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。
The phase transition of two-flavor quark matter into strange matter in the interior of a neutron star is studied.
应用新的热力学公式，我们计算奇异夸克物质的态方程，得到十分合理的结。
With the new formulas obtained, we have also calculated the equation of state for strange quark matter with reasonable results.
输运方程给出了胶子物质热平衡化时间短和夸克物质热平衡化时间长的结果。
A short thermalization time for gluon matter and a long thermalization time for quark matter are results of the transport equations.
作为应用，研究了有限化学势下冷密夸克物质系统的色动力学并计算出了色导率。
The theory is then applied for studying the color electric dynamics of cold and dense quark matter at large chemical potential, and color conductivity with non-perturbation effect is obtained.
奇异滴，即质量较小的奇异夸克物质团块，有关它的研究涉及物理学的多个重要分支。
Strangelets are lumps of strange quark matter, in the research of which many important branches of physics are involved.
本文用有效质量口袋模型描述夸克物质研究了流夸克质量的选取对奇异星性质的影响。
In this paper the influence of choice of the current quark mass on the properties of strange stars is studied by using the effective mass bag model to describe quark matter.
本文简要评述了夸克物质(夸克-胶子等离子体)在理论和实验两个方面的研究现状。
Brief status on quark matter (quark-gluon plasma) both in theoretical and in experimental fields are reviewed.
在我们介绍了磁场中夸克物质状态及奇异星的基本结构后，本文主要研究磁场在两个方面对奇异星的效应。
We introduced the state of strange quark matter and the structure of strange star in magnetic field, our paper was focus in the effect of magnetic on strange star in two sides.
利用强子物质的相对论平均场理论和夸克物质的有效质量口袋模型，研究流夸克质量的选取对混合星性质的影响。
The influences of different current quark masses on the properties of hybrid stars were studied via the relativistic mean field theory and the effective mass bag model.
分别基于组夸克质量模型和流夸克质量模型，讨论了超新星核心区两味夸克物质到更稳定的三味夸克物质的相变过程。
Based on constituent quark mass and current quark mass model, the phase transition of two-flavor quark matter to more stable three-flavor quark matter in the core of supernova is studied.
位于布鲁克海文国家实验室的RHIC试验已有明显的证据表明很可能已经产生了夸克-胶子等离子体或者说夸克物质。
There are convincible evidences to prove that QGP or quark matter has been produced in RHIC which lies in BNL.
夸克是这种物质的最基本构造块之一，它被胶子束缚在一起形成亚原子粒子“混合物”，如质子和中子。
One of the fundamental building blocks of matter, called quarks, are bound together by gluons to form 'composite' subatomic particles such as protons and neutrons.
从一些方面看，夸克——胶子物质看上去非常眼熟，和相对论重离子对撞机的理想液体一样，但我们还从中得以发现一些新的东西。
In some respects, the quark-gluon matter looks familiar, still the ideal liquid seen at RHIC, but we're also starting to see glimpses of something new.
大爆炸产生的热量逐个地熔化了原子的核物质，释放出了原子内部的粒子(比如胶子和夸克)。
The heat from the Big Bang literally melted the nuclear matter of atoms, releasing the particles inside (like gluons and quarks).
在这样的温度下，物质被认为处于一种完全不同的，被称为“夸克-胶子等离子态”的状态。
At these temperatures, matter is thought to take on an entirely different state; a state called a "quark-gluon plasma."
科学家们将通过此次实验来研究一种名为夸克-胶子等离子体的物质，它是宇宙大爆炸后极短瞬间形成超高能量密度。
The experiments will allow scientists to study a substance called the quark-gluon plasma, which existed in the fleeting first moments after the Big Bang.
在那段短暂的时间里，大约137.5亿年前，物质并不以我们熟悉的固体、液体以及气体形式存在，而是以一种夸克-胶子汤的形式存在。
At that brief time, some 13.75 billion years ago, matter didn't exist as the solids, liquids, and gasses we are familiar with, but as a kind of quark-gluon soup.
由于他们采用的暗物质模型只能衰退为诸如重夸克这样的特定粒子，并且运行速度平稳，未受温度影响。
That's because they use a model of dark matter that decays into certain types of particles such as heavy quarks and travels at the same speed no matter what the temperature is.
普通正常物质的原子内部只有上、下夸克。而其它夸克是由粒子加速器产生的。
Only the Up and Down quarks are found inside atoms of the normal matter. The other quarks are made in particle accelerators.
结果表明夸克星的质量分布在事件视界以内，即夸克星是黑洞，但构成这种黑洞的物质并没有坍缩到大小为零的一点。
That is , a quark star is a black hole, while the black hole formation has not collapsed to one point yet.
量子色动力学预言在高温高密条件下，有可能发生从强子物质到退紧闭的夸克-胶子等离子体的相变跃迁。
Quantum chromodaynamics predicts that at high temperature and high density a deconfined phase from hadronic matter to quark-gluon plasma will occur.
在此原子核与其组成的质子与中子真的就融化了，而从所有可用的能量之中，创生出更多的夸克、反夸克(夸克的反物质)与胶子。
The nuclei and their constituent protons and neutrons literally melt, and many more quarks, antiquarks (antimatter opposites of the quarks) and gluons are created from all the energy available.
时至今日，量子力学已经把物质分解到“夸克”，用科学从微观上证明了佛祖的智慧是正确的。
For now, the science has explored matters into Quark aspect, proving the correct of the Sakyamuni from micro aspect.
我们这里研究了混合相物质的体粘滞系数，计算了两类非轻子过程(超子和夸克非轻子衰变)对混合相粘滞性的贡献。
Here we study the coefficient of viscosity in mixed phases, calculate the contributions of two kinds of non-leptonic reactions (the non-leptonic decay of hyperons and quarks).
RHIC和LHC上的相对论性重离子实验的一个主要目标就是寻找这种新的物质形态—夸克胶子等离子体。
One of main objects of ultra-relativistic heavy ion collisions experiments at RHIC and LHC is to discover this kind of new state of matter-quark gluon plasma.
如果对撞的能量足够大，就可能制造出一种“夸克——胶子等离子体”，这是在宇宙大爆炸之后的高能环境下存在的一种物质状态。
A "quark-gluon plasma" can be created if the collisions are energetic enough, a state of matter that existed during the high-energy conditions just after the Big Bang .
高能重离子碰撞物理学主要目的是研究极端条件下核物质的性质，探测夸克—胶子等离子体（QGP）。
The major goal of high energy heavy ion collision is to investigate nuclear matter properties under extreme conditions and detect quark-gluon plasma (QGP).
高能重离子碰撞物理学主要目的是研究极端条件下核物质的性质，探测夸克—胶子等离子体（QGP）。
The major goal of high energy heavy ion collision is to investigate nuclear matter properties under extreme conditions and detect quark-gluon plasma (QGP).
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