自给能中子探测器温度依赖性全链路建模与主因分析

Full-link Modeling and Principal Factor Analysis of Temperature Dependence on Self-powered Neutron Detector

  • 摘要: 为探究温度对自给能中子探测器(SPND)响应的影响规律,提出一种全链路四因子分析模型,用于研究SPND的温度依赖性。该模型基于蒙特卡罗方法,在300~800 K范围内,将温度对典型发射极和绝缘层材料的SPND信号的影响分解为核反应率、几何形变、电场屏蔽以及宏观分流4个因子进行定量评估。研究结果表明:在所选温区内,中子能谱硬化所引发的核反应率衰减是导致探测器信号下降的主导因素,使SPND的灵敏度下降约(35.0±1.5)%;电场屏蔽效应仅在300 K左右且内建负电势垒达105 V量级时,会显著抑制电子输运,使灵敏度下降超过10%;而当温度升至400 K以上时,其对灵敏度的影响随之降至1%以内;几何形变与宏观分流效应对探测器灵敏度的影响可忽略不计。

     

    Abstract: Real-time monitoring of in-core neutron flux density is crucial for reactor safety. Although self-powered neutron detectors (SPNDs) are widely used, severe core temperature fluctuations significantly alter their sensitivity. Existing studies mostly focus on single factors, lacking a systematic quantitative evaluation of the full-link cascaded physical processes. Therefore, this study proposes a full-link four-factor decomposition physical model describing the temperature dependence of SPNDs. The objective is to elucidate the decisive mechanisms of temperature variations on SPND signal responses from 300 K to 800 K, providing a theoretical basis for high-precision temperature compensation. The model decoupled the output current of the detector into a reference primary current and four independent factors: nuclear reaction rate, geometric deformation, electric field shielding, and macroscopic shunting. Based on the Monte Carlo method and the SPNDSignal platform, high-fidelity computational models containing Co, Rh, and V emitters alongside oxide insulators were constructed. The study calculated the attenuation of the nuclear reaction rate using the NJOY program, reconstructed the geometric model according to the linear expansion coefficient, simulated the space charge shielding by jointly solving the continuity and Poisson equations, and established an equivalent circuit model to analyze the shunting loss. Through step-by-step additive simulations, the independent contribution of each factor was precisely quantified. Results show that the attenuation of the nuclear reaction rate caused by neutron spectrum hardening is the absolute dominant factor leading to the signal decrease, causing a sensitivity drop of approximately (35.0±1.5)% for SPNDs. The space charge effect is a typical low-temperature threshold perturbation mechanism, but its impact is minimal under actual reactor operating conditions. When the neutron flux density is constant at 1013 cm−2·s−1, when the temperature is around 300 K and the built-in negative potential barrier reaches the order of 105 V does the detector sensitivity show a decrease of over 10%. As the temperature rises above 400 K, with the sudden drop in insulation resistivity, the shielding effect attenuates rapidly, and its impact falls below 1%. Supplementary simulations indicate that in practical conditions, it is difficult for the insulation layer to build up a potential barrier sufficient to significantly inhibit electron transport. Therefore, within the selected temperature range, the impact of the space charge effect on the signal output is almost negligible. Furthermore, geometric perturbations caused by thermal expansion (with a deviation of only 0.27%) and the shunting rate under extreme high-temperature conditions (in the order of 10−5) do not constitute substantial signal attenuations. In summary, the temperature response characteristics of SPNDs over a wide temperature range are determined by microscopic nuclear reaction mechanisms, and neutron spectrum hardening is the core dominant factor for sensitivity drift. The space charge effect is theoretically a severe perturbation term in the low-temperature region but can be neglected in practical engineering; similarly, geometric and shunting effects are also negligible in engineering applications.

     

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