Md. Zahidur Rahaman and
A. K. M. Akther Hossain*
Department of Physics, Bangladesh University of Engineering and Technology, Dhaka-1000, Bangladesh. E-mail: akmhossain@phy.buet.ac.bd; zahidur.physics@gmail.com
First published on 24th September 2018
Non-toxic metal halide perovskites have become forefront for commercialization of the perovskite solar cells and optoelectronic devices. In the present study, for the first time we show that particular metal doping in CsGeCl3 halide can considerably enhance the absorbance both in the visible and ultraviolet light energy range. We have carried out DFT based first principles calculations on Mn-doped and Ni-doped CsGeCl3 halide. We investigate the detailed structural, optical, electronic and mechanical properties of all the doped compositions theoretically. The study of the optical properties shows that the absorption edge of both Ni and Mn-doped CsGeCl3 is shifted toward the low energy region (red shift) relative to the pristine one. An additional peak is observed for both doped profiles in the visible light energy region. The study of the mechanical properties demonstrates that both the doped samples are mechanically stable and ductile as the pristine CsGeCl3. The study of the electronic properties shows that the excitation of photoelectrons is easier due to the formation of intermediate states in Mn-doped CsGeCl3. As a result Mn-doped CsGeCl3 exhibits higher absorptivity in the visible region than the Ni-doped counterpart. A combinational analysis indicates that CsGe1−xMnxCl3 is the best lead free candidate among the inorganic perovskite materials for solar cell and optoelectronic applications.
The well known formula of metal halide perovskites is ABX3 (where, A = a cation, B = a metal ion and X = a halogen anion). The majority of the materials which exhibit remarkable performances in this family contain lead (Pb). Therefore, the major concern for application of these materials in practice is the toxicity of Pb. In ambient conditions lead based metal halide perovskites decompose to PbI2 which is harmful to the environment.7–9 Hence, several theoretical and experimental studies have been carried out in recent years in the quest to find novel non-toxic perovskites by replacing lead with a non-toxic metal cation. Recently Roknuzzaman et al. carried out a detailed investigation on this group of materials by using theoretical methods to find a suitable lead free candidate.10 They performed a simulation study the structural, optical, electronic and mechanical properties of CsBX3 (B = Ge, Sn and X = Cl, Br, I) semiconductors and compare their results with the lead containing semiconductors CsPbX3 (X = Cl, Br, I). After a combinational analysis they suggest that Ge-based CsGeI3 metal halide is the best lead free inorganic metal halide perovskite semiconductor for optoelectronic and solar cell applications. However, the study of the mechanical properties shows that the proposed sample is brittle in nature and hence unsuitable for real world application.
In 2016, Erdinc et al. studied the electronic, optical, thermodynamic and lattice dynamical properties of CsGeCl3 semiconductor for both paraelectric and ferroelectric phases.11 Another experimental and theoretical study suggests that CsGeCl3 is a wide band gap semiconductor with an experimental band gap value of 3.67 eV.12–15 Because of this large band gap value CsGeCl3 metal halide is not perfect for solar cell application. However, an appropriate metal dopant in CsGeCl3 can reduce the band gap to such extent which is suitable for the absorption of visible light energy. Therefore, in the present study we aim to dope with different transition metals the Ge-site of the CsGeCl3 metal halide in order to extend its absorption spectra across all the range of the solar spectrum. We have studied the optical, electronic and mechanical properties of Ni and Mn-doped CsGeCl3 by using a Density Functional Theory (DFT) based theoretical method to find a better candidate in this family for solar cell and optoelectronic applications than the previously proposed best lead free candidate CsGeI3. Finally, a thorough comparison among the key properties of the metal doped CsGeCl3 and pristine CsGeCl3 with the CsGeI3 metal halide is presented and discussed in details.
Finite strain theory21 executed within the CASTEP module is used for evaluating the elastic constants of pristine and doped CsGeCl3 metal halide. We set 0.003 as the maximum strain amplitude. Voigt–Reuss–Hill (VRH) averaging scheme22 is used for obtaining the polycrystalline mechanical parameters from the evaluated Cij. The polycrystalline elastic moduli are calculated by using the equations given elsewhere.23 The optical properties are calculated by using the CASTEP tool based on the standard DFT Kohn–Sham orbitals.24 A scissor operator of 2.673 eV is applied in the calculation in order to compensate for the gap between the theoretical value (0.997 eV) and experimental value (3.67 eV) of the pure CsGeCl3 band gap.
Fig. 1 The crystal structure (2 × 2 × 2 supercell) of CsGeCl3 metal halide. (a) Three dimensional and (b) two dimensional view. |
The evaluated absorption profiles of pristine and doped CsGeCl3 are illustrated in Fig. 2. The optical absorption coefficient is defined as the fraction of energy (wavelength) absorbed per unit length of the material and provides crucial information about the efficiency of optimum solar energy conversion of a material. Fig. 2(a) exhibits the photon energy dependent absorption coefficient of both pure and doped CsGeCl3. According to the result, the absorption edge of both Ni and Mn-doped CsGeCl3 is shifted toward the low energy region (red shift) relative to the pristine one. An additional peak is observed for both doped profiles in the low energy region. The absorption edge of Mn-doped CsGeCl3 shifts more toward the lower energy region than Ni-doped CsGeCl3. The pristine CsGeCl3 shows no absorbance in the visible light region. The metal doping in pure CsGeCl3 enhances the absorption coefficient to a great extent not only in the visible region but also in the ultraviolet region. For a better understanding of the light absorption feature of CsGeCl3 in the visible region, the wavelength dependent absorption coefficient is presented in Fig. 2(b). As shown in Fig. 2(b) the Mn-doped CsGeCl3 has a wider absorption area than the Ni-doped CsGeCl3. The reason for the formation of the broadest absorption area in the Mn-doped sample will be discussed in details in the next section. In general, wide band gap semiconductors can absorb ultraviolet light of the solar spectrum which is only 4% of the total solar energy coming to the earth.26 The visible light covers approximately 43% of the solar spectrum.27 Therefore, the intrinsic CsGeCl3 (band gap = 3.67 eV) is incapable to utilize the visible light energy for photovoltaic conversion. Hence, the prominent absorption in the visible region in the Mn-doped sample shows great promise for better utilization of the solar spectrum and may increase the solar cell efficiency.
Fig. 2 Calculated light absorption spectra of pure and metal doped CsGeCl3 perovskite. (a) Photon energy dependent and (b) wavelength dependent absorption coefficient. |
Reflectivity is one of the crucial optical properties of materials for photovoltaic applications and is defined as the amount of light energy reflected from the surface of a material with respect to the amount of light energy incident on the surface of the material. The reflectivity spectra of pristine and doped samples for photon energy up to 30 eV are illustrated in Fig. 3(a). CsGeCl3 shows low reflectivity in the whole energy range of the solar spectrum. However, the reflectivity of all metal doped samples is nearly identical to the pristine one in the ultraviolet region. An additional peak is observed in the visible region for all doped samples whereas Mn-doped CsGeCl3 has a stronger reflectivity in the low photon energy range than the Ni-doped sample. The dielectric function is characterized by the response of a material to the incident light energy. The charge carrier recombination rate and hence the overall performance of optoelectronic devices depends upon the static value of the dielectric function.28 A material with high dielectric constant has relatively less charge carrier recombination rate. As a result the overall performance of optoelectronic devices is enhanced. The real and imaginary part of the evaluated dielectric function of pure and doped CsGeCl3 are depicted in Fig. 3(c) and (d). It is evident that the Mn-doped sample shows relatively higher dielectric constant than the pure and Ni-doped CsGeCl3. Therefore, in terms of dielectric constant Mn-doped CsGeCl3 is a better candidate for solar cell and optoelectronic applications than the pristine one. Generally a material with a higher band gap exhibit lower dielectric constants.29 Since metal doping in CsGeCl3 decreases the band gap value (see Electronic properties section), the metal doped samples show a higher dielectric constant than the pure CsGeCl3. As shown in Fig. 3(c) and (d) overall the dielectric profile (both real and imaginary part) of the metal doped samples is almost identical in the high energy region (ultraviolet zone) to that of the pure sample. An additional peak of the real part of the dielectric constant is observed in the visible light energy zone. The imaginary part of the dielectric constant of all the samples goes to zero above 19 eV while the real part reaches approximately unity. This result implies that both doped and pure CsGeCl3 halide exhibit transparency with slight absorption in the high energy zone (above 19 eV) (it is also evident from the absorption coefficient graph [Fig. 2(a)]). The appearance of a sharp peak of the imaginary part of the dielectric constant of the metal doped sample in the visible region implies the occurrence of strong absorption in this region30 which also justifies the result obtained from the absorption spectra of doped CsGeCl3 [Fig. 2]. Therefore, the investigation of the dielectric constant of the pure and metal doped CsGeCl3 suggests that both pristine and doped sample possess high transmissivity in the high energy region (above 19 eV) and metal doped samples possess nearly zero transmissivity in the visible region. This is the reason for high absorptivity of metal doped CsGeCl3 (particularly Mn-doped CsGeCl3) in the visible region. However, the study of the reflectivity spectra [Fig. 3(a)] shows that Mn and Ni-doped CsGeCl3 have a slight higher reflectivity in the visible energy zone. Hence, further research should be conducted to reduce the reflectivity of the metal doped CsGeCl3 in the visible region which may further increase the absorptivity as well as efficiency of the solar cells. The optical conductivity is also defined as the photoconductivity. The conductivity spectra of doped and pristine CsGeCl3 are illustrated in Fig. 3(b) up to 25 eV light energy. The optical conductivity of the metal doped CsGeCl3 is almost similar to that of the pure sample in the high energy region. A sharp peak appeared in the visible light energy zone for both doped profiles whereas the Mn-doped sample exhibits a larger photoconductivity than the Ni-doped sample. The appearance of the large photoconductivity in the visible region for the metal doped CsGeCl3 is a consequence of its large absorptivity in the low energy region [Fig. 2].
Fig. 4 The band structure diagram of CsGeCl3 metal halide calculated by using (a) pure single cell, (b) pure supercell, (c) Ni-doped and (d) Mn-doped sample. |
The total and partial density of states of pristine and doped CsGeCl3 are depicted in Fig. 5. Fig. 5(a) illustrates the DOS profile of the pure sample. As shown in the figure the valence band is mostly composed of Cl-3p and Ge-4p orbitals with a small contribution of Cs-6s and Cs-5p orbitals. The conduction band mainly consists of Ge-4p orbital with a small contribution of Cs-6s and Cs-5p orbitals. After Ni doping in CsGeCl3 a slight change is observed in the overall DOS profile as shown in Fig. 5(b). The composition of the valence band is almost similar to that of the pristine sample except for an extra peak which appeared in the total DOS due to the formation of dopant states (Ni-3d) in the valence band of CsGeCl3. The composition of the conduction band is similar to the pristine one as no dopant peak is formed. A similar trend is observed for the Mn-doped sample as shown in Fig. 5(c). The conduction band slightly shifts toward the lower energy region. A flat peak is observed in the conduction band due to the formation of dopant states (Mn-3d) in the conduction band. Fig. 5(d) illustrates the change of the band gap due to the formation of new dopant states near the Fermi level. In case of Ni-doped CsGeCl3 the impurity energy states are formed over the Fermi level and mixed with the valence band maximum. These impurity states can trap the photoexcited holes which reduce the recombination rate of electrons and holes.32 In case of Mn-doped CsGeCl3 the impurity energy states appear in the middle of the band gap. These intermediate states reduce the energy which is necessary for electron transition to occur from the valence band to the conduction band. The valence electrons are first excited to the impurity energy states (intermediate band) and then excited to the conduction band by consuming the visible light energy. These results explain the red shift of the absorption spectra as shown in Fig. 2.
Fig. 5 The total and partial density of states of CsGeCl3 metal halide simulated by using (a) pure supercell, (b) Ni-doped sample, (c) Mn-doped sample and (d) dopant contribution at the Fermi level. |
C11 > 0, C44 > 0, C11 − C12 > 0 and C11 + 2C12 > 0 |
Phase | C11 | C12 | C44 | C12–C44 |
---|---|---|---|---|
CsGeCl3 | 55.02 | 13.14 | 11.73 | 1.41 |
CsGe1−xNixCl3 | 54.16 | 14.60 | 13.36 | 1.24 |
CsGe1−xMnxCl3 | 56.68 | 14.36 | 13.33 | 1.03 |
CsGeCl3 (ref. 10) | 54.93 | 13.08 | 11.99 | — |
Hence, both the doped phases are mechanically stable in nature. It is also evident that the calculated elastic constants of pristine CsGeCl3 (by using supercell) agrees well with the available theoretical result bearing the reliability of the present investigation. The Cauchy pressure (C12–C44) is a useful parameter to predict the brittleness and ductility of materials. The negative (positive) value of this parameter indicates the brittle (ductile) nature of a compound.30 The computed values of the Cauchy pressure of pristine and doped samples are positive [Table 2] implying that the doped samples are ductile as the pristine CsGeCl3.10
By using the computed elastic constants the most important mechanical parameters of a compound such as the shear modulus G, bulk modulus B, Young’s modulus E, B/G ratio and Poisson’s ratio ν of pristine and doped samples are calculated and listed in Table 3. It is also evident from Table 3 that all the calculated mechanical parameters show good consistency with the theoretically calculated results. The bulk modulus is one of the essential mechanical parameter which gives an indication of the stiffness of a material. The calculated bulk modulus of all the composition is comparatively low indicating the flexibility of all the samples. The value of B is slightly increased after Ni and Mn doping. However, this lower value of B ensures that it will be easier to make thin films of Mn-doped CsGeCl3 perovskite and hence suitable for solar cell applications. The shear modulus is used to calculate the plastic deformation of a material under external stress. As shown in Table 3 the value of G for all the samples is comparatively low. The value of G is slightly increased after Ni and Mn doping into CsGeCl3. However, the lower value of the shear modulus implies that CsGe1−xMnxCl3 is less rigid than the pristine sample and hence can be drawn into a desired shape. A similar trend is noticed for the Young’s modulus of all the compositions.
Phase | B (GPa) | G (GPa) | E (GPa) | ν | B/G |
---|---|---|---|---|---|
CsGeCl3 | 27.11 | 14.82 | 37.60 | 0.26 | 1.82 |
CsGe1−xNixCl3 | 27.78 | 15.63 | 39.48 | 0.26 | 1.77 |
CsGe1−xMnxCl3 | 28.46 | 16.05 | 40.53 | 0.26 | 1.77 |
CsGeCl3 (ref. 10) | 27.03 | 15.02 | 38.02 | 0.27 | 1.80 |
The Poisson’s ratio is another useful parameter for explaining the bonding nature and plasticity of a material. The calculated value of ν for all the compositions is 0.26 implying the existence of a central force in all the samples.34 However, all the samples should have predominant ionic feature as the value of ν is very close to the critical value of 0.25 which indicates an ionic crystal. The Poisson’s ratio is another useful indicator of ductility and brittleness of materials. The critical value for separating the ductility and brittleness of a material is 0.26.35 Surprisingly the computed value of ν of all the samples is exactly 0.26 thus implying the ductile nature of all the compositions. The ratio between bulk modulus and shear modulus is usually known as Pugh’s ratio which is also used to predict the failure mode of a material. In this case, the critical value for separating the ductility and brittleness of a material is 1.75.36 As shown in Table 3 all the studied compositions are ductile in nature as the value of B/G is greater than the critical value. The value of B/G is decreased after Ni and Mn doping in CsGeCl3. However, the value of Pugh’s ratio of metal doped CsGeCl3 perovskite is still greater than the critical value and hence should exhibited a ductile response as the pristine sample.
According to the present study, a small amount of Ni dopant in the Ge site of CsGeCl3 can elevate the absorption in the visible region to a great extent. However, the Mn-doped CsGeCl3 exhibits a very high absorption not only in the visible region but also in the ultraviolet region. The study of the mechanical properties shows that the proposed sample is ductile and possesses a low bulk modulus and hence it is possible to use it to make thin films. It also possesses high photoconductivity. The comparison among the key properties of pure and metal doped CsGeCl3 with CsGeI3 is presented in Table 4. From Table 4 it is clear that CsGe1−xMnxCl3 is the best lead free candidate among the inorganic perovskite materials for solar cell and optoelectronic applications.
Properties | CsGeCl3,10 [this work] | CsGeI3 (ref. 10) | CsGe1−xNixCl3 | CsGe1−xMnxCl3 |
---|---|---|---|---|
Optical absorption | High in UV-region | High in UV-region | High in UV-region | High in UV-region |
Missing in visible region | Medium in visible region | Medium in visible region | High in visible region | |
Photoconductivity | Medium | High | Medium | High |
Failure mode | Ductile | Brittle | Ductile | Ductile |
Suitability for solar cells | Not good | Good | Better | Best |
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