| Literature DB >> 31412580 |
Weijie Guo1, Nan Chen1, Binbin Xu2, Yijun Lu1, Bin Li3, Tingzhu Wu1, Qijin Cheng1, Yang Li4, Jin Chen4, Yue Lin5, Zhong Chen6,7.
Abstract
HybridEntities:
Keywords: combined stresses; electronic structure; perovskite nanocrystals; photophysical properties; stability
Year: 2019 PMID: 31412580 PMCID: PMC6724138 DOI: 10.3390/nano9081158
Source DB: PubMed Journal: Nanomaterials (Basel) ISSN: 2079-4991 Impact factor: 5.076
Figure 1The scheme of the experiments.
Figure 2(a) A typical TEM image MAPbBr3 NC in PVDF matrix; (b) TEM image of a typical MAPbBr3 NC; (c) normalized absorption and PL spectrum of the fabricated MBNCs-PVDF; and (d) PL intensities recorded during aging, normalized to the initial intensity, and presented in logarithmic ordinate. Hollow circles correspond to aging in N2, hollow squares to aging in vacuum, and hollow triangles to aging in air, while dashed lines are obtained by linear fitting for aging in vacuum and air and by reciprocal fitting for aging in N2. The temperature and 368-nm UV light illumination density during aging are 323 K and 5.6 mW/cm2, respectively.
Figure 3XRD patterns of MBNCs-PVDF: (a) After aging in N2; (b) after aging in vacuum; (c) after aging in an air atmosphere; and (d) pristine sample. For reference, (e) and (f) provide XRD patterns of PbBr2 and CH3NH3Br (MABr); and (g) provides a standard XRD pattern of NH4Pb2Br5 (PDF#74-0969). The standard patterns of MAPbBr3 (PDF#54-0752) are provided at the bottom of (d). Diamonds and stars indicate diffraction peaks of NH4Pb2Br5 and PbBr2, respectively. The temperature and 368-nm UV light irradiation density during aging are 323 K and 5.6 mW/cm2.
Figure 4(a) Electronic band structure and (b) the density of states (DOS) of NH4Pb2Br5 calculated using the full-potential linearized augmented plane wave (FP-LAPW) method implemented in the WIEN2K code. (c) Crystal structure of tetragonal NH4Pb2Br5. (d) Normalized absorption spectra and (e) normalized PL spectra of the pristine MBNCs-PVDF and the samples after aging in three different atmospheres. The temperature and 368 nm UV light irradiation density during aging are 323 K and 5.6 mW/cm2.
Figure 5Pseudo-color maps of temperature-dependent PL spectra of MBNCs-PVDF: (a) Pristine; (b) after aging in N2; (c) after aging in vacuum; and (d) after aging in an air atmosphere. The aging temperature and 368 nm UV light illumination density of (b)–(d) are 323 K and 5.6 mW/cm2.
Figure 6The comparison of two Gaussian fitted peaks from PL spectra of pristine MBNCs-PVDF: (a) Integrated PL intensity; (b) PL emission peak energy; and (d) FWHM of the fitted peaks obtained by two-peak Gaussian fitting. (c) PL spectra at 15 K, 70 K, and 90 K of pristine MBNCs-PVDF, illustrating the evolution of multipeak PL emission at low temperature, with the inset showing the two-peak Gaussian fitting result for the PL spectrum at 15 K.