中子的作用不同于质子。
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.
中子携带的能量可转化为热能。
The neutron would carry energy that could be converted into heat.
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.
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.
它最常见的形式或者同位素有146个中子。
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.
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.
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.
简要阐述了光中子产生的反应机理。
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.
它可对中子辐射进行直接，可视的探测。
Furthermore, its measure of neutron rays is visual and direct.
对肿瘤区的贡献主要来自硼中子吸收反应。
The major contribution to the tumor zone is from the neutron capture reaction of boron.
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).
其次，我们研究了零温时中子星物质的物态方程。
Secondly, the equation of state of neutron matter at zero temperature is studied.
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.
最后，我们研究了中子星的质量和半径。
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.
但是，当中子运动时，却没有运动轨迹的踪影。
详细地介绍了中子与密度测井在东濮凹陷勘探中的应用情况。
This article will introduce the application of neutron-density log in Dongpu depression exploration.
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.
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.
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