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Development of long wave infrared detectors for space astronomy.

机译:用于太空天文学的长波红外探测器的开发。

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摘要

This thesis details the research and development of 10mum cutoff detector arrays conducted at the University of Rochester in conjunction with Rockwell Scientific. Through my data analysis and theoretical modeling of detector characteristics, processes which prevent the detector arrays from meeting low background astronomical specifications are determined and fed back to the manufacturer. The first set of deliveries were manufactured in a banded format with multiple diode structures. Data analysis indicated that the smallest capacitance diode structure exhibited the lowest dark currents and the highest yield of pixels (28%) meeting the goal of less than 100e -/s dark current with adequate (> 45mV) well depth. The mechanisms limiting dark current were found to be surface current at lower biases and tunneling (trap-to-band and band-to-band) at higher biases. In order to reduce stress at the junction during hybridization (a leading cause of the observed tunneling current), a proprietary bonding method was developed by Rockwell Scientific. New detector arrays, manufactured with the optimum diode structure and bonded with the new bonding technique to the HAWAII-1RG multiplexer, showed an impressive 75% of pixels exhibiting dark current less than 30e -/s with sufficient (> 40mV) well depth. Most of these pixels exhibited extremely low dark currents, less than 0.3e -/s. I found that the dark current limiting mechanism at lower biases was still surface current on the front-side, caused by passivation processing techniques. The limiting mechanism at high biases was dislocation-induced early breakdown which took the shape of a screw dislocation (or micropipe) on an I-V curve of dark current, manifesting as a sharp increase in trap-to-band tunneling current. Burst noise was also detected in the source follower unit cell FET of the multiplexer and was fully characterized and explored. It was discovered that the burst noise was a result of oxide trapping of a single charge for most of the observed two-level characteristics. Other, more complicated forms exhibited by some pixels suggested that some multi-carrier traps exist in the bulk silicon close to the channel. With the results presented in this thesis, Rockwell Scientific will again improve their processing and manufacturing techniques on both detectors and multiplexers.
机译:本文详细介绍了与罗克韦尔科学公司一起在罗切斯特大学进行的10mm截止检测器阵列的研究和开发。通过我的数据分析和探测器特性的理论建模,确定了防止探测器阵列满足低背景天文规格的过程,并将其反馈给制造商。第一组交付以带多个二极管结构的带状形式制造。数据分析表明,最小的电容二极管结构表现出最低的暗电流和最高的像素合格率(28%),满足了井深(> 45mV)时暗电流小于100e-/ s的目标。发现限制暗电流的机制是在较低偏压下的表面电流,以及在较高偏压下的隧穿(陷波至频带和频带至频带)。为了减少杂交过程中接合处的应力(观察到的隧穿电流的主要原因),Rockwell Scientific开发了一种专有的键合方法。新的探测器阵列采用最佳的二极管结构制造,并通过新的粘合技术与HAWAII-1RG多路复用器粘合,显示出令人印象深刻的75%像素,其暗电流小于30e-/ s,且具有足够的阱深度(> 40mV)。这些像素大多数都表现出极低的暗电流,小于0.3e-/ s。我发现,在较低偏置下的暗电流限制机制仍然是钝化处理技术在正面产生的表面电流。在高偏压下的限制机制是位错引起的早期击穿,其在暗电流的I-V曲线上呈螺旋位错(或微管)的形状,表现为陷阱至带隧穿电流的急剧增加。在多路复用器的源极跟随器单元电池FET中也检测到了突发噪声,并对其进行了全面表征和研究。已经发现,对于大多数观察到的两能级特征,猝发噪声是单电荷的氧化物俘获的结果。一些像素表现出的其他更复杂的形式表明,在靠近通道的体硅中存在一些多载流子陷阱。凭借本文提出的结果,罗克韦尔科学公司将再次改进其在检测器和多路复用器上的处理和制造技术。

著录项

  • 作者

    Bacon, Candice Marie.;

  • 作者单位

    University of Rochester.;

  • 授予单位 University of Rochester.;
  • 学科 Physics Astronomy and Astrophysics.;Physics Condensed Matter.
  • 学位 Ph.D.
  • 年度 2006
  • 页码 184 p.
  • 总页数 184
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 11:40:38

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