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High-resolution Compton cameras based on Si/CdTe double-sided strip detectors

机译:基于Si / CdTe双面带状探测器的高分辨率康普顿相机

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摘要

We have developed a new Compton camera based on silicon (Si) and cadmium telluride (CdTe) semiconductor double-sided strip detectors (DSDs). The camera consists of a 500-μm-thick Si-DSD and four layers of 750-μm-thick CdTe-DSDs all of which nave common electrode configuration segmented into 128 strips on each side with pitches of 250 μm. In order to realize high angular resolution and to reduce size of the detector system, a stack of DSDs with short stack pitches of 4 mm is utilized to make the camera. Taking advantage of the excellent energy and position resolutions of the semiconductor devices, the camera achieves high angular resolutions of 4.5° at 356 keV and 3.5° at 662 keV. To obtain such high resolutions together with an acceptable detection efficiency, we demonstrate data reduction methods including energy calibration using Compton scattering continuum and depth sensing in the CdTe-DSD. We also discuss imaging capability of the camera and show simultaneous multi-energy imaging.
机译:我们开发了一种新的基于硅(Si)和碲化镉(CdTe)半导体双面带状检测器(DSD)的康普顿相机。该相机由一个500μm厚的Si-DSD和四层750μm厚的CdTe-DSD组成,所有这些都具有简单的公共电极配置,每侧分成128条,间距为250μm。为了实现高角度分辨率并减小检测器系统的尺寸,利用具有4mm的短堆叠间距的DSD堆叠来制造相机。利用半导体器件出色的能量和位置分辨率,该摄像机可在356 keV时获得4.5°的高角分辨率,在662 keV时达到3.5°的高角分辨率。为了获得如此高的分辨率以及可接受的检测效率,我们演示了数据缩减方法,包括使用Compton散射连续体和CdTe-DSD中的深度感应进行能量校准。我们还将讨论相机的成像功能并显示同步多能量成像。

著录项

  • 来源
    《Nuclear Instruments & Methods in Physics Research》 |2012年第2012期|179-183|共5页
  • 作者单位

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan;

    Department of High Energy Astrophysics, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodtn,Chuo, Sagamihara, Kanagawa 252-5210, Japan,Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Takasaki Advanced Radiation Research Institute, Japan Atomic Energy Agency (JAEA), 1233 Watanuki-machi, Takasaki, Gunma 370-1292, Japan;

    Kavli Institute for Particle Astrophysics and Cosmology. Stanford University, Stanford, CA 94305, USA;

    Solar-Terrestrial Environment Laboratory, Nagoya University, Furo-cho, Chikusa, Nagoya 464-8601, Japan;

    Department of Physics, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan;

    Department of Physical Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan;

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  • 正文语种 eng
  • 中图分类
  • 关键词

    gamma-ray imaging; compton camera; cdte double-sided strip detector;

    机译:伽玛射线成像;康普顿相机cdte双面条形检测仪;

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