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. 2017 Oct 11;139(40):14173-14180.
doi: 10.1021/jacs.7b07223. Epub 2017 Sep 27.

Phase Segregation in Cs-, Rb- and K-Doped Mixed-Cation (MA)x(FA)1-xPbI3 Hybrid Perovskites from Solid-State NMR

Affiliations

Phase Segregation in Cs-, Rb- and K-Doped Mixed-Cation (MA)x(FA)1-xPbI3 Hybrid Perovskites from Solid-State NMR

Dominik J Kubicki et al. J Am Chem Soc. .

Abstract

Hybrid (organic-inorganic) multication lead halide perovskites hold promise for a new generation of easily processable solar cells. Best performing compositions to date are multiple-cation solid alloys of formamidinium (FA), methylammonium (MA), cesium, and rubidium lead halides which provide power conversion efficiencies up to around 22%. Here, we elucidate the atomic-level nature of Cs and Rb incorporation into the perovskite lattice of FA-based materials. We use 133Cs, 87Rb, 39K, 13C, and 14N solid-state MAS NMR to probe microscopic composition of Cs-, Rb-, K-, MA-, and FA-containing phases in double-, triple-, and quadruple-cation lead halides in bulk and in a thin film. Contrary to previous reports, we have found no proof of Rb or K incorporation into the 3D perovskite lattice in these systems. We also show that the structure of bulk mechanochemical perovskites bears close resemblance to that of thin films, making them a good benchmark for structural studies. These findings provide fundamental understanding of previously reported excellent photovoltaic parameters in these systems and their superior stability.

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Conflict of interest statement

The authors declare no competing financial interest.

Figures

Figure 1
Figure 1
Schematic representation of structural motifs investigated in this study: (a) black single-cation α-FAPbI3; (b) black double- (CsFA, RbFA), triple- (CsMAFA), or quadruple-cation (RbCsMAFA) compositions (X = I, Br); and (c) yellow nonperovskite δ-FAPbI3.
Figure 2
Figure 2
Quantitative 133Cs echo-detected MAS spectra of various (Cs/Rb/MA/FA)Pb(Br/I)3 systems at 298 K and (a) 10 kHz MAS and (b–j) 20 kHz MAS acquired within 1 h after annealing. Asterisks (*) indicate spinning sidebands, and † is a transmitter artifact.
Figure 3
Figure 3
(a) Variable-temperature solid-state 133Cs MAS NMR spectra of Cs0.20FA0.80. (b) Temperature dependence of the 133Cs shift (measured at the maximum of the most intense peak). Spinning sidebands are marked with asterisks (*).
Figure 4
Figure 4
A 1H–133Cs HETCOR of Cs0.20FA0.80 at 100 K and 12 kHz MAS.
Figure 5
Figure 5
11.7 T Solid-state 87Rb echo-detected MAS (20 kHz, 298 K) spectra of various (Cs/Rb/MA/FA)Pb(Br/I)3 systems. The corresponding 100 K 13C CP MAS spectra of a–c, e, f, and j show only one FA signal corresponding to it being in a 3D perovskite environment (Figure S11).
Figure 6
Figure 6
(a) Low-temperature (100 K) 13C CP MAS spectra, (b) echo-detected 14N MAS spectra at 300 K and 5 kHz MAS of MAPbI3 (top) and K0.10MA0.90PbI3 (bottom), and (c) echo-detected 39K spectrum of K0.10MA0.90PbI3 at 300 K and 20 kHz MAS (20 s recycle delay, 12 h total acquisition time).
Figure 7
Figure 7
Solid-state MAS NMR spectra of CsMAFA(Br,I) in bulk (blue) and prepared as thin film on glass (red). (a) Echo-detected 133Cs spectra at 100 K and 12 kHz MAS (Figure 2f is the corresponding 298 K spectrum of the bulk material), (b) 13C CP at 100 K and 12 kHz MAS, and (c) 14N echo-detected spectra at 298 K and 20 kHz MAS (acquisition times: bulk 20 h, thin film 60 h). The isotropic signal marked “†” most likely comes from traces of DMF used during spin-coating.

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