在近距离几何测量中,BEGe探测器的真实巧合总和校正
Ashish Gupta1, M Shareef2, Munmun Twisha1
1Saha Institute of Nuclear Physics, 1/AF, Bidhan Nagar, Kolkata, 700064, India; Homi Bhabha National Institute, Anushaktinagar, Mumbai, 400094, India.
概括
计算了宽能探测器的巧合总和校正因数. 这种效应对距离5厘米以下的源具有显著意义,影响了马射线测量.
科学领域:
- 核物理 核物理 核物理
- 辐射检测和测量 辐射检测和测量
背景情况:
- 巧合总和在马射线光谱学中具有重要影响,特别是在接近源探测器几何学上.
- 准确的校正因子对于核测量中精确的定量分析至关重要.
研究的目的:
- 为了计算广能探测器的真实巧合总和校正因数.
- 调查源探测器几何对巧合总和效应的影响.
- 根据实验数据验证模拟方法.
主要方法:
- 使用放射性马射线源进行实验测量.
- 校正因子的分析计算.
- 用于检测器效率计算的Geant4模拟.
- 通过匹配模拟和实验效率来优化探测器参数.
主要成果:
- 对远近几何学来说,都计算了巧合总和的校正因数.
- 实验和分析校正因子显示出很好的一致性.
- 发现巧合总和效应在距离小于5厘米时是显著的.
结论:
- 该研究成功计算了宽能探测器的巧合总和校正因子.
- 当Geant4模拟被优化时,可以准确预测探测器效率.
- 接近源探测器的安排 (<5厘米) 需要仔细考虑马射线光谱学中的巧合总和效应.
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