- 更多网络例句与中子星相关的网络例句 [注：此内容来源于网络，仅供参考]
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In this scenario, a neutron star in a binary system can accrete matter from its companion.
一个双星系统中的中子星会从伴星处吸积足够物质，使得该中子星最后变成了一颗奇异星。
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But when the external fields are very strong, the trajectory of an electron begins to bifurcate, thus chaos appears.
但是 ，到了 6 0年代，人们对天体物理中的中子星进行研究时，发现中子星中的磁场很强，强到足
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At this point, a neutron star pair, or even a neutron star-black hole pair, is formed.
此刻，一个双中子星、甚至中子星-黑洞对将形成。
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When treat-ing the spectra, transition, scattering problems, we must use the semi-microscopicapproach. The main new conclusions in this thesis are following:We found the different shrinking effect in ∧ hypernuclei and 〓 hypernuclei, the shrink-ing effect in ∧ hypernuclei are confirmed in a recent experiment;We also found a new approach to treat the configuration mixing of ∧∧ hypernuclei and〓 hypernuclei and that the conversion process may change the spectra and widths of〓 hypernuclei;For the first time, we investigate the neutron star matter without the ∑ hyperon butwith the new meson 〓(975) and φ(1020), we found the contribution of 〓 and φ canmake the equation of state of neutron star soften, and the maximum mass of neutronstar reduces;we extract a set of optimum parameters of the optical potential for the scattering of 〓with nucleus, we found that the 〓 nucleus optical potential need a bigger imaginarypart.
本论文所取得的主要新成果是：独立揭示∧超核和〓超核的不同的收缩效应，其中∧超核的收缩效应被最新实验证实；提出了处理∧∧超核与〓超核混合态的新方法，并发现conversion过程使〓超核能谱和宽度改变；首次在中子星研究中在不包含∑超子的同时考虑新介子〓(975)和φ(1020)，并发现这可使中子星物质的状态方程变软、中子星半径变大、质量变小；独立提取了〓核光学势的一组最佳参数，并证明〓+核光学势要求一个较大的虚部。
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"Either Calvera is an unusual example of a known type of neutron star, or it is some new type of neutron star, the first of its kind," Rutledge said.
拉特利奇说：'卡尔维拉'要么是某种已知中子星的一个特例，要么属于一种全新类型的中子星，而'卡尔维拉'是其中的首例。
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The Crab Nebula is what remains of the supernova of the year 1054, and inasmuch as it has been theorized that neutron stars sometimes remain following supernova explosions, it is beli ...
The Crab Nebula 是1054年超新星留下的残余部分，因为中子星会在超新星爆炸会余留下来的理论已被证实，这来自 Crab Nebula 的 pilsa 就有根有据的被认为是一颗中子星。
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The influence of the temperature to the equation of state of npe neutron matter is not obvious, and the influences to the composition of various particles are mainly in the range of small baryon density.
对npe系统中子星物质的研究表明温度对该类中子星的物态方程影响不大，对粒子所占比例的影响主要表现在低重子密度区域。
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Comparing our result with the observaitonal value, we find out that the double neutron star binaries stand a good chance to be hyperon stars and the neutron stars of X-ray binaries are more like traditional neutron stars.
把计算值同观测结果相比较，发现双中子星更象超子星，X-射线双星中的中子星更象传统中子星。
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We assume the core of neutron stars is a β-stable strange matter consisting of nucleons and hyperons, then the influences of the hyperon-hyperon interaction on the properties of neutron stars are studied in the relativistic mean-field approximation.
我们假定中子星内部物质是由核子与超子混合组成的β稳定的奇异强子物质，在相对论平均场框架内研究了超子超子相互作用对中子星性质的影响。
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Since the atoms that make up normal,"solid" matter are mostly empty space, a star made almost entirely of tightly packed neutrons is extraordinarily dense: a fingernail's worth of a neutron star would have a mass of more than a trillion kilograms. A neutron star's density and gravity is second only to a black hole.
确切的说，是直径20km左右的一个超级中子，虽然不过只有一个大中型城市的体积，质量超过1.5倍太阳——译注）由原子组成的普通物质，其&实心&的物质内部其实绝大部分都是空的（大家完全可以用太阳系质量集中在太阳来想象原子内部，当然电子与行星有本质区别——译注），而一颗几乎全部由中子构成的恒星却密度极大：指甲大的一块中子星物质的质量达到万亿吨级，中子星的密度、引力仅次于黑洞。
- 更多网络解释与中子星相关的网络解释 [注：此内容来源于网络，仅供参考]
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binary star：双子星
1.老年pulsar通常以双子星(binary star)的型态出现,一个星星dumps material到另外一个中子星,造成这个星星再次爆炸,再次变成pulsar (这里有考点,请注意) 第2个第3个理由我忘了 呜呜,我刚考完的时候还记的很清楚
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dynamo：发电机
不然,大范围的磁场用太阳"发电机"(dynamo)模型可以比较好的解释. 与斑竹不同,我对此模型很不乐观. 其主要原因是致密星的内部结构以及物态方程我们目前并不清楚,因此你不能套用主序星的发电机模型. 了解中子星内部超高密物质的特性,
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equation of state：状态方程式
常见的超核子如下异物质(strange matter)等等.建中的日本强子设施 (JHF) 将能产生较高能超核子主要经由介子衰变( Mesonic decay) 很超新星爆炸(supernova explosion) 是天文在天牛星座(Taurus) 可见仍在发光的蟹状星云(Crab Nebula) 即为该次爆炸所形成. 超新星爆炸的产物, 可为中子星(neutron star) 或黑而是重子物质(bary
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neutron star：中子星
作为一位杰出的科幻作家,迄今为止,尼文已经赢得五次世界科幻大奖--雨果奖,这些获奖小说包括:短篇>(Neutron Star)、>(Inconstant Moon)、>(The Hole Man)、>(The Borderland of Sol)以及长篇小说>(R
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neutron star：中子星, Japanese-中性子星
脉冲星pulsar | 中子星, Japanese-中性子星 neutron star | 伴星 companion star
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Neutron star shocks：中子星震盪
紅外線觀測 Infrared observations | 中子星震盪 Neutron star shocks | 流體力學 Fluid dynamics
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Neutron Star Physics：中子星物理
Fundamentals of Positron Annihilation 正电子淹没谱学基础 | Neutron Star Physics 中子星物理 | Interaction Between Pariticles and Solids 粒子与固体相互作用
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ultra dense neutron star：超密中子星
超卖头寸 oversold position | 超密中子星 ultra dense neutron star | 超收的地区 localities that have excess revenues
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accretion by neutron star：中子星吸积
accretion by black hole 黑洞吸积 | accretion by neutron star 中子星吸积 | accretion of bed level 河床的淤高
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that orbit the neutron star Tryxl：他们都围绕中子星区里赛尔
- What's that?|那是什么? | that orbit the neutron star Tryxl.|他们都围绕中子星区里赛尔 | - Ice planets?|冰雪星球?