论文标题

1550nm雪崩光电二极管检测到暗电流和单个光子检测:净时间校正的概率分布和熵率

Dark Current and Single Photon Detection by 1550nm Avalanche Photodiodes: Dead Time Corrected Probability Distributions and Entropy Rates

论文作者

Menkart, Nicole, Hart, Joseph D., Murphy, Thomas E., Roy, Rajarshi

论文摘要

单光子检测器的深度计数速率很大程度上取决于检测器操作的偏置水平。在弱光源(例如新型激光器或单光子发射器)的情况下,由于光源引起的计数速率可以与检测器黑暗计数相媲美。在这种情况下,必须表征黑暗计数的统计特性。通常认为黑暗计数遵循统计学上独立于入射光子计数的泊松过程。必须针对特定类型的光电遗传学验证此假设。在这项工作中,我们专注于1550nm制造的单光雪崩光电二极管(Spads)。对于使用的INGAA探测器,我们发现所测量的分布通常与泊松的分布差异很大,因为存在死亡时间和随着偏差水平的差异的增加而产生差异。当增加死亡时间以消除后螺栓的效果时,有必要纠正死亡时间影响的测量分布。为此,我们应用了一种迭代算法来从黑暗计数的概率分布以及从外部弱激光源(已知是泊松)和黑暗计数一起检测到的光线的概率分布以及情况。我们认为,这是该算法在实际数据中综合应用的第一个实例,并发现在两种情况下,校正后的概率分布都是泊松分布。我们还使用Grassberger-Procaccia算法来估计深度计数过程的熵产生速率,该过程提供了一个表征黑暗计数与分布形状之间时间相关性的单个度量。因此,我们已经开发了一种系统的程序,用于使用1550nm Spads的数据并获得准确的光电统计量来检查新的光源。

Single photon detectors have dark count rates that depend strongly on the bias level for detector operation. In the case of weak light sources such as novel lasers or single-photon emitters, the rate of counts due to the light source can be comparable to that of the detector dark counts. In such cases, a characterization of the statistical properties of the dark counts is necessary. The dark counts are often assumed to follow a Poisson process that is statistically independent of the incident photon counts. This assumption must be validated for specific types of photodetectors. In this work, we focus on single-photon avalanche photodiodes (SPADs) made for 1550nm. For the InGaAs detectors used, we find the measured distributions often differ significantly from Poisson due to the presence of dead time and afterpulsing with the difference increasing with the bias level. When the dead time is increased to remove the effects of afterpulsing, it is necessary to correct the measured distributions for the effects of the dead time. To this end, we apply an iterative algorithm to remove dead time effects from the probability distribution for dark counts as well as for the case where light from an external weak laser source (known to be Poisson) is detected together with the dark counts. We believe this to be the first instance of the comprehensive application of this algorithm to real data and find that the corrected probability distributions are Poisson distributions in both cases. We additionally use the Grassberger-Procaccia algorithm to estimate the entropy production rates of the dark count processes, which provides a single metric that characterizes the temporal correlations between dark counts as well as the shape of the distribution. We have thus developed a systematic procedure for taking data with 1550nm SPADs and obtaining accurate photocount statistics to examine novel light sources.

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