baryon

The possible appearance of the R-parity violating ( RPV) couplings, which will violate the lepton and baryon number conservation, has gained full attention in searching for the SUSY.

在寻找超对称时，可能存在的破坏轻子数和重子数的R宇称破缺耦合受到了充分关注。

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One method looks for the effects of sound waves which originated in the Big Bang: baryon-acoustic oscillations ( Bao).

其中一种方法在寻找起源于宇宙大爆炸的音波效应：重子声学振荡（bao）。

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Lattice QCD calculations predict a phase transition from hadronic matter to a de-confined, locally thermalized Quark-Gluon Plasma ( QGP) state at high temperature and small baryon density.

格点量子色动力学预言，在高温高密的条件下有可能发生从强子相到退禁闭的局域热化的夸克胶子等离子体（QGP）相的跃迁。

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The baryon magnetic moments are studied by using a relativistic potential model.

采用相对论性势模型讨论了重子磁矩.

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Within the Naive Quark Model, hadrons are composed of qq ( for meson) or qqq ( for baryon).

在朴素夸克模型中，强子具有qq（介子）和qqq（重子）构成。

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The baryon numbers are absolutely conserved in the Standard Model.

在标准模型中重子数是绝对守恒的。

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An Analysis of Quark Effect in Two Baryon System

两重子体系夸克效应的分析

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a stable, positively charged subatomic particle in the baryon family having a mass1, 836 times that of the electron.

质子重子族群中一种稳定的带正电的中子核，质量为电子的1,836倍。

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It is studied Baryon excited states for quark confinement and chiral symmetry breaking.

研究了夸克约束的重子受激态和手征对称破缺.

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In the second part, the calculations show that baryon chemical potential HB and strangeness chemical potential// sare monotonous function of net baryon density.

在第二部分中，计算结果表明重子化学势μB和奇异子化学势μS是净重子密度的单调变化函数。

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The observed baryon-to-photon ratio of 10-9 could be produced by the decays of superheavy bosons in the very early universe if C and CP are violated in its actions.

目前观测到的重子光子数比10~（-9）可能是由极早期宇宙中的超重玻色子的衰变产生的，在这种衰变中C及CP是破坏的。

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The chemical potential of baryon is larger than that of strangeness, and they all go to zero at low side of values.

重子化学势比奇异子化学势大，在低端它们都一致趋于零。

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The important character of increment of the baryon multiplicity in Υ→ 3g fragmentation is interpreted naturally without any other assumptions.

不需引入任何其它假定，就自然解释了Υ→3g三胶子碎裂末态重子多重数增高的重要特征。

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The effective intermediate range interaction in baryon spectroscopy and its effect on N-N interaction

重子谱中的中程相互作用及其对N-N核力的影响

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We constrain these three models by using the type la supernovae, the cosmic microwave background, and the baryon acoustic oscillations data, then compare them utilizing the Bayesian evidence.

我们用Ia型超新星、宇宙微波背景和重子声学振荡的数据，对这三种模型进行了限制，并以Bayesian判据为标准，对它们进行了比较。

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