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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research >A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector
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A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector

机译:用XMASS-I检测器测量液态氙中低能伽马射线引起的闪烁的时间曲线

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摘要

We report the measurement of the emission time profile of scintillation from gamma-ray induced events in the XMASS-I 832 kg liquid xenon scintillation detector. Decay time constant was derived from a comparison of scintillation photon timing distributions between the observed data and simulated samples in order to take into account optical processes such as absorption and scattering in liquid xenon. Calibration data of radioactive sources, ~(55)Fe, ~(241)Am, and ~(57)Co were used to obtain the decay time constant. Assuming two decay components, τ_1 and τ_2, the decay time constant τ_2 increased from 27.9 ns to 37.0 ns as the gamma-ray energy increased from 5.9 keV to 122 keV. The accuracy of the measurement was better than 1.5 ns at all energy levels. A fast decay component with τ_1 ~ 2 ns was necessary to reproduce data. Energy dependencies of τ_2 and the fraction of the fast decay component were studied as a function of the kinetic energy of electrons induced by gamma-rays. The obtained data almost reproduced previously reported results and extended them to the lower energy region relevant to direct dark matter searches.
机译:我们报告了在XMASS-I 832公斤液态氙闪烁探测器中由伽马射线诱发的事件引起的闪烁发射时间分布的测量结果。衰减时间常数是通过比较观察到的数据与模拟样品之间的闪烁光子时间分布而得出的,以便考虑光学过程,例如在液态氙中的吸收和散射。使用放射性源〜(55)Fe,〜(241)Am和〜(57)Co的校准数据来获得衰减时间常数。假设两个衰减分量τ_1和τ_2,随着伽马射线能量从5.9 keV增大到122 keV,衰减时间常数τ_2从27.9 ns增加到37.0 ns。在所有能量水平下,测量精度均优于1.5 ns。要再现数据,必须具有τ_1〜2 ns的快速衰减分量。研究了τ_2的能量依赖性和快速衰减分量的分数与伽马射线诱导的电子动能的关系。获得的数据几乎重现了先前报告的结果,并将其扩展到了与直接暗物质搜索有关的较低能量区域。

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  • 作者单位

    Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8601, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kamioka Observatory, Institute for Cosmic Ray Research, The University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan,Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 305-811, South Korea;

    Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 305-811, South Korea;

    Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8601, Japan,Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan;

    Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8601, Japan;

    Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8601, Japan;

    Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8601, Japan;

    Institute of Socio-Arts and Sciences, The University of Tokushima, 1-1 Minamijosanjimacho Tokushima city, Tokushima 770-8502, Japan;

    Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan;

    Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Kavli Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba 277-8582, Japan,Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan;

    Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 305-811, South Korea,Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea;

    Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea;

    Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea;

    Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea;

    Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan;

    Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan;

    Department of Physics, Faculty of Engineering, Yokohama National University, Yokohama, Kanagawa 240-8501, Japan;

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  • 正文语种 eng
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  • 关键词

    Decay time constant; Liquid xenon; Scintillator;

    机译:衰减时间常数;液态氙闪烁体;

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