如果中子的变动率是0，那就是它了。
中子的作用不同于质子。
这个基本的等式是用来描述中子如何积累的过程。
This basic equation is used to describe how neutrons accumulate.
科学家发现的其他中子星均要比这颗更老。
Every other neutron star identified by scientists has been much older.
那个特定的中子，会被捕获的可能性就越小。
And then that's less likely that particular neutron will be captured.
中子携带的能量可转化为热能。
The neutron would carry energy that could be converted into heat.
这些混合物发生反应后就形成氦元素，并同时生成更多的中子与大批量的能量。
These react to form helium, yet more neutrons and a whole lot more energy.
这是因为，大多数到达地球的微中子都要从中穿过。
That is because most of the neutrinos that reach the Earth pass right through it.
新发现的这颗中子星只有单一的碳大气层，厚十余厘米。
The newly identified neutron star has a unique atmosphere of carbon just centimetres thick.
当然，这需要一个合适的微中子望远镜。
Of course, you would need an appropriate neutrino telescope to do this.
中子星旋转的计时，如果中子星。
这也是实验得以类比中子星物质的地方。
This is where the experiment becomes analogous to the material of a neutron star.
分散在超大质量黑洞周围的中子星。
资源目录中子目录列表中的下一个目录是ejb目录。
Next in our list of subdirectories, in the resources directory, is the ejb directory.
最常见的矿物识别交会图是中子-密度交会图。
The most common mineral identification plot is a neutron-density cross plot.
最后，我们研究了中子星的质量和半径。
但是，当中子运动时，却没有运动轨迹的踪影。
少量的裂变材料不能维持链式反应(绝大多数中子逃逸了)。
The few fissile materials could not maintain the chain type response (overwhelming majority neutron escape).
在棒的四周围着中子减速剂。
对于大多数这样的星球来说，星球核心最终会变成一颗中子星。
For most such stars, the core is left behind as a neutron star.
对中子，壳的影响非常明显。
本文对水堆中的中子局部噪声和整体噪声进行了理论分析。
The local and global components of neutron noise in water reactor are ana-lysed.
根据这个估算，他们可以估计有多少中子会通过地球的特定区域。羾。
From this they estimated how many neutrinos should pass through a particular location on Earth.
含氢指数是中子孔隙度测井响应的主要参数。
It is a key factor in the response of a neutron porosity log.
我们知道，这些物体是存在的，因为使用射电望远镜已经观察到了几个中子星。
We know that these objects exist because several have been found using radio telescopes.
本文报告了我国中子计的进展。
In this paper, the progress of neutron gauges in China is reported.
它最常见的形式或者同位素有146个中子。
它最常见的形式或者同位素有146个中子。
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