Photonics Research, 2018, 6 (6): 06000554, Published Online: Jul. 2, 2018  

Ultrafast optical nonlinearity of blue-emitting perovskite nanocrystals Download: 570次

Author Affiliations
1 College of Physics and Energy, Shenzhen University, Shenzhen 518060, China
2 Department of Electrical and Electronic Engineering, South University of Science and Technology of China, Shenzhen 518055, China
3 Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
Figures & Tables

Fig. 1. (a) Normalized linear absorption and fluorescence spectra for the perovskite NCs. The insets are the emission images of the NCs in solution: 1 for CsPbCl3 NCs and 2 for CsPb(Cl0.53Br0.47)3 NCs. TEM images of (b) CsPbCl3 NCs and (c) CsPb(Cl0.53Br0.47)3 NCs. The insets are high-resolution TEM images of the NCs. (d) Fluorescence decay kinetics of the perovskite NCs under excitation at 365 nm.

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Fig. 2. TA kinetics (a) for CsPbCl3 NCs probed at 398 nm and (c) for CsPb(Cl0.53Br0.47)3 NCs probed at 432 nm. Initially, the presence of biexcitons and even higher order multi-excitons causes a fast decay (Auger process). At time 1  ns, the signals decay exponentially, which corresponds to a single-exciton signal. GSB signal amplitude at a time delay of 1 ns as a function of excitation intensity for (b) CsPbCl3 NCs and (d) CsPb(Cl0.53Br0.47)3 NCs.

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Fig. 3. Measured fluorescence intensity as a function of the input laser intensity at 650 nm. The insets are the two-photon excited emission imaging of the NC solution and the best-fitting straight lines on logarithmic scales: 1 for CsPbCl3 NCs and 2 for CsPb(Cl0.53Br0.47)3 NCs. The concentration of CsPb(Cl0.53Br0.47)3 NCs solution is 1×106  M, while the concentration of CsPbCl3 NCs solution is 2.57×106  M.

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Fig. 4. (a) Divided Z-scan results of the OA signal for NCs at a wavelength of 650 nm. The solid lines are the fittings to the data using the Z-scan theory. (b) TPA spectra of NCs between 620 and 720 nm. The concentration of both CsPbCl3 and CsPb(Cl0.53Br0.47)3 NCs was 5.95×106  M.

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Fig. 5. (a) Divided Z-scan results of the CA signal by the OA signal at a wavelength of 650 nm. The solid lines are the fittings to the data using the Z-scan theory. (b) Wavelength-dependent intrinsic nonlinear refractive index of CsPb(Cl0.53Br0.47)3 NCs. The concentration of both CsPbCl3 and CsPb(Cl0.53Br0.47)3 NCs was 5.95×106  M.

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Fig. 6. Wavelength-dependent figure of merit (T) of CsPb(Cl0.53Br0.47)3 NCs.

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Table1. Calculated NLO Parameters of the CsPbCl3 and CsPb(Cl0.53Br0.47)3 NCs and Other Materials Reported Elsewhere

Samplesλem (nm)σ2 (GM) or β (cm/W)n2 (intrinsic) (cm2/W)References
p-SeptiphenylViolet-blue880 GM (0.5 ps, 660 nm)[27]
Ladder-type oligo(p-phenylene)s449 nm1046 GM (120 fs, 880 nm)[28]
Diphenylamino and 1,2,4-triazole endcapped oligofluorenes422 nm57 GM (100 fs, 800 nm)[29]
Bis(styryl)benzene derivatives455 nm995 GM (725 nm)[30]
ZnSViolet-blue21100 GM (28 ps, 532 nm) or 17200 GM (28 ps, 520 nm)[31]
ZnSe/ZnS420 nm or 408 nm5100 GM or 13900 GM (100 fs, 806 nm)[32]
ZnSe420 nm or 408 nm4900 GM or 12200 GM (100 fs, 806 nm)[32]
Truxene-based star-shaped oligofluorenes441 nm2200 GM (120 fs, 800 nm)[33]
1,4-Bis(carbazolyl)benzene derivatives395 nm448 GM (100 fs, 720 nm)[34]
CsPbCl3456 nm1.36×1013  cm/W (396 fs, 787 nm)5.30×1015 (396 fs, 787 nm)[35]
CsPbBr3460 nm1.71×1013  cm/W (130 fs, 800 nm)5.18×1013 (130 fs, 800 nm)[36]
CsPb(Cl0.53Br0.47)3447 nm28347 GM or 3.22×1012  cm/W (100 fs, 630 nm)1.4×1013 (100 fs, 620 nm)This work
CsPbCl3409 nm6963 GM or 7.91×1013  cm/W (100 fs, 630 nm)<0.46×1013 (100 fs, 620 nm)This work

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Junzi Li, Can Ren, Xin Qiu, Xiaodong Lin, Rui Chen, Cheng Yin, Tingchao He. Ultrafast optical nonlinearity of blue-emitting perovskite nanocrystals[J]. Photonics Research, 2018, 6(6): 06000554.

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