2016
DOI: 10.1088/0022-3727/49/27/275107
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Electron transition pathways of photoluminescence from 3C-SiC nanocrystals unraveled by steady-state, blinking and time-resolved photoluminescence measurements

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Cited by 11 publications
(14 citation statements)
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“…The FWHM of the 1/β distribution peak is about 140 meV, which is very close to the FWHM of the steady-state PL spectrum (~144 meV). On the contrary, as reported previously, for PL of SiC NCs caused by size effect, both τ and β are hardly dependent on the detection wavelength [33]. In that case, the ultra-broad PL widths with FWHM>600 meV are originated from the size distribution of the NCs.…”
Section: Resultscontrasting
confidence: 44%
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“…The FWHM of the 1/β distribution peak is about 140 meV, which is very close to the FWHM of the steady-state PL spectrum (~144 meV). On the contrary, as reported previously, for PL of SiC NCs caused by size effect, both τ and β are hardly dependent on the detection wavelength [33]. In that case, the ultra-broad PL widths with FWHM>600 meV are originated from the size distribution of the NCs.…”
Section: Resultscontrasting
confidence: 44%
“…When excitation wavelength increases, more NCs with big sizes and narrow bandgaps are selectively excited, resulting in PL spectral redshift, which has been extensively observed in Si quantum dots, SiC NCs, carbon nanoparticles, graphene quantum dots, and MoS2 quantum dots. [31][32][33] Here, the PL peaks of perovskite NCs that hardly shift tend to imply minor contribution from size effect. PL excitation (PLE) spectra monitored at emission wavelengths of 455, 465, and 475 nm are also acquired.…”
Section: Resultsmentioning
confidence: 94%
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“…A numerical analysis is performed based on a reported model. 28,29 Specically, uorescence process could be described by relaxation time s and recombination time b. And these two values could be extracted by tting the time-resolved uorescence curves.…”
Section: Resultsmentioning
confidence: 99%
“…ffiffiffiffiffiffiffiffi ffi FðtÞ p is linearly related with t. During this time interval ħu n is almost unoccupied, while the variations of ħu 1 and ħu 0 occupations are similar. 28,29 Thence in this time window, radiative recombination time b (relax from ħu 1 to ħu 0 ) can be acquired.…”
Section: Resultsmentioning
confidence: 99%