首先叙述了弱相互作用的数学模型。
The mathematical model of the weak interaction is described at first.
卤键是一种类似氢键的分子间弱相互作用。
Halogen bond is known as a kind of non - covalent intermolecular interaction.
卤键是一种类似氢键的分子间弱相互作用。
Halogen bond is known as a kind of non-covalent intermolecular interaction.
涉及中微子的相互作用介导的弱相互作用。
Interactions involving neutrinos are mediated by the weak interaction.
卤键是一种类似氢键的分子间弱相互作用。
The interaction energies of the halogen-bonded complexes were calculated.
得到的笼形包合物中存在不同的弱相互作用。
There exist different weak interactions in the clathrate complexation.
假定奇异性是除弱相互作用以外的所有相互作用中的一个守恒量。
Strangeness is assumed to be a conserved quantity in all interactions that are not weak.
二者之存在弱相互作用，这一作用将配合物联接成一维链状结构。
The complexes was linked by this interaction to form one-dimensional structure.
将这一理论应用到更多的弱相互作用现象的研究中去是有意义的。
It is shown, other conbinations of Fermi interactions can not give result in agreement with experiment.
在夸克的弱相互作用基下，得到了下夸克质量矩阵的唯象约束条件。
The phenomenological constraints on the down-quark mass matrix in the weak interaction base were investigated.
有限能量电弱磁单极子在电弱相互作用唯象论中有重要的实际应用。
Finite energy electroweak monopoles have important physical applications in the phenomenology of electroweak interaction.
本文提出了SU(6)对称性理论中的一个弱相互作用中间玻色子方案。
An intermediate boson scheme of weak interactions is proposed within the framework of the SU (6) symmetry theory.
在1957年，我们中的3,4个人提出了一个还算完整的弱相互作用理论。
Three or four of us, in 1957, put forward a partially complete theory of one of these forces, this weak force.
并利用荧光光谱和核磁共振波谱法研究了芳香性氨基酸与ATP的弱相互作用。
The non-covalent interactions between ATP and Phe or Trp were also investigated by fluorescence spectrometry and NMR.
根据弱相互作用理论，本文建立了损耗大气中极性重力波的非线性相互作用方程。
A set of the interaction equations of inertial gravity waves in a dissipative atmosphere on the basis of the weak nonlinear theory is derived.
新材料是超分子聚合物，由金属间弱相互作用力将小分子聚合而成，就如同一种分子尼龙扣的结合。
It's a supramolecular polymer, made of smaller molecules held together by weak interactions with metals, which act like a kind of molecular Velcro.
事实上，这些胆小鬼(弱相互作用大质量粒子)不与自己在同一交互方式“正常”的事一样。
In fact, these WIMPs (Weakly Interacting Massive Particles) do not interact with themselves in the same way that "normal" matter does.
应用数值计算的方法计算了谐振势阱中有弱相互作用的玻色气体凝聚的临界温度和基态占据率。
The critical temperature and the ground state fraction of weakly interacting Bose Einstein condensation in a harmonic potential trap are calculated with numerical method.
当两个大质量弱相互作用粒子碰撞时，它们会彼此消灭，从而产生另一些粒子——比如正电子。
When two WIMPs collide, they can annihilate each other, giving rise to other particles—such as positrons. The data from AMS so far match these predictions.
射线分析显示化合物1和2的晶体结构均由分子间氢键和-弱相互作用堆积而成的二维层状结构。
The X-ray analysis reveals that the crystal structures of compounds 1 and 2 are two-dimensional layer structures through intramolecular hydrogen bonding and -? stacking.
科学早就通过测量、观察和实验告诉我们宇宙中有四种力：电磁力、强相互作用力、弱相互作用力和万有引力。
Science has shown us through measurement, observation and experimentation that there are four forces in the Universe: electromagnetism, strong interaction, weak interaction and gravitation.
杨振宁和李政道因为在弱相互作用下宇称不守恒原理方面的工作获得了1957年的诺贝尔物理学奖。
Yang received the 1957 Nobel Prize in Physics together with Tsung-dao Lee, for their work on parity non-conservation of weak interaction.
众所周知，在自然界中有四种基本的相互作用力：电磁力、强相互作用力、弱相互作用力和万有引力。
Well, as you all know, there are four fundamental forces in physics: electromagnetism, strong nuclear interaction, weak nuclear interaction and gravity.
一旦承认有可能存在性质超越标准弱相互作用重粒子的粒子，人们自然而然会联想还有没有其它可能。
Once one admits the possibility of hidden particles with properties that go beyond the standard WIMP scenario, it is natural to consider the full range of possibilities.
幻灯片出现：在1957年，我们中有人提出一个还算完整的弱相互作用理论，但是却与7个实验事实矛盾。
Slide - "in 1957 some of us put forward a partially complete theory of the weak force, in disagreement with the results of seven experiments."
超分子化学的研究范围是由两个或更多的化学实体通过分子间弱相互作用而构建的高度有序及复杂性的体系。
The study field of supramolecular chemistry is high-order and complicated system constituted from two or more moleculars through weak interaction between different molecules.
有证据表明宇宙中锂元素的含量比预计要少，所以假设的超级弱相互作用重粒子可以作为一种方法解释这种差异。
There is some evidence that the universe has less lithium than expected, and the super-WIMP hypothesis is one way to explain the discrepancy.
科学家们相信是弱相互作用粒子(WIMPS)构成了暗物质，在地球上进行的深地下实验正试图直接探测到这种粒子。
Deep underground experiments on Earth have attempted to directly detect the weakly interacting particles (WIMPS) that scientists believe constitute dark matter.
WIMP即大质量弱相互作用粒子，是暗物质理论最主要的候选者。WIMP产生于大爆炸中，自产生后一直聚集、散开形成星系。
The leading candidate is a WIMP, or weakly-interacting massive particle, that was produced in the big bang and has been clumping up and seeding structures such as galaxies ever since.
WIMP即大质量弱相互作用粒子，是暗物质理论最主要的候选者。WIMP产生于大爆炸中，自产生后一直聚集、散开形成星系。
The leading candidate is a WIMP, or weakly-interacting massive particle, that was produced in the big bang and has been clumping up and seeding structures such as galaxies ever since.
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