Shengzi
Zhang
ab,
Lei
Kang
*a and
Zheshuai
Lin
*ac
aTechnical Institute of Physics and Chemistry, Chinese Academy of Sciences, Beijing 100190, China. E-mail: kanglei@mail.ipc.ac.cn; zslin@mail.ipc.ac.cn
bUniversity of Chinese Academy of Sciences, Beijing 100049, China
cCenter of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
First published on 3rd July 2020
We propose a series of novel ASnX (A = Na, H; X = N, P) layered structures based on first-principles modeling and simulation. These nanosheet materials are all derived from the rational design for the parent structures of NaSnX (X = N, P) with unique divalent tin lone electron pairs. First-principles calculations show that the polar divalent tin effect can lead to strong second-order nonlinear optical (NLO) and large birefringence response in bulk materials, and can also greatly enhance the second harmonic generation (SHG) effect in the corresponding two-dimensional (2D) nanostructures by hydrogen passivation or strain engineering. The correlation between structural evolution and bandgap is illustrated through detailed analysis of the electronic structure and charge transfer model. The SHG effect and its origin can be further evaluated based on the SHG-weighted density scheme, which will facilitate the NLO research of 2D materials in the nitride and phosphide systems.
In this work, different from the 2D structural characteristics of metal chalcogenides, we attempt to construct 2D NLO layered structures in nitride and phosphide systems by introducing the polar lone electron pairs (LEP) into the covalent framework. This design proposal is mainly based on the following three reasons: (i) Nitride and phosphide-family semiconductors can exhibit wide bandgap range and strong SHG effects, such as GaN (≈3 eV, 5 pm V−1), ZnGeP2 (≈2 eV, 70 pm V−1) and GaAs (≈1 eV, 110 pm V−1);10–12 (ii) Polar effect of LEPs could enlarge the second-order NLO response such as the SHG effect (e.g., in BiB3O6 with Bi3+ LEP) and shift-current effect (e.g., in CsPbI3 with Pb2+ LEP);13,14 and (iii) LEP might enhance the layered structural stability to some extent due to the stable dangling bonds between layers.
By screening nitride and phosphide compounds from the inorganic crystal structure database (ICSD), we have focused on a series of non-centrosymmetric layered structures with divalent tin (i.e., Sn2+) LEP effect, including ASnX (A = Na, K; X = N, P, As, Sb).15–18 We selected two representative structures including NaSnN and NaSnP as the initial crystal models for the first-principles design. Accordingly, we have systematically investigated the SHG properties and structural stabilities of their bulk and 2D materials. Detailed analysis of the structure–property correlations provides important clues for us to understand the origin of SHG effects. Our study can play a positive role in promoting the development of 2D NLO materials in the nitride and phosphide systems.
Based on the optimized structure, the electronic energy bands, partial density of states (PDOS), atomic charge and orbitals are obtained. Further, the linear (e.g., refractive indices n and birefringence Δn) and NLO (e.g., static SHG coefficients dijk = χijk/2) properties are calculated. The SHG coefficients herein are calculated using the following expression:24
χαβγ = χαβγ(VE) + χαβγ(VH) + χαβγ(TB) |
Here, α, β and γ are Cartesian components, v and v′ denote valence bands, and c and c′ denote conduction bands. P(αβγ) denotes full permutation and explicitly shows the Kleinman symmetry of the SHG coefficients. The band energy difference and momentum matrix elements are denotes as ℏωij and pαij, respectively, and they are all implicitly k dependent.
The screened exchange local density approximation (sX-LDA) method is employed to accurately (in particular for the narrow-gap semiconductors) predict the energy bandgaps Eg,25 and LDA is used to calculate the optical properties corrected by the scissor operator, which is set as the difference between LDA and sX-LDA bandgaps.26,27 This self-consistent ab initio approach has been proven to be effective to investigate the optical properties in many types of NLO materials without introducing any experimental parameter.19 Note that the SHG coefficients of 2D materials are related to the thickness (unit is Å pm V−1). For comparison, herein we use relative SHG effect, defined as the SHG effect per unit thickness (unit is pm V−1), to evaluate the NLO performance of ML structures.
Based on the proposed method, we have calculated the energy bandgaps and SHG properties for the important NLO systems of ZnGeP2 and MoS2 as the benchmark for bulk and ML, respectively. It is demonstrated that the calculated results as listed in Table 1 are in good agreement with the experimental measurements (relative error < 10%).
System | E g (eV) | d ijk (pm V−1) by our method | n o | n e | Δn | |||
---|---|---|---|---|---|---|---|---|
By LDA | By sX-LDA | At 2 μm | ||||||
a Ref. 11. b Ref. 5. c Strain is 10%. d Strain is 15%. | ||||||||
ZnGeP2 | Bulk | Cal. | 1.39 | 2.02 | d 123 = 65 | 3.291 | 3.325 | 0.033 |
Bulk | Exp. | 2.00 | 2.00 | d 123 = 70 (@10.6 μm)a | 3.149 | 3.189 | 0.040 | |
MoS2 | ML | Cal. | 1.86 | 2.05 | d 111 = −d122 = 149 | — | — | — |
ML | Exp. | 1.80 | 1.80 | ≈520 × SiO2 (d222 = 0.3 for SiO2)b | — | — | — | |
NaSnN | Bulk | Cal. | 1.14 | 1.34 | d 113 = d223 = −2.7; d333 = 27 | 3.160 | 2.531 | 0.629 |
HSnN | ML | Cal. | 0.72 | 1.08 | d 111 = −d122 = 147; d113 = d223 = −46; d333 = −11 | — | — | — |
NaSnN | MLc | Cal. | 0.18 | 0.15 | d 111 = −d122 = 129; d113 = d223 = 491; d333 = 489 | — | — | — |
MLd | Cal. | 0.66 | 0.76 | d 111 = −d122 = 102; d113 = d223 = 301; d333 = 277 | — | — | — | |
NaSnP | Bulk | Cal. | 0.61 | 1.10 | d 113 = d223 = 6.2; d333 = 16 | 3.391 | 2.947 | 0.445 |
ML | Cal. | 0.81 | 0.87 | d 111 = −d122 = 203; d113 = d223 = 618; d333 = 533 | — | — | — | |
HSnP | ML | Cal. | 1.74 | 2.18 | d 111 = −d122 = 12; d113 = d223 = −6.3; d333 = −14 | — | — | — |
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Fig. 1 Unit cell structure of NaSnX (X = N, P) (a), covalent ML structure of SnX with Na embedded (b), structural evolution from surface (c) to hydrogen-passivated surface (d) and HSnX ML (e). |
An interesting structural feature is that the interlayer cations Na+ are attracted to the adjacent N3− from the lower layer but are repelled by the adjacent Sn2+ from the upper layer, which results in the weak connection between adjacent NaSnN layers. First-principles calculations for Mulliken bond population (MBP) as listed in Table 2 show that there are anti-bonds (MBP < 0) between Na+ and Sn2+ while weak covalent bonds (MBP ≈ 0.17, bond length L ≈ 2.47 Å) between Na+ and N3−.28
System | Sn–X bond | A–X bond | A–Sn bond | A atom | X atom | Sn atom | |||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
MBP | L (Å) | MBP | L (Å) | MBP | L (Å) | MAP | Charge | MAP | Charge | MAP | Charge | ||
a Hydrogen-passivated surface. b Strain is 10%. c Strain is 15%. | |||||||||||||
NaSnN | Bulk | 1.54 | 2.07 | 0.17 | 2.47 | −1.04 | 3.22 | 8.37 | 0.63 | 6.09 | −1.09 | 3.54 | 0.46 |
ML | 1.18 | 2.12 | 0.07 | 2.38 | — | — | 8.62 | 0.38 | 6.12 | −1.12 | 3.26 | 0.74 | |
Surface | 1.67 | 2.08 | −0.10 | 2.51 | — | — | 8.80 | 0.20 | 6.10 | −1.10 | 3.23 | 0.77 | |
Inner layer | 1.55 | 2.05 | 0.14 | 2.52 | −1.13 | 3.23 | 8.42 | 0.58 | 6.11 | −1.11 | 3.46 | 0.54 | |
Surfacea | 0.85 | 2.11 | 0.68 | 1.04 | — | — | 0.71 | 0.29 | 6.12 | −1.12 | 3.31 | 0.69 | |
Inner layer | 1.54 | 2.05 | 0.14 | 2.52 | −1.11 | 3.25 | 8.43 | 0.57 | 6.11 | −1.11 | 3.46 | 0.54 | |
HSnN | ML | 0.74 | 2.12 | 0.60 | 1.03 | — | — | 0.67 | 0.33 | 6.18 | −1.18 | 3.15 | 0.85 |
NaSnN | MLb | 1.05 | 2.28 | 0.16 | 2.42 | — | — | 8.58 | 0.42 | 6.04 | −1.04 | 3.38 | 0.62 |
MLc | 0.99 | 2.35 | 0.17 | 2.47 | — | — | 8.56 | 0.44 | 6.02 | −1.02 | 3.42 | 0.58 | |
NaSnP | Bulk | 1.69 | 2.51 | 0.34 | 2.89 | −1.25 | 3.87 | 8.57 | 0.43 | 5.62 | −0.62 | 3.81 | 0.19 |
ML | 1.41 | 2.55 | 0.26 | 2.74 | — | — | 8.56 | 0.44 | 5.73 | −0.73 | 3.72 | 0.28 | |
HSnP | ML | 1.19 | 2.53 | 0.65 | 1.43 | — | — | 0.96 | 0.04 | 5.41 | −0.41 | 3.63 | 0.37 |
The band structure and PDOS of bulk NaSnN are plotted in Fig. 2a, showing that it is an indirect-gap semiconductor. The ionic Na–N coupling and covalent Sn–N hybridization lead to the bandgap between valence bands (VB) and conduction bands (CB). The other orbitals in the top of VB and the bottom of CB are composed by the s orbitals of Sn, which are mainly non-bonding states contributing to the LEP effect.
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Fig. 2 Band structures and PDOS of NaSnN bulk (a), ML (b), surface (c), hydrogen-passivated surface (d), HSnN ML (e), 15%-strained NaSnN ML (f), NaSnP bulk (g), NaSnP ML (h) and HSnP ML (i). |
Table 1 lists the bandgap Eg, SHG coefficients dijk, refractive indices no, ne and birefringence Δn of bulk NaSnN. Its bandgap calculated by sX-LDA is 1.34 eV, within the suitable bandgap range of promising photovoltaic materials. The SHG coefficient d113 (or d223) is relatively small (≈2.7 pm V−1), since it mainly originates from the in-plane polarization of the layered orbitals but the polarization directions for the upper and lower layers are opposite. As a comparison, the d333 caused by the polar LEP effect along the c-axis is much larger (≈27 pm V−1), which can be confirmed from the analysis of SHG-weighted density as shown in Fig. 3a. Based on the SHG-weighted charge density analysis tool developed by our group, the SHG coefficient is “decomposed” onto the respective orbital or band according to a “band-resolved” scheme, and then the SHG-weighted bands are used to sum the charge densities of all occupied (OCC) or unoccupied (UNOCC) states.29 As a result, the electronic states irrelevant to SHG are not shown in the OCC or UNOCC SHG density, and the orbitals vital to SHG are highlighted in the real space. It is clearly illustrated from Fig. 3a (for details see Table S2 in the ESI†) that the SHG density is mainly located in the Sn and N atoms from the VE process, indicating that the dominant contribution of the SnN backbone with the LEP effect to the SHG effect. Moreover, the calculated birefringence is much larger (Δn ≈ 0.63) than most of NLO materials such as β-BaB2O4 (Δn ≈ 0.12), LiIO3 (Δn ≈ 0.17) and BiB3O6 (Δn ≈ 0.18), demonstrating that it has larger structural anisotropy and sufficient phase-matching ability for the effective NLO conversion.
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Fig. 3 SHG density of NaSnN bulk (a), HSnN ML (b), strained NaSnN ML (c), NaSnP bulk (d), NaSnP ML (e) and HSnP ML (f). |
Unfortunately, the bandgap of NaSnN ML is closed as shown from the band structure in Fig. 2b, demonstrating that it has become a semimetal from an insulator. The PDOS analysis further shows that the s orbitals of Sn and hybrid Sn–N p orbitals mainly contribute to the VB maxima, while the Na states make up the CB minima. This is mainly due to the relatively free Na+ that are not bound by the covalent layers. Detailed Mulliken atomic population (MAP) as listed in Table 2 shows that the charge transfer (≈0.38) from Na to SnN layer in the NaSnN ML is less than that in the NaSnN bulk (≈0.63), which results in the great decrease of bandgap in ML.
Note that the proper band gap is very important for NLO applications, especially for frequency conversion in transparent regions. Therefore, in order to open a bandgap so as to meet the requirement of NLO transparency, we have further designed NaSnN BL, trilayer (TL) and multilayer (e.g., 5L) as shown in Fig. S2a of the ESI† to enlarge the charge transfer between Na and SnN layer by increasing the number of layers. However, their bandgaps are still closed as shown from the band structures in Fig. S2b of the ESI,† because there is still little charge transfer (e.g., 0.27 for BL, 0.24 for TL, 0.21 for 5L from the calculations) between exposed Na and adjacent SnN, which causes the Na states still located around the Sn–N coupling gap from the PDOS analysis in Fig. S2c of the ESI.†
Note that eliminating the influence of substrate may be effective to improve the charge transfer of HSnN on the surface. Considering the weak interlayer connection between substrate NaSnN and covered HSnN, we theoretically peel off the covalent HSnN from the NaSnN substrate as a single layer as depicted in Fig. 1e. Analysis of MBP and MAP shows that the framework of HSnN ML is more covalent than that of NaSnN ML, and the charge transfer (≈0.33) between H and SnN for HSnN ML are more than that (≈0.29) of HSnN on the NaSnN substrate. Consequently, HSnN ML exhibits an opened bandgap (≈1.08 eV) by the sX-LDA calculation. Fig. 2e further shows that it is an indirect-gap semiconductor, and the states around the bandgap are mainly from the s orbitals of Sn and the hybrid p orbitals between Sn and N. The H orbitals are far from the bandgap, different from those states of free Na in the NaSnN nanosheets.
Table 1 lists the SHG coefficients of HSnN ML, in which the largest coefficient d111 (or d122) is in-plane and about 147 pm V−1, as large as that of MoS2 (cal. d111 ≈ 149 pm V−1, exp. d111 ≈ 158 pm V−1).5 Further from the analysis of SHG-weighted density as shown in Fig. 3b, the effect of d111 is mainly originated from the Sn LEP states in the VE process. In addition, the d113 (or d223 ≈ 46 pm V−1) becomes much larger than that of NaSnN bulk although the d333 becomes smaller (≈11 pm V−1). These SHG coefficients are also from the polar Sn2+ LEP along the c-axis, which MoS2 does not have. Moreover, the phonon vibration spectrum is calculated to confirm the structural stability of designed HSnN ML. The results are plotted in Fig. S3a of the ESI,† indicating that it is dynamically stable without any virtual frequency. Therefore, HSnN ML may be used as a possible 2D NLO structure that can exhibit strong SHG effect comparable to that of MoS2 ML.
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Fig. 4 Band evolution of NaSnN ML with strain varying from 0 to 15% (a), bandgap (b) and SHG effect (c) with respect to the strain. |
First-principles results from Table 1 demonstrate that NaSnP bulk exhibits a smaller indirect bandgap (≈1.1 eV) and SHG effect (d333 ≈ 16 pm V−1) than those (≈1.3 eV and 27 pm V−1) of NaSnN bulk. Its band structure and PDOS are shown in Fig. 2g, which is basically similar to the energy bands of NaSnN bulk with slightly different dispersion. Interesting, when stripped into the NaSnP ML, it exhibits an opened bandgap (≈0.87 eV) and huge SHG effects in d111 (≈203 pm V−1), d113 (≈618 pm V−1) and d333 (≈533 pm V−1). The SHG effects are much larger than those of HSnN ML (≈147 pm V−1) and MoS2 ML (cal. ≈149 pm V−1), and comparable to the strained NaSnN ML (≈300–500 pm V−1). This is mainly because that the covalent bonding between Na and (SnP) layer is relatively weaker than that between Sn and P. The further analysis demonstrates that the charge transfer (0.28) from P to Sn in NaSnP ML is more than that (0.19) in NaSnP bulk, which can enlarge the polar effect of Sn LEP and further enhance the SHG effect. It can be confirmed from Fig. 3d and e that, compared with the SHG density of NaSnP bulk, there is much stronger SHG density for d113 of NaSnP ML on the Sn LEP and P site in the main VE process. Meantime, different from those for NaSnN bulk, there is some density around Na atoms that also contributes to SHG effect in the VH process (see Table S2 in the ESI†). It can be also found from PDOS that the Na orbitals are relatively isolated at the bottom of CB. Moreover, these bands around the bandgap are flatter than those in bulk, exhibiting a quasi-direct gap, which is not only beneficial to the enhancement of SHG but also favorable to the optoelectronic applications.
In order to confirm the structural stability of strained NaSnN ML and NaSnP ML, the phonon spectra are obtained from first principles as shown in Fig. S3b and S3c of the ESI.† The results show that there exists a virtual frequency in the 15%-strained NaSnN ML, indicating that it may be a metastable structure. For NaSnP ML, the dispersion of the lowest vibration frequencies is normal without any virtual frequency. Thus, the NaSnP ML structure could exhibit the dynamical stability, and needs to be verified by the experiment.
Similar as HSnN ML, we can also design the HSnP ML structure. Unfortunately, its SHG effect (≈14 pm V−1) is much weaker than those of NaSnP systems although its bandgap (≈2.18 eV) is abnormally larger. This is because the SHG effect is mainly originated from the covalent SnP framework (see PDOS of Fig. 2i and SHG density of Fig. 3f), but the small anionic charge (−0.41 for P) and cationic charge (0.37 for Sn) as listed in Table 2 cause the electronic polarization to be weak and the SHG effect to be decreased. Moreover, it is metastable with a virtual frequency as shown in Fig. S3d of the ESI.† Thus, it cannot exhibit usable SHG effect like HSnN ML.
In addition to the dynamical stability, we also need to provide more clues to evaluate the structural rationality of HSnN and NaSnP ML materials. For such, the interlayer interaction energies of the two structures are calculated with respect to the interlayer distance as well as those of MoS2 as plotted in Fig. S4 of the ESI.† It is found that the interlayer binding energy for NaSnP (275 meV per atom) is larger than those of HSnN (115 meV per atom) and MoS2 (114 meV per atom), indicating that its nanosheet is more difficult to be cleaved than HSnN and MoS2. Meanwhile, the thermodynamic stability can be approximated by the formation energy, i.e., the difference in energy and the lowest value for any mixture of bulk materials. The calculations show that NaSnP has indeed higher formation energy (428 meV) than those of HSnN (172 meV) and MoS2 (133 meV).30 The cohesive energy, usually used to discuss the energetic stability of the structure, is also obtained by the difference between the energy of the dispersed gas of its constituent atoms (or molecules) and the energy of the crystal at absolute zero of temperature.31,32 The calculated cohesive energy decreases from MoS2 (7.8 eV per atom) to HSnN (6.0 eV per atom) and NaSnP (4.2 eV per atom), indicating that the energetic stability decreases from MoS2 to HSnN and NaSnP. The above results demonstrate that the NaSnP and HSnN nanosheets maybe more difficult to be obtained than MoS2.
Footnote |
† Electronic supplementary information (ESI) available: Tables S1, S2 and Fig. S1–S4. See DOI: 10.1039/d0nr03778h |
This journal is © The Royal Society of Chemistry 2020 |