一个反宇宙β-γ巧合系统用于放射测量
Qi Li1, YuanQing Fan1, ShiLian Wang1
1CTBT Beijing National Data Centre and Beijing Radionuclide Laboratory, Beijing, 100085, China.
概括
一个新的反宇宙β-玛巧合系统增强了放射探测灵敏度. 该系统显著降低了背景噪声,实现了关键的同位素的超低最低可检测活性水平.
科学领域:
- 核物理 核物理 核物理
- 环境监测环境监测环境监测
- 放射化学 放射化学是指辐射化学.
背景情况:
- 高检测灵敏度对于放射性子测量至关重要.
- 背景辐射,特别是来自宇宙射线子,可以干扰敏感的测量.
- 现有的β-玛巧合系统需要进一步优化性能.
研究的目的:
- 开发和实施一个反宇宙探测器系统,用于beta-gamma巧合设置.
- 为了减少由宇宙射线子引起的背景噪音.
- 评估升级的放射测量系统的性能提升.
主要方法:
- 整合一个宇宙射线否决探测器与宽能 gamma探测器和塑料闪光灯β探测器.
- 对抗宇宙β-玛巧合系统的设置和调试.
- 24小时测量活动,以评估系统性能和背景减少.
主要成果:
- 反宇宙系统有效地减少了背景噪音.
- 为131mXe实现的最小可检测活动 (MDA):0.9 mBq.
- 在133mXe: 1.1 mBq,133Xe: 2.2 mBq,和135Xe: 2.1 mBq.中实现了MDA.
结论:
- 实施的反宇宙系统显著提高了beta-gamma巧合设置的检测灵敏度.
- 该系统在超低MDA值的放射监测方面表现出色.
- 这一进步对于准确的环境监测和核事件检测至关重要.
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