Abstract

We numerically investigate the impact of electron–phonon scattering on the optical properties of a perovskite material (CH3NH3PbI3). Using nonequilibrium Green function formalism, we calculate the local density of states for several values of the electron–phonon scattering strength. We report an Urbach-like penetration of the density of states in the band gap due to scattering. A physical analytical model allows us to attribute this behavior to a multiphonon process. Values of Urbach energy up to 9.5 meV are obtained, meaning that scattering contribution to the total experimental Urbach energy of 15 meV is quite important. We also show that the open-circuit voltage Voc, for a solar cell assuming such a material as an absorber, depends on the scattering strength. Voc loss increases with the scattering strength, up to 41 mV. Finally, an unexpected result of this study, is that the impact of electron–phonon scattering on Urbach tail and Voc increases with the phonon energy. This low value in perovskite (8 meV) is therefore an advantage for photovoltaic applications.
Introduction
Perovskite materials are widely studied for both device conception and theoretical understanding. Among the variety of perovskites materials, organic–inorganic hybrid perovskites are the most promising materials for optoelectronic applications. First, photovoltaic cells made of hybrid perovskites lacked stability and had a low solar conversion efficiency, of the order 3%. Nowadays, fabrication techniques of perovskites have been largely improved, making them more stable and reliable to use in solar cells. Production costs have also been drastically reduced, paving the way to further decrease the PV electricity price.1 This fast evolution of technology has led to an increase of efficiency, up to 24% in less than 10 years,2 and have reached over 28% in Si-perovskite tandem devices.3
Hybrid perovskite represents one of the most promising materials for reliable solar conversion technology, thanks to their excellent optical and electrical properties. They exhibit high carrier diffusion lengths, reaching up to 1 μm even in nanostructures.4 High carrier lifetime has also been measured to be around several microseconds.5 Moreover, it has been shown that hybrid perovskites have remarkable photon absorption properties.6 These properties have also been observed in perovskite layers as thin as 50 nm.7 The main advantage of such thin films is to be integrated in lightweight, flexible, and transparent solar cells8 that could find applications in wearable electronics.
However, remarkable properties of these materials cannot be fully understood considering the peculiar structure of hybrid perovskites. On the one hand, with these excellent carrier-transport properties, we could expect hybrid perovskites to exhibit high carrier mobilities. Yet, several groups have reported low values for carrier mobilities in perovskite-based devices. Mei et al. found mobilities of 1 cm2/(V s) in a field-effect transistor.9 Shi et al. estimated the electron mobility in a single crystal to be 115 cm2/(V s)10 Microwave conductivity measurements gave carrier mobilities from 6 to 60 cm2/(V s).11,12 These measured values are quite low compared to mobilities in other inorganic materials used in PV cells (electron mobility is equal to 1500 cm2/(V s) in silicon) and could indicate some disorder in the crystalline structure. On the other hand, it is possible to extract information about the quality of the material from the absorption features below the band gap. The Urbach rule gives the absorption coefficient below the band gap as a function of photon energy and temperature. It is described by a “tail” with the expression
| 1 |
where α0 is a constant, Eg is the material band gap, hν is the incident photon energy, and EU is the Urbach energy, corresponding to the width of the exponential part of the absorption below the band gap. This empirical formula is an important tool to study the optical absorption due to its simplicity and applicability for various types of materials and structures. This phenomenon has three principal physical causes which are the crystal disordering,13 trap states due to impurities14 and electron–phonon scattering (EPS).15,16 Depending on the type of material, one of these causes dominates. In amorphous material, the Urbach energy, which can reach up to 50 meV,17 is mainly due to disordering, while in well-ordered materials like GaAs, the Urbach energy, which is as low as 7.5 meV,18,19 is mainly due to the EPS. In the case of hybrid perovskite-based device, the Urbach energy has been estimated experimentally to be 15 meV.20 However, the origin of this band tail is still debated in the literature. In ref (21), the authors attribute the latter to the presence of trap states in the band gap. The understanding of this behavior is important since it modifies the characteristic of the corresponding solar cell with a Stokes shift and impacts the open-circuit voltage Voc.22 The definition of the optical band gap can also be discussed.23,24
In hybrid perovskites, the scattering with polar optical phonons is expected to be large since (i) the difference between ϵ∞ and ϵstat (the dynamic and the static dielectric constant respectively) is large25 and (ii) the small phonon energy implies a large number of phonons (all parameters are reported in Table 1). Moreover, rotations of the CH3NH3 organic matrix may play a key role in quantum transport properties.26 Random rotations of cations induce fluctuations of the electrostatic potential. Electrons and holes in the material become localized and spatially separated, affecting their transport properties and the corresponding mobilities. It can then be expected that EPS also impacts the Urbach tail.
Table 1. Constant Parameters of CH3NH3PbI3.
| parameter | value |
|---|---|
| me*/m0 | 0.23 |
| mh*/m0 | 0.17 |
| ϵ∞ | 6.0 |
| ϵstat | 29.0 |
| Epop (meV) | 8.0 |
Numerical study of Urbach tail assumes that the acoustic phonon has already been conducted.16 Recently, using nonequilibrium Green’s functions (NEGF) formalism,27 impurities and EPS have been considered to allow to reproduce the band tail and the band gap narrowing in a nanowire. Using the same formalism,28 in the present work, we numerically study the impact of the polar optical phonon on the optical and electrical properties of hybrid perovskite materials. We show that such an interaction modifies the electronic density of states (DOS), leading to the enhancement of an Urbach tail in the band gap. To better interpret our results, we develop an original analytical model of the DOS in the band gap. This model is in good agreement with the numerical results assuming only well-known material parameters such as effective masses, electron–phonon coupling, and phonon energy. It also allows to illustrate that the Urbach tail due to polar optical phonon is related to a multiphonon process. Finally, calculations of the absorption and the emission current contributions allow to estimate the variation of Voc with respect to the EPS strength.
Methodology
To study the impact of EPS, we made numerical calculations using NEGF formalism within the self-consistent Born approximation.29 This model is detailed in ref (28), but we recall here the main elements needed for an easier understanding. We consider a three-dimensional (3D) device, with wide transverse dimensions perpendicular to the transport axis. This allows to assume a one-dimensional (1D) model in the longitudinal direction for each transverse mode corresponding to a propagation in the transverse plane with a given transverse wave vector. In our case, we consider Nkt = 30 transverse modes. For each mode, we define a Hamiltonian Hkt, in the 1D site basis using the effective mass approximation, which is suitable for the study of most crystalline material, including perovskite.30 This allows to calculate the corresponding lesser G<(E, kt) and greater G>(E, kt) Green’s functions, relative to electron and hole densities, respectively. The DOS in both conduction and valence bands is given by the retarded Green function GR(E, kt). We consider the diagonal approximation to describe the EPS and assume the effective mass approximation for both conduction and heavy-hole valence bands. To make the calculations with such formalism, we need to take the band diagram of the device as well as the EPS strength and phonon density as input data in our code. For calculations in a solar cell, the band diagram, relative to electric field and band offset, is obtained by the Poisson–Schrödinger self-consistent approach. To do so, we implemented the structure in SCAPS software.31 SCAPS is a solar cell simulation program that calculates the optical and electronic characteristics of multilayer semiconductor devices based on a drift-diffusion model. In our case, we have used SCAPS to extract data relative to the band diagram of our device as an input file of our Green’s function simulations.
In such a polar material, polar optical phonons dominate the carrier transport. While the model of Sarangapani et al. includes scatterings with both polar optical phonon and charged impurities, and Grein et al. assumed only acoustic phonons, we then only assume the polar optical phonons. The strength of this electron–phonon interaction is given by
| 2 |
where S is the surface of the transverse cross section of radius R = 30 nm; Epop is the polar optical phonon energy of the material; ϵ0 is the vacuum permittivity; and ϵ∞ and ϵstat are the relative dynamic and static permittivities, respectively. All used parameters are given in Table 2. CEPS is a numerical fitting factor, which is adjusted to a value such that the model accounts for the correct value of the electron mobility.32 The relation between CEPS and mobility is shown in Table 2. Electron mobility in hybrid perovskites has been experimentally measured from 1 to 100 cm2/(V s). Mechanisms controlling the carrier mobility in this material are not clearly understood, since the CH3NH3 molecular rotations could have an impact on carrier-transport properties.26 From a formalism point of view, these rotations are close to the electron–phonon interaction, but with unknown parameters. In the following, we perform calculations with 4 different values of CEPS corresponding to mobilities ranging from 0.13 to 86 cm2/(V s) as reported in the literature.
Table 2. Numerical Values of the Scattering Strength Multiplicative Coefficient, with the Estimated Electron Mobility and Calculated Urbach Energy.
| CEPS | μe– (cm2/(V s)) | EU (meV) |
|---|---|---|
| 1.6 | 86 | 5.25 |
| 5.0 | 18 | 6.6 |
| 10.0 | 1.7 | 7.9 |
| 20.0 | 0.13 | 9.5 |
The number of phonons per unit cell
is given by the Bose–Einstein distribution
| 3 |
where E = Epop = 8 meV and T = 300 K in the case
of phonons in CH3NH3PbI3. Since Epop is small in the considered perovskite material
(compared to kBT = 25.7
meV and compared for example to the GaAs value of 35 meV),
is large. We consider the EPS by calculating
the corresponding interaction self-energies
| 4 |
| 5 |
where Mt(kt, kt′) is the intermode coupling matrix, which depends on
both considered modes kt and kt and on Mpop.33Equation 4 describes the interaction with electrons,
while eq 5 accounts for
those with holes. Terms in
correspond to phonon absorption, while
terms in
correspond to phonon emission. Calculations
of self-energies are self-consistent, since G< and G> also depend on these
self-energies28
NEGF calculations allow us to estimate the current generated by the cell in the dark as well as under illumination. From current calculations, we can thus deduce the relation between Voc and EPS.
The electrical characteristic of a solar cell is close to the diode characteristic. In the dark, the current generated by the cell is given by
| 6 |
where I0 is the current relative to recombination of majority carriers in the cell for a bias V = 0 V. In the dark, I0 compensates the minority carrier current and the total current is zero. Under illumination, the current in the cell at a bias V can be estimated by
| 7 |
where Isc is the short-circuit current of the cell, which is the photocurrent at zero bias. Here, we consider that the photocurrent does not depend on the bias V. It is then possible to estimate the open-circuit voltage Voc only with the Green’s functions calculated at V = 0 V
| 8 |
Voc is calculated for each value of CEPS, and each Voc is compared to the ballistic counterpart (CEPS = 0) to estimate δVoc, the losses due to EPS. Isc and I0 are calculated using
| 9 |
and
| 10 |
where
is a band coupling parameter,34E is the electron energy, hν is the photon energy, and Ω is the solid
angle of the light source, which is equal to 6.79 × 10–5sr for Isc and π sr for I0.
is the Bose–Einstein distribution
of photons (see eq 3)
at the energy hν and temperature Tsun = 6000 K and ρ(hν) iss
the photon DOS per unit energy and unit volume
| 11 |
I0 depends on G<(E + hν) and G>(E), which are the electron density at energy E + hν and the hole density at energy E, respectively. An electron in the conduction band can recombine with a hole in the valence band, emitting a photon of energy hν. On the other hand, eq 9 shows that Isc depends on G<(E) and G>(E + hν), which are the electron density at energy E and the hole density at energy E + hν. An electron in the valence band can interact with a photon with energy hν to populate a state in the conduction band.
Results and Discussion
Density of States
Figure 1 shows the local DOS calculated in a solar cell with an hybrid perovskite active region. We performed the calculations with a CEPS corresponding to an electron mobility of 86 cm2/(V s) and in the ballistic approximation (CEPS = 0). The two situations are compared in Figure 1. In the ballistic case, quantum tunneling leads to a small but finite penetration of the DOS in the band gap. This DOS distribution has been shown to impact the optical properties of ultrathin solar cells.35 By comparison, the presence of EPS strongly enforces the penetration of DOS within the band gap, which largely dominates the one induced by quantum tunneling. The presence of these near-band-edge states allow both electrons and holes to be either photogenerated or recombined at energies lower than the material band gap of 1.55 eV. To illustrate the evolution of broadening with the interaction strength, we have also made local DOS calculations for each value of the scattering strength. Figure 2 shows these DOS in the middle of the device versus the electron energy. The DOS tends to penetrate deeper in the band gap as the EPS becomes stronger.
Figure 1.

Local density of states in a perovskite-based device (shown above) as a function of position and electron energy, calculated (a) with electron–phonon interaction and (b) without electron–phonon interaction.
Figure 2.

Logarithm of the density of states as a function of electron energy at a fixed position in the middle of the active region of the perovskite-based device. Each color corresponds to a different scattering coupling strength, and thus to a different value of electron mobility.
To get some physical insight, we developed an analytic model showing the relative importance of the various parameters. The gap density of states is related to the imaginary part of the retarded Green’s function
| 12 |
where Ekt is the energy of the band edge
(we consider here the conduction band) and
. Using eqs 4 and 5 and
the approach developed in ref (33), we can write Γkt in a continuous form
| 13 |
which is valid for small electron concentrations. As shown in the Supporting Information (eqs S5 and S9), this set of equations can be reduced to
| 14 |
with
.
This is a set of ladder equations,
which are related to multiphonon
process, leading to an exponential decrease of large negative energies.
In this regime, |E| ≫ Epop and eq 14 become a simple differential equation, valid at large
. To solve it, we use the expected exponential
behavior by writing D(E) = A exp(σ(E)) and incorporate
it into eq 14 together
with a first-order expansion σ(E ± Epop) = σ(E) ± σ′(E)Epop. With this, all terms
in σ(E) disappear and, by expanding exp(±σ′(E)Epop) to second order and
keeping the dominant term in |E|, one gets
| 15 |
whose integration gives
| 16 |
This depends upon two basic parameters Epop and EMt. Note that it depends upon 1/Mt linearly. This analytical expression is compared to the full numerical result in Figures 3 and 4, showing an excellent agreement at large energies, apart from a shift due to the constant. In particular, we confirm that the slope of the Urbach tail is proportional to Epop and also to EMt3/4, which is linear in Mt and one that can relate to the mobility.
Figure 3.

Density of states in the considered device as a function of the electron energy. Each color corresponds to a value of the EPS strength (and therefore of the electron mobility). Plain lines correspond to the self-consistent calculations. Dashed lines correspond to the calculated DOS using eq 16. The conduction band edge has been shifted in energy to 0 eV.
Figure 4.

Density of states in the considered device as a function of the electron energy. Each color corresponds to a value of the optical phonon energy. Plain lines correspond to the self-consistent calculations. Dashed lines correspond to the calculated DOS using eq 16. The conduction band edge have been shifted in energy to 0 eV.
As seen before, DOS tends to penetrate deeper in the band gap as the scattering with optical phonons becomes more important. Another interesting and unexpected result shown Figure 4 is that the polar optical phonon energy also plays an important role. The higher ithe phonon energy, the deeper the DOS expands below the band edge. This result confirms the fact that the DOS penetration in the gap is due to the multiphonon process. While with a smaller Epop, the impact of scattering is expected to be larger, because the number of phonons increases, we show that the consequence on the DOS is smaller. From the Urbach tail point of view, the low value of Epop in perovskites appears to be finally an advantage.
Urbach Energy
Using our results, we can now estimate the Urbach energies by calculating the exponential decay of the absorption coefficient α. Starting from the calculation of the photogenerated current Isc (eq 9), we obtain α expressed as a function of the photon energy hν
| 17 |
where L is the thickness of the device; ve(hν) is the group velocity of electrons generated by a photon of energy hν; and a and dhν are the numerical steps in position and energy, respectively. Applying this procedure to GaAs,19 we find the Urbach energy of 8 meV, which is in good agreement with the experimental value of 7.5 meV.18 For the perovskite, Figure 5 shows α for each CEPS as a function of the photon energy. It confirms the Urbach-like exponential decrease of the DOS inside the band gap, which is all the more severe as EPS is large. The corresponding Urbach energies are reported in Table 2. Despite the very low Epop, the calculated EU are not negligible, up to 9.5 meV, compared to the experimental value of 15 meV. Yet, this value is generally explained by crystalline disorder; our result shows that EPS also impacts the Urbach behavior. However, contrary to the disorder, scattering with phonons is intrinsic and, therefore, unavoidable.
Figure 5.

Absorption coefficient α (solid lines) versus photon energy calculated for each value of the electron–phonon scattering strength. Colored dashed lines correspond to the slopes used to calculate Urbach energies. Black dashed line correspond to the band gap of CH3NH3PbI3 at 1.55 eV.
Emission and Voc
Figure 6 shows the calculated emission spectra for each value of the scattering strength, calculated with eq 10. We report both a red shift and an increase of the intensity with the EPS strength. This is another consequence of the DOS penetration. Electrons in the conduction band can occupy the states below the bottom of conduction band to recombine with holes above the top of valence band, emitting photons of lower energies than the material band gap. In an efficient photovoltaic device, we want to absorb as many photons as possible while preventing electron–hole recombinations as much as possible. To quantify the impact of scattering on the open-circuit voltage, we calculate the ratio of absorption to emission (needed in eq 8). Figure 7a shows the calculation of this ratio as a function of CEPS. The ratio decreases for higher values of phonon coupling. The penetration of the DOS due to EPS therefore favors the recombination and thus the photon emission. This confirms that the degradation of the sharpness of the absorption coefficient due to Urbach tail tends to deteriorate the quality of the material for photovoltaic applications.23 Decrease of the absorption-to-emission ratio with the EPS can be linked to the Urbach behavior. Corresponding values of δVoc are also shown in Figure 7b. We then confirm that Voc decreases with the EPS up to 41 mV for the highest CEPS, therefore for the lowest mobility. Fortunately, this degradation is limited by the low value of Epop in the studied perovskite material. However, this value is not negligible and such a behavior is intrinsic and generalizable to all semiconductors.
Figure 6.

Emission spectra calculated for each value of the electron–phonon scattering strength.
Figure 7.
Top: Isc/I0 ratio for each value of CEPS considered. Bottom: Voc losses due to electron–phonon scattering for each value of CEPS considered.
Conclusions
In this paper, we studied the impact of the electron–phonon scattering on optical and electrical properties of an hybrid perovskite. Our numerical calculations showed that electron–phonon scattering induces a penetration of the density of states in the band gap, which increases with the scattering strength. Such modifications induce an energy shift of the emission spectra, since photogenerated electrons and holes can recombine at lower energies than the material band gap. We have also investigated the Urbach effect induced by electron–phonon scattering. We obtained values of Urbach energies from 5.25 to 9.5 eV, which means that phonon scattering contributes significantly to the exponential decrease of absorption below the band gap. The analytical description of the density of states shows that the Urbach tail is due to the multiphonon process, implying an unexpected dependence on the phonon energy. The low value of this energy in the considered material appears to be an advantage. Finally, we calculated the open-circuit voltage Voc for each scattering strength compared to the ballistic counterpart. We obtained Voc losses up to 41 mV due to the electron–phonon scattering. To tweak the results concerning the impact of electron–lattice interactions on the optical and electrical properties, a more precise inclusion of CH3NH3 rotations should be led. Moreover, the study of the influence of temperature can also provide relevant information about the carrier-transport properties in such materials.
Supporting Information Available
The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsomega.9b03178.
(PDF)
The authors declare no competing financial interest.
Supplementary Material
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