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对InGaAs/InP单光子雪崩光电二极管进行结构设计与数值仿真,得到相应的电学与光学参数。针对雪崩击穿概率对器件光子探测效率的影响,研究了两次Zn扩散深度差、Zn扩散横向扩散因子、Zn掺杂浓度以及温度参数与器件雪崩击穿概率的关系。研究发现,当深扩散深度为2.3μm固定值时,浅扩散深度存在对应最佳目标值。浅扩散深度越深,相同过偏压条件下倍增区中心雪崩击穿概率越大,电场强度也会随之增加。当两次Zn扩散深度差小于0.6μm时,会发生倍增区外的非理想击穿,导致器件的暗计数增大。Zn扩散横向扩散因子越大,倍增区中心部分雪崩击穿概率越大,而倍增区边缘雪崩击穿概率会越小。在扩散深度不变的情况下,浅扩散Zn掺杂浓度对雪崩击穿概率无明显影响,但深扩散Zn掺杂浓度越高,相同过偏压条件下雪崩击穿概率越小。本文研究可为设计和研制高探测效率、低暗计数InGaAs/InP单光子雪崩光电二极管提供参考。 相似文献
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雪崩光电二极管单光子探测器是一种具有超高灵敏度的光电探测器件,在远距离激光测距、激光成像和量子通信等领域有非常重要的应用.然而,由于雪崩光电二极管单光子探测器的雪崩点对工作温度高度敏感,因此在外场环境下工作时容易出现增益波动,继而导致单光子探测器输出信号的延时发生漂移,严重降低了探测器的时间稳定性.本文发展了一种稳定输出延时的方法,采用嵌入式系统控制雪崩光电二极管,使其处于恒定温度,并实时补偿由环境温度引起的延时漂移,实现了雪崩光电二极管单光子探测器的高时间稳定性探测.实验中,环境温度从16 ℃变化到36 ℃,雪崩光电二极管的工作温度稳定在15 ℃,经过延时补偿,雪崩光电二极管单光子探测器输出延时漂移小于±1 ps,时间稳定度达到0.15 ps@100 s.这项工作有望为全天候野外条件和空间极端条件下的高精度单光子探测应用提供有效的解决方法. 相似文献
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针对雪崩光电二极管(Si-APD)所加偏压需要随环境温度作调整,且偏压电路所需的低纹波低噪声等因素,构建了以Royer振荡器和微控制器为核心的偏压电路。该Si-APD偏压电路以BL8032型同步降压控制器作为Royer振荡器的输入电源,以MS5221M型DAC作为该输入电源的调整单元,以AD8606型集成运放和AD7980型ADC作为Royer振荡器输出电压采样单元,以STM32F103TBU6型微控制器作为计算与时序控制单元。本偏压电路不仅具有温度自适应性,而且具有低纹波、低噪声、低功耗和电气安全隔离的特点,能在9~36 VDC宽输入电压范围和-40~70℃环境下良好工作。 相似文献
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Yasunori Saito Tomoyuki Maruyama Hideaki Yamaki Fumitoshi Kobayashi Takuya D. Kawahara Akio Nomura Mitsuyoshi Tanaka 《Optical Review》1999,6(5):459-463
Static characteristics of two different structured InAlGaAs/InAlAs superlattice avalanche photodiodes (SLAPDs) cooled by liquid nitrogen were evaluated at a wavelength of 1.5 μm. The dark current of the SLAPD having a thick superlattice layer of 0.504 μm was 5 × 10−13 A. This was successively reduced by four orders of magnitude compared to that of the thin layer SLAPD of 0.231 μm at a breakdown voltage of around 20 V. The thickened layer was effective in suppressing tunneling dark current. An output current of 1.7×l0−12 A at a bias voltage of 15 V was measured for an optical input with a wavelength of 1.5 μm and a signal power of 1 × 10−12 W. This showed a sharp distinction from the dark current. 相似文献
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A. M. Povolotsky V. B. Priezzhev Chin-Kun Hu 《Journal of statistical physics》2003,111(5-6):1149-1182
An asymmetric stochastic process describing the avalanche dynamics on a ring is proposed. A general kinetic equation which incorporates the exclusion and avalanche processes is considered. The Bethe ansatz method is used to calculate the generating function for the total distance covered by all particles. It gives the average velocity of particles which exhibits a phase transition from an intermittent to continuous flow. We calculated also higher cumulants and the large deviation function for the particle flow. The latter has the universal form obtained earlier for the asymmetric exclusion process and conjectured to be common for all models of the Kardar–Parisi–Zhang universality class. 相似文献
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Abstract Recently pulses of the electromagnetic cosmic radiation of varies frequency ranges were detected by means of space flight equipment [1]. But so far the physical nature of the sources of these pulses are not well known. Since the generators of these pulses are at far distances obviously, the latters should have considerable power. But in this case we are forced to accepte that that the radiation is generated not only by the surface but also by the bulk mass of the distant object. It is also reasonable to propose that the objects are superdense ones [2]. In the Latter case the electromagnetic radiation cann't difused up to the surface of a superdense object from the centre and so no electromagnetic and acoustic processes can give radiation from the bulk mass of an object. On the contrary gravitational and neutrino radiation may be generated by the bulk mass of a massive object and at the surface of these objects these radiations tightly bounded to matter may be partly transformed into electromagnetic radiation [3]. And we can suppose that namely this very small part of the whole radiational energy is at time registrated at the earth and space laboratories. The mauy ask why all of the remaining purt of teh rediated energy has not been detected yet? There where made some attempts to performe neutrino astronony equipment out no solar neuttinos have been detected yet. As to the camical gravitational radiation it is pregently inveutigated only at low frequencles and no distinet conclucion about its occurence in been reached in the lilorature. 相似文献
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提出了四能级耦合系统的光子雪崩上转换模型,首先从理论上分析了光子雪崩产生的条件,给出了雪崩阈值以及在低于或高于阈值条件下荧光强度随时间变化关系;再将该模型结合数值分析应用于Tm^3+:LiYF4晶体这一列,理论分析结果与实验基本一致。因此应用此模型及其理论结果将有助于探索新型光子雪崩上转换材料。 相似文献
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Based on the standard self-organizing map (SOM) neural network model and an integrate-and-fire mecha-nism, we introduce a kind of coupled map lattice system to investigate scale-invariance behavior in the activity of modelneural populations. We find power-law distribution behavior of avalanche size in our model. But more importantly, wefind there are different avalanche distribution behaviors in different specific areas of our system, which are formed by thetopological learning process of the SOM net. 相似文献
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ZHAOXiao-Wei CHENTian-Lun 《理论物理通讯》2003,40(3):363-368
Based on the standard self-organizing map (SOM) neural network model and an integrate-and-fire mecha-nism, we introduce a kind of coupled map lattice system to investigate scale-invariance behavior in the activity of model neural populations. We find power-law distribution behavior of avalanche size in our model. But more importantly, we find there are different avalanche distribution behaviors in different specific areas of our system, which are formed by the topological learning process of the SOM net. 相似文献