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The development of two-phase xenon dark matter detectors.

机译:氙气两相暗物质探测器的发展。

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摘要

The nature of dark matter remains one of the great unsolved mysteries of modern physics. The existence of dark matter has been inferred from its gravitational interactions and is strongly supported on theoretical grounds. A primary candidate for the dark matter is the Weakly Interacting Massive Particle (WIMP), which may be an undiscovered particle from the supersymmetric sector. This dissertation describes the research and development in two-phase liquid xenon dark matter detector technology and the results from the full-scale detector XENON10. Two-phase liquid xenon detectors use position sensitivity and simultaneous measurement of light and charge to remove background electron recoil events. The development of this technology has been rapid -- the work in this dissertation began in the summer of 2003 when the potential of this technology had yet to be determined, and in early 2008 the XENON10 collaboration published the then world-best upper limit on the spin-independent WIMP-nucleon cross section. The first measurement of the charge based discrimination performance at low energies was achieved in a prototype in early 2005. This prototype also determined the performance of discrimination via scintillation pulse shape. Although pulse shape discrimination was shown to be far weaker than that from charge yield, the combined use of the two methods demonstrated a discrimination power beyond that achieved by either method alone. Alternative detector technologies were also explored. Electron multiplication on wire grids was demonstrated in a two-phase prototype and its discrimination power potential is shown to be near that of the typical electroluminescence charge-readout technique. This could allow for the removal of some or all of the photo-multipliers in the detector, which would greately reduce radioactive backgrounds. The use of a wavelength shifter was tested in an attempt to improve light collection and was shown to impede charge collection. The magnitude of fluctuations in recombination in electron recoils, which are an important component in charge resolution, was also measured. The final chapter describes the XENON10 detector, its operation at the Gran Sasso National Laboratory, the analysis of the data, and the results of the WIMP search.
机译:暗物质的性质仍然是现代物理学尚未解决的重大谜团之一。暗物质的存在是从其引力相互作用推断出来的,并在理论上得到了有力的支持。暗物质的主要候选者是弱相互作用质量粒子(WIMP),它可能是超对称扇区中未发现的粒子。本文介绍了两相液体氙暗物质检测器技术的研究与发展,以及全尺寸XENON10检测器的研究成果。两相液体氙探测器使用位置灵敏度并同时测量光和电荷,以消除背景电子反冲事件。这项技术的发展非常迅速-本论文的工作始于2003年夏天,当时还没有确定这项技术的潜力。2008年初,XENON10合作发布了当时世界上最高的上限。自旋无关的WIMP核子截面。在2005年初的一个原型中,首次测量了低能量下基于电荷的辨别性能。该原型还通过闪烁脉冲形状确定了辨别性能。尽管显示出脉冲形状判别能力远不如电荷产量判别能力强,但两种方法的组合使用证明了判别能力超出了单独使用任一方法所能达到的能力。还探索了替代检测器技术。在两相原型中证明了线栅上的电子倍增,并且其判别能力电势已显示出与典型的电致发光电荷读出技术相近。这可以允许去除检测器中的一些或所有光电倍增器,这将大大减少放射性背景。测试了波长偏移器的使用,以尝试改善光的收集,并证明它会阻碍电荷的收集。还测量了电子反冲中复合波动的幅度,这是电荷分辨力的重要组成部分。最后一章介绍了XENON10检测器,在Gran Sasso国家实验室的操作,数据分析以及WIMP搜索的结果。

著录项

  • 作者

    Kwong, John.;

  • 作者单位

    Princeton University.;

  • 授予单位 Princeton University.;
  • 学科 Physics Astronomy and Astrophysics.;Physics Elementary Particles and High Energy.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 351 p.
  • 总页数 351
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;高能物理学;
  • 关键词

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