable only under high-pressure conditions (>2 GPa), previous reports of their synthesis may be viewed as nonequilibrium, precursor-based routes to high-pressure phases at low-pressure conditions. The understanding of such intrinsic interrelationships between thermodynamics and kinetics is thus the next step to explore that could open the potential for other precursor-based syntheses of high-pressure phases.
[0060] In addition to their innovations discussed above, the inventors have unexpectedly discovered that the new compound Na.sub.4Si.sub.24 is an excellent precursor in the production of another new compound Si.sub.24.
[0061] In one embodiment of the invention, the Na.sub.4Si.sub.24 compound may be subjected to dynamic vacuum conditions at modest temperatures to remove the sodium atoms and produce a sodium-free version of the compound: Si.sub.24 (also named oC24 silicon or Cmcm-24 silicon).
[0062] Si.sub.24, never before discovered or described in a publication, has an orthorhombic structure. The lattice constants are as follows: a=3.83 , b=10.69 and c=12.63 . This material is semi-conducting with an indirect band gap of 1.30 eV and a direct band gap of 1.34 eV. Si.sub.24 is a significantly better absorber of sunlight than d-Si.
[0063] The Si.sub.24 structure of silicon is produced by treating the Na.sub.4Si.sub.24 precursor under vacuum conditions (.sup.110.sup.2 torr) at elevated temperature (.sup.130 C.) for a preferred period of several days. At conditions of only 80 C. and no vacuum (ambient pressure), sodium atoms start to leave the Na.sub.4Si.sub.24 structure. At 110.sup.5 torr and 130 C. for 4 days, no sodium is detectable by energy dispersive spectroscopy measurements (EDS).
[0064] As shown in
[0065] The sodium content was also verified by using energy dispersive spectroscopy (EDS) on a scanning electron microscope (SEM).
[0066]
[0067] Density functional theory calculations were performed to confirm the stability of the Si.sub.24 structure and to further investigate the electronic band structure.
[0068] The light absorption of Si.sub.24 relevant to solar applications was also calculated.
[0069] The studies discussed herein have been motivated by the potential to find new silicon allotropes with advanced optical and electronic properties beyond those of d-Si [B4, B8, B16-B18]. In particular, photovoltaic applications ideally require a direct band gap of .sup.1.3 eV [B6], which has not been achieved by any existing silicon phase. Theoretically, low-energy silicon allotrope candidates were suggested that exhibit greatly improved visible light absorption characteristics with quasidirect band gaps (nearly degenerate indirect and direct gaps) [B4, B8]; however, no experimental synthesis was reported thus far. Of the known metastable Si allotropes, the BC8 structure is likely semi-metallic [B17] and the R8 structure was calculated to possess a small indirect gap of 0.24 eV [B16]. Lonsdaleite silicon, produced by heating the BC8 structure above 470 K, has an indirect gap of .sup.1 eV [B16, B17] and the crystal structure of allo-Si is not clearly resolved [B19]. Type-II silicon clathrate, Si.sub.136, possesses a wide band-gap of 1.9 eV [B18], which is not suitable for photovoltaic applications. In addition, symmetry analysis of the cubic Si.sub.136 structure shows that electric dipole transitions associated with this gap are forbidden [B20].
[0070] Silicon-rich compounds may be considered as another route for synthesizing novel classes of silicon allotropes. This approach was used previously for the synthesis of type II silicon clathrate [B13] and germanium clathrate [B19], both of which utilize chemical precursors that are formed at ambient pressure. In this discovery, applicants considered using compounds recovered from high-pressure conditions as chemical precursors, rather than using compounds formed at ambient pressure. In this case, the synthesis of entirely new, previously inaccessible phases become possible by performing ambient-pressure chemical manipulations on inherently metastable materials recovered from high pressure. Applicants disclose herein the formation of Na.sub.4Si.sub.24 above .sup.8 GPa, and the concomitant metastable recovery of this phase to ambient conditions [B5]. This compound consists of a channel-like sp.sup.3 silicon host structure filled with linear Na chains as a guest structure. These open channels that host Na suggest a possible pathway for Na removal via diffusion along the channels as schematically shown in
[0071] By exposing recovered Na.sub.4Si.sub.24 samples to elevated temperatures, removal of Na from the structure was observed. This process occurs at temperatures as low as 320 K, while type-II silicon clathrates (Na.sub.xSi.sub.136) require much higher temperatures (>623 K) for Na removal [B13, B21]. Thermal degassing of Na.sub.4Si.sub.24 at 400 K under dynamic vacuum resulted in a gradual reduction of the Na content and Na was completely removed from structure over a period of eight days.
[0072] The absence of sodium was also demonstrated using energy-dispersive X-ray spectroscopy (EDXS). EDXS measurements were performed on degassed samples of Na.sub.xSi.sub.24 (0x4) (
[0073] Si.sub.24 possesses an orthorhombic structure (Cmcm, space group 63) with lattice parameters a=3.825(1) , b=10.700(2) , and c=12.648(2) . There are three non-equivalent Si positions (discussed in more detail below) and each Si atom is connected tetrahedrally with bond lengths ranging from 2.33 to 2.41 , as compared with the bond length of d-Si (2.35 ). Along the a-axis, Si.sub.24 possesses octagonal linear channels, which were occupied by Na in Na.sub.4Si.sub.24. To maintain the void space, the bond angles are distorted in a range from 93.7-135.9, deviated from the perfect tetrahedral angle (109.5). The low density of Si.sub.24 (2.16 g/cc), due to its high nanoporosity, is between that of d-Si (2.33 g/cc) and Si.sub.136 clathrate (2.15 g/cc).
[0074] The thermodynamic and dynamic stability of the new silicon phase was investigated using first principles calculations. Total energy calculations using density functional theory (DFT) show that Si.sub.24 possesses a higher enthalpy than d-Si by 0.09 eV/atom and is energetically more favorable than other known metastable BC8 and R8 phases [B4]. Phonon dispersion relations for Si.sub.24, obtained from lattice dynamics calculations (Supplementary Information, see below), indicate that this structure is dynamically stable at both high- and low-pressure conditions. This fact demonstrates that the removal of sodium atoms from Na.sub.4Si.sub.24 does not affect the lattice stability of the Si framework. At ambient pressure, the Si.sub.24 lattice maintains dynamic stability, which is consistent with our experimental observations at ambient conditions. In our calculations, Si.sub.24 is destabilized above 10 GPa and we speculate that it might transform to the metallic Si-II (-tin) structure, similar to type-II Si clathrate, above 12 GPa [B22].
[0075] To gain further insight into the properties of Si.sub.24, the electronic band structure was calculated. Using DFT, Si.sub.24 was calculated to have a direct band gap (E.sub.d) of 0.57 eV and an indirect band gap (E.sub.i) 0.53 eV (Supplementary Information, see below). The difference between E.sub.d and E.sub.i is small, albeit formally an indirect band gap material. The highest valence and the lowest conduction bands are very flat in the F-Z direction, indicating a quasidirect gap nature for Si.sub.24. It is a well-known limitation of standard DFT to underestimate the band gap of silicon. Therefore, we used quasiparticle (G.sub.0W.sub.0) calculations for accurate band gap estimations. Under this approach, we successfully reproduced the indirect gap value of 1.12 eV for d-Si (1.17 eV from experiment) and found that the G.sub.0W.sub.0 corrected E.sub.d and E.sub.i for Si.sub.24 are 1.34 eV and 1.30 eV, respectively (
[0076] The temperature dependence of the electrical conductivity , for Si.sub.24, is shown in
[0077] Optical reflectivity measurements were performed on samples of Si.sub.24 in order to obtain absorption information from the powder samples and to further evaluate the band gap.
[0078] To check for potential improvements in light absorption properties, we calculated absorption spectra of Si.sub.24 as shown in
[0079] Applicants have presented the discovery of a new allotrope of silicon, Si.sub.24, formed through a novel high-pressure precursor process. The sodium concentration was found to be <0.1 atom %, the laboratory detection limit. Electrical resistivity and optical reflectivity measurements indicate that Si.sub.24 is a semiconductor with a band gap of .sup.1.3 eV, in excellent agreement with our first principles calculations. The difference between E.sub.d and E.sub.i is negligibly small (<0.1 eV) and both are well within the optical band gaps for photovoltaic applications (<1.5 eV), which is a unique property of this new silicon allotrope. It is interesting that the band gap of Si.sub.24 coincides with the theoretically proposed optimal value that maximizes solar conversion efficiency for a single p-n junction to 33.7%, namely the Shockley-Queisser limit [B6]. Therefore, Si.sub.24 appears to be a promising candidate for thin-film solar applications, which should be investigated further along with other properties such as carrier mobility and potential for light emission. The quasidirect nature of the band gap allows for greatly improved optical properties, while the material maintains advantages of silicon, e.g., potential for doping, oxide layer, etc. The synthesis of Si.sub.24 currently requires a high-pressure precursor, which places limitations on scalability for eventual applications. However, low-pressure methods such as chemical vapor deposition could enable larger scale production of Si.sub.24, as is the case for diamond [B29], another high-pressure phase. Furthermore, the unique nanoporous nature of this structure may be of interest for gas and/or lithium storage and for molecular-scale filtering applications. More broadly, Si.sub.24 expands the known allotropy in element fourteen and the novel high-pressure precursor synthesis approach suggests potential for entirely new materials with desirable properties.
Examples
Synthesis
[0080] Si.sub.24 was synthesized in a two-step process. In the first step, Na.sub.4Si.sub.24 was synthesized from a Na/Si mixture with 15 mol % Na. The mixture was ground in a ceramic mortar for one hour inside a high-purity Ar glovebox and loaded into a Ta capsule. The capsule was then introduced in a 14/8 multianvil assembly using a Re heater and ZrO.sub.2 insulation. Shorting between Ta and Re was prevented by employing Al.sub.2O.sub.3 tubes, and a WRe C-type thermocouple, imbedded in an Al.sub.2O.sub.3 plug, was used for accurate temperature control. The mixture was pressurized in a 1500 ton multianvil press at a rate of 10 bar/hour (oil pressure) to a pressure of 10 GPa and reacted at 800 C. in two steps: preheating at 400 C. for 30 min, in order to avoid a blow-out of the overheated Na, and reaction at the final temperature for one hour, after which the sample was quenched by switching off the power. The recovered sample was easily removed from the Ta capsule and washed with distilled water. The resulting product of the reaction was polycrystalline Na.sub.4Si.sub.24. In the second step, polycrystalline agglomerates of Na.sub.4Si.sub.24 were placed in a furnace under a dynamic vacuum of .sup.10.sup.5 Torr and degassed at 125 C. for 8 days in order to obtain the empty Si.sub.24 structure, which was subsequently washed thoroughly with water.
Powder X-Ray Diffraction
[0081] PXRD data were collected on Rigaku Rapid diffractometer with MoK radiation and curved area detector. The sample to detector distance was refined using a high purity silicon standard. Rietveld refinements were carried out using GSAS with EXPGUI software.
Electron Microscopy
[0082] EDXS measurements were performed using JEOL JSM-6500F microscope equipped with Oxford Instruments X-max detector (80 mm.sup.2) and the data were analyzed using the Aztec software.
Electrical Measurements
[0083] Electrical resistivity was measured with a Physical Property Measurement System (PPMS) from Quantum Design using a two-probe method. Platinum wires (5 m) were attached to the dense polycrystalline specimens (.sup.50 m in size) using Leitsilber conductive silver cement (Ted Pella, silver content 45%, sheet resistance: 0.02-0.04 ohms/square).
Optical Reflectivity
[0084] Optical reflectivity measurements were performed on polycrystalline powder samples of Si.sub.24 using the near/mid IR light source from an Agilent Cary 670 spectrometer. Reflected light was focused into a dispersive spectrometer with CCD detector. A PTFE standard was used as a reflectance reference. Reflectivity data were processed under the Kubelka-Munk formalism and band gaps were estimated from Tauc plots.
First-Principles Calculations
[0085] For accurate band gap estimations, we have employed quasi-particle calculations (GW) and a hybrid functional approach (HSE06) for a comparison. We used Bethe-Salpeter equation (BSE) to compute the Coulomb correlation between the photoexcited electrons and holes. The full details of first principles calculations, with complete references, can be found in the Supplementary Information.
Supplementary Information
Electronic Structure Calculations
[0086] Electronic structure calculations and ionic relaxation were performed using Density Functional Theory (DFT) [C1, C2] with the Generalized Gradient Approximation (GGA) and Perdew, Burke, and Ernzerhof (PBE) exchange-correlation functional [C3, C4], as implemented in the Quantum ESPRESSO software [C5]. Applicants used a plane-wave basis set cutoff of 60 Ry and a Brillouin-zone integration grid of a 161616 k-points.
Crystal Structure
[0087]
TABLE-US-00004 TABLE 4 Crystallographic data for Si.sub.24. Si.sub.24 - full profile refinement, MoK.sub.a Space group Cmcm (#63) a () 3.8246(5) b () 10.7002(18) c () 12.6476(19) Atomic coordinates x y z Occupancy U.sub.iso Si1 (8f) 0 0.2427(8) 0.5553(5) 1 0.0176(11) Si2 (8f) 0 0.5718(6) 0.3439(6) 1 0.0176(11) Si3 (8f) 0 0.0295(6) 0.5918(5) 1 0.0176(11) Refinement statistics .sup.2 = 0.3889 .Math. 10.sup.2 wRp = 0.0859 (-Bknd) Rp = 0.0486 (-Bknd)
TABLE-US-00005 TABLE 5 Crystallographic data for Si.sub.24 (DFT, PBE) Si.sub.24 - DFT, PBE calculations, 1 atm Space group Cmcm (#63) a () 3.8475 b () 10.7443 c () 12.7342 Atomic coordinates x y z Occupancy Si1 (8f) 0 0.24285 0.55476 1 Si2 (8f) 0 0.57130 0.34274 1 Si3 (8f) 0 0.02862 0.59056 1
Band-Gap and Absorption Calculations
[0088] Applicants calculated band gaps for d-Si and Si.sub.24 using several computational approaches to make it clear that Si.sub.24 is a quasidirect band gap semiconductor. It is well-known issue that standard Density Functional Theory (PBE here) underestimates the band gap of materials. GW (where G means the single-particle Green's function and W the screened Coulomb potential) calculations were performed to correct the PBE band gap values and the Bethe-Salpeter equation (BSE) [C6, C7] was used to compute the Coulomb correlation between the photoexcited electrons and holes using the ABINIT software [C8]. Applicants conducted GW.sub.0 calculations with the cutoff dielectric matrix of 5 Hartree, which was tested to various semiconductors and insulators successfully [C9]. Applicants applied BSE calculations to d-Si for testing convergence of the calculations and then calculated Si.sub.24. For BSE calculations, applicants used a cutoff of 3.0 Hartree for the dielectric matrix.
[0089] The GW approximation was applied to the self-energy [C10, C11, C12] (the proper exchange-correlation potential acting on an excited electron or hole), which can be written as the product of the one-electron Green's function times the screened Coulomb interaction =iGW. In our calculations, applicants have used both single shot GW(G.sub.0W.sub.0) and partially self-consistent GW.sub.0. It is worth noting that full correction to both G and W (GW) on d-Si overestimated the band gap significantly [C13]. As shown in Table 6, for d-Si, G.sub.0W.sub.0 and GW.sub.0 give excellent agreement with the experimental band gap for d-Si (1.17 eV) and in the main text, applicants used G.sub.0W.sub.0 results. The Heyd-Scuseria-Ernzershof (HSE) exchange-correlation functional [C14] was also tested by us, which is more accurate for large band gap materials.
TABLE-US-00006 TABLE 6 Calculated band gaps for d-Si and Si.sub.24 using various functionals. Units are in eV. d-Si, Si.sub.24, indirect indirect (direct) PBE 0.62.sup.b 0.53 (0.57) HSE06 1.28.sup.a 1.41 (1.45) G.sub.0W.sub.0 1.12 1.30 (1.34) GW.sub.0 1.2.sup.b 1.43 (1.46) .sup.aRef [C15], .sup.bRef [C9]
Lattice Parameter Change with Respect to Sodium Concentration
[0090] Applicants calculated the lattice parameters, a, b, and c for Na.sub.xSi.sub.24 (0x4) at different values of x. Supercells of Si.sub.24 unit cells were constructed with only one sodium atom: 1x1x1 (x=0.25), 2x1x1 (x=0.125), 3x1x1 (x=0.083). Atomic positions were relaxed to determine the influence of Na content on the lattice parameters. Theoretical optimizations are in excellent agreement with experimental data for Na.sub.4Si.sub.24 and Si.sub.24 (
Metal-Insulator transition in Na.sub.xSi.sub.24
[0091] Computationally, applicants checked if Na.sub.xSi.sub.24 becomes a semiconductor at low values of x.
Phonon Dispersion Relations
[0092] Phonon calculations were performed using Density Functional Perturbation Theory [C16], as implemented in the Quantum-espresso package. The electronic wave function was expanded with a kinetic energy cutoff of 60 Ry. A Uniform with a 666 q-point mesh of phonon momentum has been calculated with a 121212 k-point mesh.
[0093] The dynamical stability of Si.sub.24 was examined at ambient pressure and at 10 GPa.
Raman Scattering
[0094] Raman scattering data were collected from degassed samples Si.sub.24. A 532 nm diode laser was used as an excitation source and focused onto the sample using a 20 long working distance objective lens. The power at the sample was approximately 10 mW. Scattered radiation was collected in the 180 back-scatter geometry and focused onto a 50 m confocal pinhole, which served as a spatial filter. This light was then passed through two narrow-band notch filters (Ondax, SureBlock) and focused onto the entrance slit of a spectrograph (Princeton Instruments, SP2750). Light was dispersed off of an 1800 gr/mm grating and recorded using a liquid nitrogen-cooled charge-coupled device detector (Princeton Instruments, Plyon).
[0095] The Raman active mode was calculated using density functional perturbation theory [C17]. A Brlliouin zone sampling grid with 20.04 .sup.1 was used with a plane basis set cutoff of 500 eV. The ionic positions were carefully relaxed at ambient pressure.
Uniaxial Compression Effect on the Band Gap
[0096] Strictly speaking, Si.sub.24 is an indirect band gap material, however, electronic dispersion relations show nearly flat bands along the to Z direction. Due to the small difference between E.sub.d and E.sub.i, applicants examined band gap changes during uniaxial compression of Si.sub.24 along c-axis. The difference between the direct and indirect band gaps (E.sub.d.Math.E.sub.i) is shown in
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[0184] As the present invention may be embodied in several forms without departing from the spirit or essential characteristics thereof, it will be understood that the invention is not limited by the details of the foregoing description, unless otherwise specified, but rather should be construed broadly within its spirit and scope as defined in the appended claims, and therefore all changes and modifications that fall within the metes and bounds of the claims. Accordingly, the invention is defined by the appended claims.