neutron matter的例句大全

It is Shown that the periodic structure of the Condensate field leads to a periodic modulation of the density and spin in a neutron matter.

结果表明凝聚场的周期结构将使中子物质的密度与自旋受到周期的调制。

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pf superfluidity in neutron matter and the effect of microscopic three-body force

态超流性和微观三体核力效应

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gamma ray bursts: phase transition from neutron matter to quark-gluon plasma

射线暴：从中子物质到夸克胶子等离子体的相变

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Self-energy Dispersion Effects on Neutron Matter Superfluidity

中子物质中超流性的自能色散效应

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Equation of State of Neutron Star Matter in Uniform Strong Magnetic Fields

均匀强磁场中中子星物质的物态方程

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Study on Mass and Radius of Neutron Star Using Asymmetry Equation of State of Nuclear Matter

利用非对称核物质状态方程对中子星的质量和半径的研究

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Effect of σ~,Φ Mesons on the Neutron Star Matter at Finite Temperature

σ~和φ介子对有限温度中子星物质的影响

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An equation of state of high-dense matter and the structure of neutron star

高密物质的一种状态方程和中子星的结构

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The Influence of π~-Meson Condensation on Neutron Star Matter

π介子凝聚对中子星物质的影响

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The Vibration Damping Effect of Quark Matter in the Interior of Neutron Stars

中子星内部夸克物质的振动阻尼效应

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preliminary study of airborne particulate matter in a beijing sampling station by instrumental neutron activation analysis

用中子活化分析仪对北京一取样站的空气颗粒物的初步研究

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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。

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description of the nuclear matter and neutron star in relativistic mean field theory with density-dependent interactions

密度相关的相对论平均场理论对核物质和中子星的描述

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description of nuclear matter and neutron stars in density-dependent relativistic mean field theory

利用密度相关的相对论平均场理论对核物质与中子星的研究

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Kaon Condensation in Neutron Star Matter and Nuclear Three-Body Force Effect

中子星物质中的K介子凝聚与三体核力效应

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The collapse of a star may produce a White Dwarf or a neutron star& a star, whose matter is so dense that it continually shrinks by the force of its own gravity.

一颗超新星的崩溃可能会产生白矮星或中子星，其物资的密度非常大以至于在其自身重力的作用下持续收缩。

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The EOS of asymmetric nuclear matter is crucial for understanding many astrophysical problems and phenomena related to the global properties of neutron stars, supernova explosion and neutron star cooling.

非对称核物质的状态方程在理解中子星的整体性质，超新星的爆发、中子星的冷却等许多天体物理的现象中起着决定性的作用。

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