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 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。
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。
Immediately after supernova, if the remnant core has a mass of less than three SUNS, one would expect a blob of degenerate neutron matter to be spinning in the explosion's wake.
在经历超新星后，假如剩下的残核小于三个太阳质量，爆炸的残余物质就将可能演变成旋转着的中子团。
But the best thing is that they don't have to actually create neutron degenerate matter itself, just cool some lithium-6 gas to nearly absolute zero, grab it inside a laser trap and make it wobble.
但最好的事情莫过于他们不必真的制造出中子简并物质本身，只要把一些锂- 6气体冷却到接近绝对零度，然后把它们抓到激光阱并使之振动即可。
But they didn't have to scoop a chunk of neutron degenerate matter from the surface of a real neutron star either.
但他们也并不需要从一颗真正的中子星表面挖来一块中子星简并物质。
After the supernova, the leftover matter could either have collapsed into a black hole or an extremely dense neutron star.
超新星爆发以后，剩余的物质可能塌缩为一个黑洞，也可能形成一颗密度极大的中子星。
They go around in the plane of the blackboard, say, and so this matter cannot fall radially in but it will fall in and spiral in and forms what we call an accretion disk around the neutron star.
平面内绕行，这个质量不是，呈放射状减小，而是，呈螺旋形减小，我们称之为中子星，周围的吸积盘，这个叫做吸收星。
And I take a little bit of matter m, and I drop it from a large distance onto the neutron star.
从很远的距离扔到，中子星上，那个小物体。
The dark matter star would collapse into a black hole. "Then the neutron star won't be able to survive anymore, and it'll collapse too," says Fairbairn.
“暗物质恒星就会坍塌成为黑洞，然而，在这个时候，包围它的中子恒星不能再存在下去，也会跟着一起坍塌”，费尔贝恩说。
The dark matter star would collapse into a black hole. "Then the neutron star won't be able to survive anymore, and it'll collapse too, " says Fairbairn.
“暗物质恒星就会坍塌成为黑洞，然而，在这个时候，包围它的中子恒星不能再存在下去，也会跟着一起坍塌” ，费尔贝恩说。
"We could look for evidence that neutron stars don't live very long in regions with a lot of dark matter," he says.
“我们可以寻找证据表明，中子恒星不会长期地居留在有大量暗物质存在的区域里”，他说。
"This state of matter doesn't exist anywhere naturally on Earth and is thought to only now occur during the collision of two neutron stars," he said.
“这种物质状态在地球上的任何地方都不会自然存在，如果想现在出现这种状态，只有在两颗中子星发生碰撞期间。”他说。
And this is another view that gives you an idea of the donor and then the swirl of matter, and then it swirls in and ends up here on the neutron star.
给你供体星的概念，然后是物体的旋转，它旋转，终止于中子星上，这里你看到的是。
As matter falls onto the neutron star, it gives off X-rays.
当伴星物质陷落到中子星上时，它就发射出X射线。
The phase transition of two-flavor quark matter into strange matter in the interior of a neutron star is studied.
研究了中子星内部从两味夸克物质到三味夸克物质的相变过程。
Properties of nuclear matter and neutron star are described in relativistic mean field theory with density-dependent effective interactions.
基于密度相关有效相互作用的相对论平均场理论，研究了核物质和中子星的性质。
Neutrinos occupy about 43% of the neutron mass, If the universe as a medium and large child, Neutrino accounted for 43% of total mass of the universe, It is the so-called "dark matter".
中微子占有中子质量的43％左右，如果把宇宙看成一个大中子，中微子则占宇宙总质量的43％，它就是所谓“暗物质”。
Analysis of the X-ray data shows that the point sources are associated with binary star systems that contain a neutron star or black hole that is pulling matter away from a normal star.
对X射线数据的分析表明，点源与包含有中子星或黑洞(它们正从正常恒星吸走物质)的双星系统成协。
The equation works on every body of matter and every particle of matter in the universe, including black holes, neutron stars, white dwarf stars, stars, and nuclei.
这个方程既适用于黑洞、中子星、白矮星及恒星，也适用于原子核。
The equation works on every body of matter and every particle of matter in the universe, including black holes, neutron stars, white dwarf stars, stars, and nuclei.
这个方程既适用于黑洞、中子星、白矮星及恒星，也适用于原子核。
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