Tsallis distribution and luminescence decays
classification
❄️ cond-mat.other
cond-mat.dis-nn
keywords
luminescencedistributiontsallisdecaysexponentialobtainedresultstretched
read the original abstract
Usually, the Kohlrausch (stretched exponential) function is employed to fit the luminescence decays. In this work we propose to use the Tsallis distribution as an alternative to describe them. We show that the curves of the luminescence decay obtained from the Tsallis distribution are close to those ones obtained from the stretched exponential. Further, we show that our result can fit well the data of porous silicon at low temperature and simulation result of the trapping controlled luminescence model.
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