首页> 外文会议>International Conference on Particle Physics and Astrophysics >Modeling of low-energy charged particles passage through GAMMA-400 gamma-telescope thermal insulation and two-layer plastic scintillation detectors used as anticoincidence shield
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Modeling of low-energy charged particles passage through GAMMA-400 gamma-telescope thermal insulation and two-layer plastic scintillation detectors used as anticoincidence shield

机译:通过伽玛-400伽马 - 望远镜的低能量带电粒子通过抗渗抗和双层塑料闪烁探测器的模拟。

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The results of low-energy charged particles passage through GAMMA-400 gamma-telescope thermal insulation and two-layer plastic scintillation detectors used as anticoincidence shield are presented. An existing GEANT4 GAMMA-400 model is used. Effects of thermal insulation on charged particle passage are investigated. These results will be used to testing the effect of low-energy charged particles flux on GAMMA-400 gamma-quanta registration capabilities. Sufficiently large energy deposition in two-layer plastic anticoincidence scintillation detectors might interfere with high-energy particle registration and identification. However, GAMMA-400 detection capabilities are not affected by this, as the energy deposition in the lower layer of S3 is less than 1.5 MeV in all simulated cases. This value is less than threshold for high energy particles identification start (2.5 MeV). It makes impossible to incorrectly identify a low-energy charged particle energy deposition as backsplash from a high-energy gamma-quantum.
机译:提供了通过伽马-400伽马望远镜的低能量带电粒子通道的结果和用作抗凝视屏蔽的双层塑料闪烁探测器。使用现有的GEANT4 GAMMA-400模型。研究了热绝缘对带电粒子通道的影响。这些结果将用于测试低能量带电粒子通量对γ-400伽马 - QUAMA - Quanma登记能力的影响。在两层塑料抗渗透闪烁探测器中足够大的能量沉积可能干扰高能粒子配准和鉴定。然而,伽玛-400检测能力不受这一点,因为在所有模拟案例中,由于S3的下层中的能量沉积小于1.5meV。该值小于高能粒子识别开始(2.5 meV)的阈值。它不可能从高能量伽马量子中错误地识别作为背板的低能量带电粒子能沉积。

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