Triet Ho Le Thanh, Mukherjee Atreyo, Vasileska Dragica, Akis John, Stavro Jann, Zhao Wei, Goldan Amir H
Department of Electrical Engineering, College of Engineering and Applied Sciences, Stony Brook University, Stony Brook, New York 11794, United States.
School of Electrical, Computer and Energy Engineering, Arizona State University, Tempe, Arizona 85287, United States.
ACS Appl Electron Mater. 2021 Aug 24;3(8):3538-3546. doi: 10.1021/acsaelm.1c00444. Epub 2021 Aug 2.
Amorphous selenium (-Se) with its single-carrier and non-Markovian, hole impact ionization process can revolutionize low-light detection and emerge to be a solid-state replacement to the vacuum photomultiplier tube (PMT). Although -Se-based solid-state avalanche detectors can ideally provide gains comparable to PMTs, their development has been severely limited by the irreversible breakdown of inefficient hole blocking layers (HBLs). Thus, understanding of the transport characteristics and ways to control electrical hot spots and, thereby, the breakdown voltage is key to improving the performance of avalanche -Se devices. Simulations using Atlas, SILVACO, were employed to identify relevant conduction mechanisms in -Se-based detectors: space-charge-limited current, bulk thermal generation, Schottky emission, Poole-Frenkel activated mobility, and hopping conduction. Simulation parameters were obtained from experimental data and first-principle calculations. The theoretical models were validated by comparing them with experimental steady-state dark current densities in avalanche and nonavalanche -Se detectors. To maintain bulk thermal generation-limited dark current levels in -Se detectors, a high-permittivity noninsulating material is required to substantially decrease the electric field at the electrode/hole blocking layer interface, thus preventing injection from the high-voltage electrode. This, in turn, prevents Joule heating from crystallizing the -Se layer, consequently avoiding early dielectric breakdown of the device.
非晶态硒(-Se)具有单载流子以及非马尔可夫空穴碰撞电离过程,可彻底改变微光探测,并有望成为真空光电倍增管(PMT)的固态替代品。尽管基于 -Se的固态雪崩探测器理论上可提供与PMT相当的增益,但其发展却因低效空穴阻挡层(HBL)的不可逆击穿而受到严重限制。因此,了解传输特性以及控制电热点的方法,进而掌握击穿电压,是提高雪崩 -Se器件性能的关键。利用SILVACO公司的Atlas软件进行模拟,以确定基于 -Se的探测器中的相关传导机制:空间电荷限制电流、体热产生、肖特基发射、普尔-弗伦克尔激活迁移率以及跳跃传导。模拟参数从实验数据和第一性原理计算中获取。通过将理论模型与雪崩和非雪崩 -Se探测器中的实验稳态暗电流密度进行比较,对理论模型进行了验证。为了在 -Se探测器中维持体热产生限制的暗电流水平,需要一种高介电常数的非绝缘材料,以大幅降低电极/空穴阻挡层界面处的电场,从而防止从高压电极注入。这反过来又可防止焦耳热使 -Se层结晶,进而避免器件过早发生介电击穿。