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CdWO4 中 100fs 激光脉冲的带尾吸收饱和。

Band tail absorption saturation in CdWO4 with 100 fs laser pulses.

机构信息

Institute of Physics, University of Tartu, Tartu, Estonia.

出版信息

J Phys Condens Matter. 2013 Jun 19;25(24):245901. doi: 10.1088/0953-8984/25/24/245901. Epub 2013 May 24.

Abstract

The decay kinetics of the excitonic emission of CdWO4 scintillators was studied under excitation by powerful 100 fs laser pulses in the band tail (Urbach) absorption region. A special imaging technique possessing both spatial and temporal resolution provided a unique insight into the Förster dipole-dipole interaction of self-trapped excitons, which is the main cause of the nonlinear quenching of luminescence in this material. In addition, the saturation of phonon-assisted excitonic absorption due to extremely short excitation pulses was discovered. A model describing the evolution of electronic excitations in the conditions of absorption saturation was developed and an earlier model of decay kinetics based on the Förster interaction was extended to include the saturation effect. Compared to the previous studies, a more accurate calculation yields 3.7 nm as the Förster interaction radius. It was shown that exciton-exciton interaction is the main source of scintillation nonproportionality in CdWO4. A quantitative description using a new model of nonproportionality was presented, making use of the corrected value of the Förster radius.

摘要

研究了在强 100fs 激光脉冲激发下,CdWO4 闪烁体在带尾(Urbach)吸收区域中激子辐射衰减的动力学。一种具有空间和时间分辨率的特殊成像技术,为自陷激子的福斯特偶极-偶极相互作用提供了独特的见解,这是导致该材料中荧光非线性猝灭的主要原因。此外,还发现了由于极短的激发脉冲导致声子辅助激子吸收的饱和。提出了一个描述在吸收饱和条件下电子激发演化的模型,并将基于福斯特相互作用的早期衰减动力学模型扩展到包括饱和效应。与之前的研究相比,更精确的计算得出福斯特相互作用半径为 3.7nm。结果表明,激子-激子相互作用是 CdWO4 闪烁体非比例性的主要来源。利用修正后的福斯特半径值,提出了一个新的非比例性定量描述模型。

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