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Simulation and optimization of a soft gamma-ray concentrator using thin film multilayer structures

机译:使用薄膜多层结构模拟和优化软伽玛射线聚光器

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摘要

We are reporting the investigation result of using multilayer thin film structures for channeling and concentrating soft gamma rays with energies greater than 100 keV, beyond the reach of current grazing-incidence hard X-ray mirrors. This will enable future telescopes for higher energies with same mission parameters already proven by NuSTAR. A suitable arrangement of bent multilayer structures of alternating low and high-density materials will channel soft gamma-ray photons via total external reflection and then concentrate the incident radiation to a point. We present the latest results of producing Ir/Si and W/Si multilayers with the required thicknesses and smoothness by using magnetron sputter technique, In addition to experimental works, we have been working on gamma-ray tracking model of the concentrator by IDL, making use of optical properties calculated by the IMD software. This modeling allows us to calculate efficiency and track photon for different energy bands and materials and compare them with experimental result. Also, we describe combine concentrator modeling result and detector simulation by MEGAlib to archive a complete package of gamma-ray telescope simulation. This technology offers the potential for soft gamma-ray telescopes with focal lengths of less than 10 m, removing the need for formation flying spacecraft and providing greatly increased sensitivity for modest cost and complexity and opening the field up to balloon-borne instruments.
机译:我们正在报告使用多层薄膜结构来引导和聚集能量大于100 keV的软伽玛射线的研究结果,这超出了当前掠入射硬X射线镜的范围。这将使未来的望远镜具有更高的能量,并且具有NuSTAR已经证明的相同任务参数。交替排列的低密度和高密度材料的弯曲多层结构的合适布置将通过全外反射引导软伽马射线光子,然后将入射辐射集中到一个点。我们介绍了使用磁控溅射技术生产具有所需厚度和光滑度的Ir / Si和W / Si多层膜的最新结果,除实验工作外,我们还一直在研究IDL选矿厂的伽马射线跟踪模型,使用IMD软件计算的光学性能。该模型使我们能够计算效率并跟踪不同能带和材料的光子,并将其与实验结果进行比较。此外,我们描述了结合聚光器建模结果和MEGAlib进行的探测器仿真,以归档完整的伽马射线望远镜仿真包。这项技术为焦距小于10 m的软伽马射线望远镜提供了潜力,从而消除了对编队飞行航天器的需求,并为适度的成本和复杂性大大提高了灵敏度,并为气球型仪器打开了视野。

著录项

  • 来源
    《Optics for EUV, x-ray, and gamma-ray astronomy VIII》|2017年|103991A.1-103991A.11|共11页
  • 会议地点 San Diego(US)
  • 作者单位

    Space Science Center, University of New Hampshire, Durham, NH 03824 USA,Department of Physics, University of New Hampshire, Durham, NH 03824 USA;

    Space Science Center, University of New Hampshire, Durham, NH 03824 USA,Department of Physics, University of New Hampshire, Durham, NH 03824 USA;

    Materials Science Program, University of New Hampshire, Durham, NH 03824 USA,Department of Mechanical Engineering, University of New Hampshire, Durham, NH 03824 USA;

    Space Science Center, University of New Hampshire, Durham, NH 03824 USA;

    Space Science Center, University of New Hampshire, Durham, NH 03824 USA,Department of Physics, University of New Hampshire, Durham, NH 03824 USA,Southwest Research Institute, Department of Earth, Oceans, and Space, Durham, NH 03824 USA;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Soft gamma-ray astronomy; Gamma-ray optics; Gamma-rays; Thin-film multilayers; Magnetron sputtering;

    机译:软伽玛射线天文学;伽玛射线光学;伽马射线;薄膜多层;磁控溅射;

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