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。

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The effect of each composition of two-body central potential on the critical density for ferromagnetic transition is calculated for neutron matter.

就中子物质计算并讨论了二体中心势中各成分对出现铁磁相变临界密度的影响。

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For neutron matter with M-S interaction, the critical density of the ferromagnetic transition, the equation of state and the neutron star models are calculated.

还计算了在M - S势作用下的中子物质出现铁磁相变的临界密度、含有铁磁相变的物态方程及中子星模型。

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So if we see the positrons coming from a particular direction, it means astrophysics like a pulsar (a type of neutron star) is responsible for the signal, not dark matter.

BBC: Alpha Magnetic Spectrometer to release first results