effective neutron temperature 有效中子温度
neutron-temperature measurement 中子测温
high temperature neutron diffraction 高温中子衍射
temperature neutron 中子温度
finite-temperature neutron star 有限温度中子星
But all this stuff, these cross sections are measured as a function of energy, they're measure as a function of the neutron energy which is a function of the temperature of the particular medium.
但是，所有这个材料，这些横截面被测量的，是以能量的函数，它们是测量，中子能量的函数，那也是特定的媒介的，温度的函数。
Secondly, the equation of state of neutron matter at zero temperature is studied.
其次，我们研究了零温时中子星物质的物态方程。
The large nuclear temperature evaluation would violate conservation of energy, and may lead a negative neutron KERMA factor.
这就可能使评价核温度太高而导致平均次级中子能量（?） 过大，破坏了能量守恒，而导致了负KERMA因子。
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