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具有不同平均尺寸的非晶硅纳米颗粒集合体的光致发光的温度依赖性。

Temperature dependence of the photoluminescence from ensembles of amorphous silicon nanoparticles with various average sizes.

作者信息

Brüggemann R, Nesheva D, Meier S, Bineva I

机构信息

Institute of Physics, Carl von Ossietzky University Oldenburg, D-26111 Oldenburg, Germany.

出版信息

J Nanosci Nanotechnol. 2011 Feb;11(2):959-65. doi: 10.1166/jnn.2011.3103.

Abstract

Amorphous SiO(x) thin films with three different oxygen contents (x = 1.3, 1.5, and 1.7) have been deposited by thermal evaporation of SiO in vacuum. Partial phase separation in the films has been induced by annealing at 773 or 973 K in argon for 60 and 120 min and thus Si-SiO(x) composite films have been prepared containing amorphous Si nanoparticles of various sizes (< 3 nm). Photoluminescence from the films has been measured in the temperature range 20-296 K. The single Gauss band observed in the photoluminescence spectra of the samples with x = 1.3 and centered in the range 1.55-1.75 eV has been related to radiative recombination in Si nanoparticles. Two bands, a red-orange one (related to radiative recombination in Si nanoparticles) and a green band peaked at approximately 2.3 eV (related to radiative recombination via defects) have been resolved in the photoluminescence spectra of the films with x = 1.5 and 1.7. The band in the spectra of the x = 1.3 samples has shown a relative strong thermal quenching but it is significantly weaker than the photoluminescence quenching in bulk a-Si. Besides, the higher the initial oxygen content, the weaker is the photoluminescence thermal quenching. These observations have been related to carrier confinement which is stronger in smaller nanoparticles. The thermally induced photoluminescence decrease with increasing temperature in the samples with x = 1.3 obeys the relation that is characteristic for bulk a-Si:H while the photoluminescence decrease in x = 1.5 and 1.7 samples is of Arrhenius type. We suggest that in nanoparticles larger than 2 nm recombination via band tail states is the dominating photoluminescence mechanism while in smaller nanoparticles exciton-like recombination dominates.

摘要

通过在真空中热蒸发SiO制备了具有三种不同氧含量(x = 1.3、1.5和1.7)的非晶SiO(x)薄膜。通过在氩气中于773或973 K退火60和120分钟,诱导薄膜中发生部分相分离,从而制备了包含各种尺寸(< 3 nm)非晶硅纳米颗粒的Si-SiO(x)复合薄膜。在20 - 296 K的温度范围内测量了薄膜的光致发光。在x = 1.3的样品的光致发光光谱中观察到的单个高斯带,其中心位于1.55 - 1.75 eV范围内,与硅纳米颗粒中的辐射复合有关。在x = 1.5和1.7的薄膜的光致发光光谱中分辨出两个带,一个红橙色带(与硅纳米颗粒中的辐射复合有关)和一个在约2.3 eV处达到峰值的绿色带(与通过缺陷的辐射复合有关)。x = 1.3样品光谱中的带显示出相对较强的热猝灭,但比块状非晶硅中的光致发光猝灭明显较弱。此外,初始氧含量越高,光致发光热猝灭越弱。这些观察结果与载流子限制有关,在较小的纳米颗粒中载流子限制更强。在x = 1.3的样品中,随着温度升高,热诱导的光致发光下降遵循块状非晶硅氢的特征关系,而在x = 1.5和1.7的样品中,光致发光下降是阿仑尼乌斯类型的。我们认为,在大于2 nm的纳米颗粒中,通过带尾态的复合是主要的光致发光机制,而在较小的纳米颗粒中,类激子复合占主导。

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