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Development of phonon-mediated transition-edge-sensor x-ray detectors for use in astronomy.

机译:用于天文学的声子介导的过渡边缘传感器X射线探测器的开发。

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摘要

Low temperature detectors have grown in popularity over the years for a variety of reasons. Reduced thermal noise and the associated reduction in statistical fluctuations improve signal to noise. Novel material properties at low temperature such as superconductivity can be exploited. And let us not forget easier access to cryogenic techniques, for example industry made and sold refrigerators eliminating the need for graduate students to make their own.; In this thesis I discuss development of a novel phonon-mediated distributed transition-edge-sensor x-ray detector which would be useful for astrophysical studies such as magnetic recombination in the solar corona, the warm-hot intergalactic medium and surveys of clusters and groups of galaxies.; The detector uses a large semiconductor absorber and Transition-Edge-Sensors (TESs) to readout the absorbed energy. Calorimetry is performed on individual photons and a partitioning of the energy between various TESs allows for position determination. Hence time varying astronomical sources can be spectroscopically studied and imaged.; I will conclude with a discussion of the detector's performance and propose a next generation detector which could make significant improvements on the design discussed in this thesis.
机译:多年来,由于多种原因,低温检测器已变得越来越流行。减少的热噪声和相关的统计波动减少可改善信噪比。可以利用低温下的新材料特性,例如超导性。而且,我们不要忘记更容易获得低温技术,例如,工业制造和销售的冰箱消除了研究生们自己制造冰箱的需要。在这篇论文中,我讨论了一种新型的声子介导的分布式跃迁边缘传感器x射线探测器的开发,该探测器可用于天体研究,例如太阳日冕中的磁重组,热热星际介质以及星团和群的测量星系。该检测器使用大型半导体吸收器和过渡边缘传感器(TES)读取吸收的能量。对单个光子执行量热法,并且在各种TES之间分配能量,从而可以确定位置。因此,可以对时变的天文源进行光谱研究和成像。最后,我将对检测器的性能进行讨论,并提出一种下一代检测器,它可以对本文所讨论的设计做出重大改进。

著录项

  • 作者

    Leman, Steven W.;

  • 作者单位

    Stanford University.;

  • 授予单位 Stanford University.;
  • 学科 Physics Astronomy and Astrophysics.; Physics Condensed Matter.
  • 学位 Ph.D.
  • 年度 2006
  • 页码 175 p.
  • 总页数 175
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

  • 入库时间 2022-08-17 11:39:37

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