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. 2018 Jun 26;12(6):5504-5517.
doi: 10.1021/acsnano.8b01122. Epub 2018 May 22.

Exploration of Near-Infrared-Emissive Colloidal Multinary Lead Halide Perovskite Nanocrystals Using an Automated Microfluidic Platform

Affiliations

Exploration of Near-Infrared-Emissive Colloidal Multinary Lead Halide Perovskite Nanocrystals Using an Automated Microfluidic Platform

Ioannis Lignos et al. ACS Nano. .

Abstract

Hybrid organic-inorganic and fully inorganic lead halide perovskite nanocrystals (NCs) have recently emerged as versatile solution-processable light-emitting and light-harvesting optoelectronic materials. A particularly difficult challenge lies in warranting the practical utility of such semiconductor NCs in the red and infrared spectral regions. In this context, all three archetypal A-site monocationic perovskites-CH3NH3PbI3, CH(NH2)2PbI3, and CsPbI3-suffer from either chemical or thermodynamic instabilities in their bulk form. A promising approach toward the mitigation of these challenges lies in the formation of multinary compositions (mixed cation and mixed anion). In the case of multinary colloidal NCs, such as quinary Cs xFA1- xPb(Br1- yI y)3 NCs, the outcome of the synthesis is defined by a complex interplay between the bulk thermodynamics of the solid solutions, crystal surface energies, energetics, dynamics of capping ligands, and the multiple effects of the reagents in solution. Accordingly, the rational synthesis of such NCs is a formidable challenge. Herein, we show that droplet-based microfluidics can successfully tackle this problem and synthesize Cs xFA1- xPbI3 and Cs xFA1- xPb(Br1- yI y)3 NCs in both a time- and cost-efficient manner. Rapid in situ photoluminescence and absorption measurements allow for thorough parametric screening, thereby permitting precise optical engineering of these NCs. In this showcase study, we fine-tune the photoluminescence maxima of such multinary NCs between 700 and 800 nm, minimize their emission line widths (to below 40 nm), and maximize their photoluminescence quantum efficiencies (up to 89%) and phase/chemical stabilities. Detailed structural analysis revealed that the Cs xFA1- xPb(Br1- yI y)3 NCs adopt a cubic perovskite structure of FAPbI3, with iodide anions partially substituted by bromide ions. Most importantly, we demonstrate the excellent transference of reaction parameters from microfluidics to a conventional flask-based environment, thereby enabling up-scaling and further implementation in optoelectronic devices. As an example, Cs xFA1- xPb(Br1- yI y)3 NCs with an emission maximum at 735 nm were integrated into light-emitting diodes, exhibiting a high external quantum efficiency of 5.9% and a very narrow electroluminescence spectral bandwidth of 27 nm.

Keywords: formamidinium; halides; microfluidics; nanocrystals; perovskites; quantum dots.

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Conflict of interest statement

The authors declare no competing financial interest.

Figures

Figure 1
Figure 1
Formabilities of the 3D and 1D polymorphs of CsPbI3 and FAPbI3 compounds and the goal of this study: near-infrared emissive LHP NCs. The PbI6 octahedra of α-FAPbI3 NCs are assembled in a 3D cubic metastable lattice, which spontaneously converts into a 1D hexagonal version (nonluminescent) at room temperature. In the case of CsPbI3, the PbI6 octahedra of FAPbX3 NCs are assembled in a 3D orthorhombic metastable lattice (γ-phase), which eventually converts at room temperature into a 1D orthorhombic δ-phase (nonluminescent). The goal of this study is highlighted with a question: can high-throughput microfluidic screening identify the existence of stable multinary CsxFA1–xPb(Br1–yIy)3 phases in the form of colloidal NCs, which cover the PL region of 700–800 nm, i.e., in-between ternary 3D phases (CsPbI3 and FAPbI3)? We note that bulk α-FAPbI3 emits at 840 nm and γ-CsPbI3 emits at 710 nm, whereas their NC counterparts are commonly reported to emit at ≤700 and ≤780 nm, respectively.,−, It is also noted that the space groups reported for the γ- and δ-phases of CsPbI3 do not differ (while their structures manifestly do), as they can easily be interconverted by simple axis permutations. We used the original Pbnm and Pnma for the γ- and δ-forms, respectively, to maintain consistency with past literature.
Figure 2
Figure 2
(Left) Illustration of the segmented-flow reaction platform equipped with online PL and absorbance modules for the synthesis and real-time monitoring of CsxFA1–xPbX3 perovskite NCs. The microfluidic platform allows for a systematic and independent variation of precursor molar ratios, such as Cs/Pb, FA/Pb, Cs/FA, and Br/I, growth times (determined by the flow rate and tube lengths), and temperature. Droplets are generated by adjusting the flow rates of the carrier phase (50–200 μL/min) and that of the dispersed phase (1.2–50 μL/min). (Right) Illustration of a typical flask-based hot-injection synthesis of CsxFA1–xPbX3 NCs. Overall, synthesis optimization was performed by mutual information exchange between flask-based experimentation (identification of suitable precursors, solvents, and capping ligands) and microfluidics (optimization of the reaction parameters). The optimized reaction parameters were successfully transferred from microfluidics back into flask reactors, followed by up-scaling and additional postsynthetic characterization (XRD, electron microscopy, and stability tests).
Figure 3
Figure 3
Microfluidic synthesis of CsxFA1–xPbI3 NCs. Variation in the (a) PL spectra, (b) fwhm, and (c) PL maximum as a function of temperature for Cs0.03FA0.97PbI3 NCs (with the variation in the Cs/FA molar ratio indicated). Other parameters were as follows: FA/Pb = 9.3, Cs/Pb = 0.3, and reaction time = 10 s. (d–f) Temporal evolution of the normalized online PL spectra, PL maxima, and fwhm of Cs0.02FA0.98PbI3 NCs at 80 °C.
Figure 4
Figure 4
(a) PL spectra of colloidal CsxFA1–xPb(Br1–yIy)3 NCs synthesized using the microfluidic platform and exhibiting composition-tunable band-gap energies between 690 and 780 nm with fwhm values of 40–65 nm and (b) representative online PL and in online absorption spectra at different quantities of Cs+ and Br in the reaction mixture.
Figure 5
Figure 5
Optical absorption and PL spectra of CsxFA1–xPb(Br1–yIy)3 NCs synthesized in conventional flask reactors, exhibiting a fwhm of 40 nm. (b) Bright-field scanning TEM (STEM) image of CsxFA1–xPb(Br1–yIy)3 NCs. (c) Synchrotron XRD pattern (black) and best fit (red, 2θ range of 0.5–130°; λ = 0.563 729 Å) for CsxFA1–xPb(Br1–yIy)3 NCs, yielding a refined lattice parameter (a = 6.3296 Å) and the anionic composition. The inset illustrates the cubic perovskite structure of CsxFA1–xPb(Br1–yIy)3 NCs (space group Pmm, with y = 0.87 and x = 0), in which the perovskite framework consists of PbX6 units sharing the octahedral corners; the X anions are disordered in four equivalent positions.
Figure 6
Figure 6
(a) Energy diagram of LED devices with CsxFA1–xPb(Br1–yIy)3 NCs as emissive layers. (b) Current density and radiance versus voltage characteristics of device 1. (c) External quantum efficiency versus current density characteristics shown for devices 1 and 2. (d) Narrowest EL spectra of device 1 and device 2.

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