Strange quark
- 网络奇异夸克;奇夸克
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Bulk Viscosity of Strange Quark Matter in High Temperature Approximation
高温近似下奇异夸克物质的体粘滞系数
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The Study of Dynamics of Strange Quark Matter and Properties of Strange Stars
奇异夸克物质动力学与奇异星性质研究
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Strange Quark Matter and Strange Star in Magnetic Field
磁场中的奇异夸克物质与奇异星
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Charge Dependence of the Critical Density of Strange Quark Matter in a New Mass Scaling
新的质量标度下奇异夸克物质的电荷与临界密度
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Baryon Wave Functions of the System With Strange Quark
具有奇异夸克系统的重子波函数
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Strange quark matter at finite temperature
有限温度奇异夸克物质
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On the Properties of Strange Quark Matter
关于奇异夸克物质的性质
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Bulk Viscosity of Strange Quark Matter at First-Order Perturbative QCD Approximation
一级微扰QCD耦合的夸克物质体粘滞系数
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The Neutrino Emissivity of Urca Process of Strange Quark Matter in Weak and Ultra Strong Magnetic Field
弱磁场及甚强磁场下奇异夸克物质Urca过程的中微子能量损失率
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Reduction of Strange Quark Suppression in Relativistic Nucleus-Nucleus Collisions
相对论性核-核碰撞中奇异夸克压低的约化
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The situation becomes more complicated in moderate density because of the strange quark mass , β equilibrium and the charge neutrality conditions .
在中等密度下,由于奇异夸克质量,β平衡,荷中性条件等影响情况变得非常复杂。
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Strangelets are lumps of strange quark matter , in the research of which many important branches of physics are involved .
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。
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The bulk viscosity of the strange quark matter is the effective energy damping mechanism and the pivotal parameter determining the r-mode window .
奇异夸克物质的体粘滞是耗散能量的有效机制,它是决定r-模窗口的关键参数之一。
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Taking medium effects into account , we calculate the bulk viscosity of strange quark matter in high temperature approximation using a consistent thermodynamics method in quasi particle description .
在准粒子描述下,采用自洽的热力学方法,考虑奇异夸克物质(SQM)的介质效应,计算了高温近似下奇异夸克物质的体粘滞系数。
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In this article , we describe the dynamic of the strange quark matter concentrating on the existing models including medium effects : density dependent model , chemical potential dependent model and temperature dependent model .
在本论文中,我们描述了奇异夸克物质的动力学。集中讨论了现有的包含介质效应的模型:密度依赖模型,化学势依赖模型以及温度依赖模型。
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Especially in recent years , people pay more attention to the bulk viscosity of strange quark and neutron matter after the finding of important r-mode instability in rotating compact stars .
特别是最近几年,由于发现旋转致密星存在重要的r-模不稳定性,奇异夸克物质和中子物质体粘滞性的巨大差异受到了更大的重视。
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The development of the high energy nuclear physics and high-energy heavy-ion collision experiments indicate the exist of quark matter and the importance of the neutron star model containing strange quark matter .
随着地面高能核物理的发展,高能重离子碰撞实验也预示夸克物质的存在,含有奇异夸克物质的中子星理论模型研究显得日益重要。
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Because the transition temperature of the nonzero ms strange quark paring is re-duced , phase diagram with respect to temperature and magnetic field contains a region where only u and d flavors condensate .
由于具有非零质量的奇异夸克配对的转变温度降低,关于温度和磁场强度的相图包含了一个只有u,d夸克配对的区域。
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The equation of states turns out to be " softened " when applying the above thermodynamics to strange quark matter in strange stars , and this is consistent with the results of the mass chemical potential dependent model .
利用这一等效热力学讨论奇异夸克物质的物态方程及声速,得到了一个软化的物态,这与质量-密度相关模型是一致的。
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In the study of strange particles production at the RHIC and LHC energies , considering the reduction mechanism of strange quark suppression can well explain experimental phenomena .
在研究RHIC及LHC能区奇异粒子时,考虑奇异夸克压低减弱机制能很好的解释实验现象。