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.
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.
由于对于非对称核物质性质的研究有助于对中子星物质的认识，考察了非对称致密热核物质的液—气相变。
As the study of properties of warm asymmetric nuclear matte may shed a light on the study of neutron star, the liquid-gas phase transition of warm asymmetric nuclear matte is investigated.
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