Photoluminescence characterization of vertically aligned ZnO microrods
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DUMCHENKO, Dumitru, HUANG, Ying-Sheng, KUO, Donghau, TIONG, Kwong-Kaw. Photoluminescence characterization of vertically aligned ZnO microrods. In: Journal of Luminescence, 2012, vol. 132, pp. 1890-1895. ISSN 0022-2313. DOI: https://doi.org/10.1016/j.jlumin.2012.02.037
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Journal of Luminescence
Volumul 132 / 2012 / ISSN 0022-2313

Photoluminescence characterization of vertically aligned ZnO microrods

DOI:https://doi.org/10.1016/j.jlumin.2012.02.037

Pag. 1890-1895

Dumchenko Dumitru12, Huang Ying-Sheng1, Kuo Donghau1, Tiong Kwong-Kaw3
 
1 National Taiwan University of Science and Technology, Taipei,
2 Institute of Applied Physics, Academy of Sciences of Moldova,
3 National Taiwan Ocean University, Keelung
 
 
Disponibil în IBN: 6 octombrie 2023


Rezumat

A detailed optical characterization of vertically aligned ZnO microrods (μRs) grown using a Ni-based catalyst was carried out by excitation-power- and temperature-dependent photoluminescence (PL) measurements. Low-temperature PL spectra of ZnO μRs are dominated by near-band-edge (NBE) emission consisted of a series of sharp lines typical for the bulk ZnO. Starting from the higher energy free exciton (FX) emission feature, the majority of them can be explained by radiative recombination of excitons bound to neutral donors (D 0X), defect bound exciton (DBX), two-electron satellites emission, free-to-bound, i.e. free electrons to the neutral acceptors (eA 0) transition, as well as their longitudinal-optical phonon replicas. An additional excitonic line located in between the FX and D 0X lines, denoted as the surface excitons (SX) for ZnO μRs is observed. The intensity of the SX line is found to be smaller than that of the nanosized counterpart and has been attributed to the surface-volume ratio effects. The excitation-power-dependent results of FX line at low and high power regimes show quite close values corresponding to, respectively, p=2 and p=1 limits of the theoretical power law expression I∼L p and larger deviations for the D 0X, SX and DBX lines. The temperature-dependent measurements confirmed the presence of eA 0 line showing kT/2 influence to the position of eA 0 emission line in comparison with FX. FX emissions persist up to 300 K and together with the dominant eA 0 emission govern the line shape of the NBE emission range, while D 0X and SX lines are quenched completely at 150 K. 

Cuvinte-cheie
Excitons, II-VI semiconductors, photoluminescence