| Literature DB >> 29116121 |
Wei Wang1, Yu Li1,2, Xiangyuan Wang3, Yang Liu1, Yanping Lv3, Shufeng Wang4,5, Kai Wang3, Yantao Shi6, Lixin Xiao1, Zhijian Chen1, Qihuang Gong7.
Abstract
For highly interested organolead perovskite based solar cells, the exciton and free carriers are the photoproducts in the working layers. In this study, we revealed their two forms of relations depending on heat-annealing condition. In non-annealed films and single crystal, they are in density-dependent dynamical balance (co-existing). For the sufficiently heat-annealed films, they present a significant emissive exciton-carrier collision (ECC). The two relations indicate the emergence of a subgrain morphology within the tetragonal phase of crystal grain, induced by heat annealing process. Such subgrain structure could be assigned to a ferroelastic twinning structure recently found inside the crystal grain of the films. Since the heat annealing is a general procedure in preparing perovskite working layers, we propose that the ECC and subgrain morphology widely exist in real devices. We suggest that the subgrain structure provides another level of morphological basis for in depth understanding high performance of organolead perovskite working layers.Entities:
Year: 2017 PMID: 29116121 PMCID: PMC5677142 DOI: 10.1038/s41598-017-15097-y
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1The typical fluorescent decay of CH3NH3PbI3 films after excitation. The films were pumped by a femtosecond laser at 517 nm with various pulse energy, while the peaks of fluorescence are ~772 nm. The PL 0 is taken at the maxima for each fluorescent decay (circled). The corresponding excitation densities are labelled for each decay.
Figure 2PL 0 versus excitation density n. (a) and (b) are the I3 films without/with annealing, respectively. The film thickness is ~250 nm. The straight red lines are drawn with strict slop of 2, 3/2, and 1, for visualization. Corresponding SEM images are of 1×1 μm2. The PL 0-n curve for single crystal are also drawn, with density estimated according to a film of ~250 nm thickness. (This estimation will not affect the power dependencies) The scale bar is 0.4 mm (c). The PL 0 of I3-sa film at 340 K is recorded (d).
Figure 3The simulation of density-dependent photoproducts inside perovskite films. (a) The relative ratio, x, of free carriers in total excitation density, according to Saha-Langmuir equation. (b) The simulated density of free carriers and excitons. (c) The simulated density-resolved PL 0 when the free carriers and exciton dynamically co-exist inside perovskite, and (d) when ECC become dominant in the system.
Figure 4The photoproduct systems and their conversion for organolead perovskite films.