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GAMMA HEATING ESTIMATE AT THE MCMASTER NUCLEAR REACTOR

机译:麦克马斯特核反应堆的伽玛加热估计

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Gamma heating is an important issue that can contribute significantly to the heat generation in the reactor core, either by prompt- or delayed decay processes. While photons account for around 7% of the total energy produced in fission along with the additional component of capture gamma production, this is still a considerable amount of energy created. In this paper, a measurement has been carried out to estimate the nuclear heating using a Halden-type Gamma Thermometer (GT) at the McMaster Nuclear Reactor (MNR). It was found that around 84 ± 8.4 % of the measured nuclear heating in non-fuel regions is due to the prompt gamma, including radioactive captures, and a maximum of around 14 ± 1.4 % is due to the decay gamma heat. The latter usually occurs immediately after the reactor shuts down and then it decreases exponentially.
机译:伽玛加热是一种重要的问题,可以通过促进或延迟衰变过程显着贡献反应器核中的热量。虽然光子占裂变中产生的总能量的约7%以及捕获伽马生产的附加组分,但这仍然是相当数量的能量。在本文中,已经进行了测量以在McMaster核反应堆(MNR)处使用Halden型γ温度计(GT)来估计核加热。发现在非燃料区中测量的核加热约84±8.4%是由于伽马,包括放射性捕获,最大约14±1.4%是由于衰减伽马热量。后者通常在反应器关闭后立即发生,然后呈指数递减。

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