相对论的

Study of X-rays from accreting black holes will enable us to learn the nature of the accretion physics and test the theory of general relativity eventually.

黑洞吸积与辐射是天体物理中的热点问题，通过对黑洞X射线辐射的研究，人们可以了解吸积的物理过程并最终认证广义相对论。

Any mention of sin grates against today's relativistic values and the kind of "freedom" where anything goes.

任何提及仙箅子对今日的相对论和价值观的那种&自由&而东西的。

Physics a wave that is hypothesized to propagate gravity and to travel at the speed of light.

被广义相对论所预言的、以光的速度传播重力的波。

Marked the birth of the theory of relativity, is that in 1905 when the 26-year-old Einstein published "On the electrodynamics of moving."

相对论诞生的标志，是1905年即爱因斯坦26岁时发表的《论动体的电动力学》。

Under the framework of constituent quark model, according to the effective degrees of freedom used, we have the Glashow-Isgur model , the spontaneous chiral symmetry breaking model, the hybrid model and so on.All of these models are successful to describe the properties of the mesons and baryons.

组分夸克模型是一种非相对论模型，根据所采用的有效自由度的不同，组分夸克模型又可以分为好几种具体的模型，主要有：Glashow-Isgur模型、手征对称自发破缺模型和&杂化&模型等。

The influences of hyperon coupling constant on the properties of neutron star were studied by making use of -GL85 parameter set in the framework of the relativistic mean field theory and taking, freedoms of hyperons into consideration.

采用相对论平均场理论下的GL85参数组，在考虑超子Λ，Σ(上标+，Σ^0，Σ，Ξ^0，Ξ自由度下，研究超子耦合常数的选取对中子星内粒子数密度分布、状态方程及质量－半径关系的影响。

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。

The various effective interactions'(including DDME1,TW99,NL2,TM1,TM2,GL85 and GL97) influence on the constitute, equation of state and mass of neutron star are studied in the framework of relativistic mean field theory considering the interacting nucleons, hyperons and mesons system at finite temperature (T=20 MeV).

从相对论平均场（Relativistic Mean Field，RMF）理论出发，考虑核子、超子和介子的相互作用，研究了一定温度（T=20 MeV）下，各种不同相互作用参数组（DDME1、TW99、NL2、TM1、TM2、GL85和GL97）对中子星物质的粒子组成、状态方程和质量等的影响。

Based on the principle of special relativity, the formula of "Light Pressure" and the equation of movement of the object propelled by photon propulsion under the condition of movimg object are deduced.

利用狭义相对论推导了物体运动情形下的光压公式和光子推进下物体的运动方程，分析了光子推进过程中的能量转换关系。

Moreover, the first-quantized theory of photons is established, and a quantum-mechanical equation of photons inside a waveguide is presented, these are important for us to study photons locality in three dimensional spaces.

其中给出了光子的一次量子化理论，建立了波导内光子的相对论量子力学方程，这些研究对于光子的空间局域性理论研究有着重要意义。

As she looked at Warrington's manly face, and dark, melancholy eyes, she had settled in her mind that he must have been the victim of an unhappy attachment.

每逢看到沃林顿那刚毅的脸，那乌黑、忧郁的眼睛，她便会相信，他一定作过不幸的爱情的受害者。

Maybe they'll disappear into a pothole.

也许他们将在壶穴里消失