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Electron transport and charge induction in cadmium zinc telluride detectors with space charge build up under intense x-ray irradiation

机译:在强X射线辐射下会形成具有空间电荷的碲化镉锌探测器中的电子传输和电荷感应

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摘要

Under intense x-ray irradiation, wide band gap semiconductor radiation detectors fabricated from crystals with low hole transport properties develop a steady-state space charge distribution that results from a dynamic equilibrium between charge carrier dynamics and the incident photon field. At a high enough x-ray flux, this space charge can collapse the electric field within the detector, resulting in the paralyzation of photon counting (i.e., high-flux polarization). However, well before polarization causes a catastrophic device failure, there can be enough space charge present to significantly modify the electric field. A modified field affects the electron transport and, therefore, signal generation within the sensor, which can ultimately degrade the performance of high-rate photon counting electronics. In this study, we analytically solve the fundamental equation of charge conservation to derive the modified electron transport in the presence of an exponential space charge distribution that results from the incident x-rays. We use these space-time solutions to calculate and study the time dependence of the resulting charge-induced signals. The predicted induced signals are compared throughout with numerical solutions of the full charge transport equation. In addition, we present analogous closed-form signals for a uniform distribution relevant to a broader class of γ-ray applications. Finally, we use these solutions to derive a two-parameter family of modified Hecht curves that naturally predict a voltage offset that appears due to the space charge.
机译:在强X射线辐射下,由具有低空穴传输特性的晶体制成的宽带隙半导体辐射探测器会形成稳态空间电荷分布,该空间电荷分布是由电荷载流子动力学和入射光子场之间的动态平衡引起的。在足够高的X射线通量下,这种空间电荷会使检测器内的电场崩溃,从而导致光子计数麻痹(即高通量偏振)。但是,在极化导致灾难性设备故障之前,可能存在足够的空间电荷来显着改变电场。修改后的场会影响电子传输,从而影响传感器内的信号生成,最终会降低高速率光子计数电子器件的性能。在这项研究中,我们分析性地解决了电荷守恒的基本方程,以在存在入射x射线的指数空间电荷分布的情况下,得出修正的电子传输。我们使用这些时空解决方案来计算和研究所产生的电荷感应信号的时间依赖性。将预测的感应信号与整个电荷传输方程的数值解进行比较。此外,我们提出了与更广泛的γ射线应用相关的均匀分布的类似闭式信号。最后,我们使用这些解决方案来推导两参数族的修改后的赫克特曲线,这些曲线自然地预测了由于空间电荷而出现的电压偏移。

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  • 来源
    《Journal of Applied Physics》 |2010年第11期|P.114512.1-114512.10|共10页
  • 作者

    Derek S. Bale; Csaba Szeles;

  • 作者单位

    eV Microelectronics, a division of Endicott Interconnect Technologies Inc., Saxonburg, Pennsylvania 16056, USA;

    rneV Microelectronics, a division of Endicott Interconnect Technologies Inc., Saxonburg, Pennsylvania 16056, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
  • 原文格式 PDF
  • 正文语种 eng
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