The current thin-film photovoltaic technologies can be classified by the different materials used for the light absorption in a solar cell. These materials include amorphous and polycrystalline silicon, CdTe, CuInxGa1-xSe2(CIGS), GaAs, and photosensitive organic dyes. A transformative technology may emerge when a new and better material is being discovered for thin-film photovoltaic applications.
D. Scaife, P. Weller, and W. Fisher, reported an early study on the structural information of CsSnI3 compound in form of powders, J. Solid State Chem. 9, 308 (1974).
P. Mauersberger and F. Huber, synthesized a yellow, needle-like CsSnI3 microcrystal, and studied its crystal structure, Acta Cryst. B 36, 683 (1980).
K. Yamada, S. Funabiki, H. Horimoto, T. Matsui, T. Okuda, and S. Ichiba, reported the polymorph nature of CsSnI3compound, Chem. Lett. (The Chemical Society of Japan) 20, 801 (1991).
The black polymorph of CsSnI3 could be obtained through a phase transition from the yellow polymorph CsSnI3 by increasing its temperature above 425° K. It was further demonstrated by differential thermal analysis and X-ray diffraction that during the cooling of the black CsSnI3 from 450° K, its ideal cubic perovskite structure (B-α) deformed to a tetragonal structure (B-β) at 426° K, and became an orthorhombic structure (B-γ) below 351° K. Experimental studies of electrical and optical properties of this compound have been hindered by lack of high quality CsSnl3 samples either in bulk or thin film format.
Aiming at the unique properties of hybrid organic-inorganic perovskites based on tin halides, I. Borriello, G. Gantel, and D. Ninno, recently calculated band structures of B-α, B-β, and B-γ from the first principles using the crystal structures published by Yamada et al., Phys. Rev. B 77, 235214 (2008). It was concluded that all three structures had direct band-gap (Eg) at Z, R, and Γ points for B-α, B-β, and B-γ, respectively, with Eg (B-α)<Eg (B-β)<Eg (B-γ).
A need still exists in the industry for developing low cost synthesis methods for CsSnI3 thin films, especially in large scale. The successful implementation of these materials for various applications requires a detailed understanding of both their processing and materials properties.
This invention is directed to solution-based synthesis of cesium tin tri-iodide (CsSnI3) films. This invention is also directed to effective and inexpensive methods to synthesize the films on large-area substrates such as glass, ceramics, and metal foils.
One embodiment of this invention is directed to a process of forming CsSnI3 film on a substrate, comprising steps of:
Another embodiment of this invention is directed to a process of forming CsSnI3 film on a substrate, comprising steps of:
Yet, another embodiment of this invention is directed to CsSnI3 films synthesized on a substrate by any one of the processes disclosed above.
In the process, the steps are performed under ambient condition; the substrate is selected from glass, ceramic, silicon, and metal foils; a ratio of the CsI solution to the SnCl2 solution in the mixture ranges from about 1/10 to about 1/3.
The CsI solution is made by fully dissolving CsI powder (99.9% purity) in a solvent selected from the group consisting of water, deionized water, distilled water and mixtures thereof. The CsI solution is about 5 wt % to about 50 wt % CsI solution.
The SnCl2 solution is made by fully dissolving SnCl2 powder (99.9% purity) in a solvent selected from the group consisting of anhydrous alcohol, glacial acetic acid; ethylene glycol or triethylene glycol; and mixtures thereof. The SnCl2 solution is about 5 wt % to about 80 wt % SnCl2 solution.
U.S. patent application Ser. No. 13,151,243 discloses the vacuum-powder-based synthesis and characterization of CsSnI3 thin films. The precursor materials (powder) of CsI and SnCl2 (or SnI2) were alternately evaporated in a vacuum chamber on a substrate. The resulting CsSnI3 thin-film was formed after a post-deposition thermal treatment. The CsSnI3 thin films exhibit outstanding optical, electrical, and ferroelectric properties. These features make CsSnI3 thin films ideally suited for a wide range of applications such as light emitting and photovoltaic devices.
More specifically, U.S. patent application Ser. No. 13,151,243 discloses that CsSnI3 is a promising material in the application of thin-film solar cells, since CsSnI3 was found to possess a direct band gap of 1.32 eV at room temperature, right in the narrow region of optimal band gaps for the Shockley-Queisser maximum efficiency limit of a solar cell.
An effective and inexpensive method to synthesize large domain size high quality perovskite semiconductor thin films on large-area substrates such as glass, ceramics, silicon, and metal foils are disclosed in the present invention.
More specifically, a non-vacuum, solution-based method to synthesize CsSnI3 films is disclosed in the present invention. The films can be fabricated on inexpensive substrates such as glass, ceramics, silicon, and metal foils by the solution-based drop-coating. This non-vacuum-powder based demonstration of the CsSnI3 film formation further enhances the likelihood of using CsSnI3 as a new absorption material for solar cells.
The procedures of synthesizing polycrystalline CsSnI3 film using solutions were described.
The solutions of precursor materials were synthesized in ambient conditions. The ambient conditions refer to: room temperature or temperature of 298.15° K. (or 25° C., 77° F.); and an absolute pressure of 100 kPa (or 14.504 psi, 0.986 atm). The experimental setup was shown in
12 gram of CsI powder (99.9% purity) was added to 30 gram of deionized water to form 28.6 wt % (weight percent) CsI solution. The CsI powder was fully dissolved in deionized water. The CsI solution was stirred for 30 minutes.
CsI solution was colorless and stable in ambient conditions.
The CsI solution could comprise more CsI powder as long as the amount of CsI powder was fully dissolved in deionized water, and the CsI solution was colorless. CsI powder could dissolve in less than its own mass of water without apparent decomposition.
It would be apparent to one skilled in the art that CsI solutions could be made using any solvents other than those used in the examples. Examples of the solvent include but not limited to, water, distilled water, mixtures thereof.
The wt % range of the CsI solution was ranging from about 5.0 wt % to about 50.0 wt %, or from about 15 wt % to about 40 wt %.
An amount of 4 gram of SnCl2 powder (99.9% purity) was added to 20 gram of anhydrous ethanol to form 16.7 wt % of solution. The SnCl2 powder was fully dissolved in anhydrous ethanol to form the SnCl2 solution. The solution was stirred for 30 minutes.
SnCl2 solution was colorless and stable in ambient conditions.
The SnCl2 solution could comprise more SnCl2 powder as long as the amount of SnCl2 powder was fully dissolved in anhydrous ethanol, and the solution was colorless.
It would be apparent to one skilled in the art that SnCl2 solutions could be made using any solvents other than those used in the examples. Examples of the solvent include but not limited to, anhydrous alcohol, such as but not limited to, anhydrous methanol and anhydrous isopropyl; glacial acetic acid; ethylene glycol or triethylene glycol; and the mixtures thereof.
The wt % range of the SnCl2 solution was ranging from about 20 wt % to about 80%, or from about 10 wt % to about 50 wt %.
A given amount of the prepared CsI solution was transferred to a reaction vial first. SnCl2 solution was then slowly dropped into the vial by a pipet. The ratio of CsI solution to SnCl2 solution was in a range of about 1/10 to about 1/3. CsSnI3 was formed immediately as black grains suspending in the mixed solution. This phenomenon implied that the CsSnI3 was neither soluble in DI water nor in ethanol.
After five minutes sonication (using ultrasonic vibrator), homogeneous black CsSnI3solution with CsSnI3 black grains uniformly distributed in the solution, was formed. The homogeneous CsSnI3 solution contained CsSnI3 grains with a typical diameter of a few micrometers.
The homogeneous CsSnI3 solution was drop-coated on a substrate, such as a microscope glass slide or a piece of ceramics.
After drop-coating, the substrate was heat treated at 70° C. for 5 minutes to remove residual solvents. SnCl2 film with a thickness ˜40 μm was obtained by drop-coating the homogeneous CsSnI3 solution. The heating temperature ranged from about 50° C. to about 90° C.
The cross-sectional scanning electron micrographic (SEM) image taken from the film on a glass substrate was shown in
The chemical reaction for the mixture of the solutions could be described as the following:
3CsI+SnCl2→CsSnI3+2CsCl,
The reaction was verified by identifying the end products of CsSnI3 and CsCl using the X-ray diffraction (XRD) data to be discussed later.
Photoluminescence (PL) data and X-ray diffraction data (XRD) were used to identify CsSnI3 and to characterize the crystalline quality of each individual domain.
PL spectra were taken from a Nanolog system from Horiba Jobin Yvon. The Nanolog system had a 450 W Xe-lamp light source, a double-grating excitation spectrometer to select a central excitation wavelength and its bandwidth, a sample compartment, and an emission spectrometer to spectrally select desired emission to a photomultiplier tube (Hamamatsu P2658P) coupled with single photon-counting electronic circuits.
A relative low photoexcitation level of ˜20 mW cm−2 was used.
As shown in
The PL line shape was identical for the solution-based and vacuum-powder based deposition or synthesis methods as displayed in the inset of the
XRD data were used not only to further verify the crystal structure of CsSnI3 but importantly also to identify the side products when the CsI solution was formed as the end products and mixed with the SnCl2 solution (as shown in the reaction).
a) showed the XRD data measured from the same drop-coated CsSnI3film used for taking the SEM image in
b) showed theoretical calculated XRD profile by using a commercial software package CASTEP written by researchers at the Universities of York, Durham, St. Andrews, Cambridge and Rutherford Labs, using orthorhombic crystal structure of CsSnI3. CASTEP uses density functional theory with a plane wave basis set to calculate the electronic properties of crystalline solids and other materials from first principles.
All the measured peaks were accounted for and sorted into four groups.
The first group consisted of the peaks of 1 to 3 and all others not number-labeled. These peaks were originated from the orthorhombic structure of CsSnI3 and match the calculated XRD profile, as taught by CASTEP, as shown in
Peaks 1 and 2 reflected the expected XRD features of the Sn—I—Sn bond tilting) (163° in the a- and b-direction, respectively, in reference to the cubic-structure of CsSnI3.
Peak 3 represented the signature of the Sn—I—Sn bond tilting (170°) in the c-direction in reference to the tetragonal structure of CsSnI3.
The second group included the peaks of 4 and 5. Those peaks were originated from the residual material CsI.
The peaks of 6 and 7 made up the third group. The peaks of 6 and 7 were originated from CsCl, leading to the unambiguous determination of the chemical reaction as the CsI solution was transferred into the SnCl2 solution to form CsCl.
Finally, the presence of peaks 8 and 9 made up the fourth group. The peaks 8 and 9 matched Sn (IV) dioxide, SnO2. It should be mentioned here that the absence of XRD peaks associated with the residual SnCl2 strongly suggested that the chemical reaction under the ambient conditions resulting in favor of CsSnI3 formation.
In summary, CsSnI3 were synthesized using the CsI and SnCl2 solutions.
A solution-based method, capable of large-scale production, was employed to fabricate CsSnI3 films at a low cost, especially suitable for solar cell applications. The film polycrystalline quality was characterized by SEM, PL, and XRD data. Those data was verified to be comparable to that of similar thin-films synthesized by the vacuum-powder-based evaporation method.
While the invention has been described in detail and with reference to specific examples and the embodiments thereof, it will be apparent to one skilled in the art that various changes and modifications can be made therein without departing from the spirit and scope thereof.
This invention is a continuation-in-part of U.S. non-provisional application Ser. No. 13,151,243, filed Jun. 2, 2011, entitled: “PEROVSKITE SEMICONDUCTOR THIN FILM AND METHOD OF MAKING THEREOF”. The disclosure of this non-provisional application is hereby incorporated by reference.
Number | Date | Country | |
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Parent | 13151243 | Jun 2011 | US |
Child | 13491562 | US |