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QCD vacuum: nuclear forces, nucleons, pions ...

机译:QCD真空:核动力,核磁,核心......

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This contribution contains six sections, namely:1. from QCD to chiral perturbation theory - QCD is widely accepted as the theory of strong interactions, but direct applications to low-energy hadronic processes are difficult. In this regime, the light quarks u and d prevail, and one can employ a rigorously equivalent effective theory, known a chiral perturbation theory, based on hadronic degrees of freedom. 2. strong vacuum and the pion - Chiral symmetry is not exact in the real world. Nevertheless, the absence of of parity multiplets and the smallness of the pion mass suggest that it is a good approximate symmetry, realized in the Nambu-Goldstone mode. Its ground state, the vacuum, is filled with a condensate, made of quark-antiquark pairs. In sections 1-3, instances are presented of observables strongly influenced by the QCD vacuum. 3. nuclear forces - In the last few years, chiral perturbation theory has produced a very reliable picture of both two- and three-nucleon forces. In particular, the important isospin independent central potential V~+_C is well understood and known to be dominated by the scalar form factor of the nucleon, a function that describes the disturbance it produces over the vacuum. 4. nucleon scalar form factor - The spatial integration of the nucleon scalar form factor gives rise to aN, the nucleon a-term. The value of this quantity can be extracted from experiment and the empirical value accepted presently is 45±8 MeV. A simple model, based on the idea that the pion cloud of the nucleon is constructed at the expenses of the surrounding condensate, produces a aN in the range 43-49 MeV, with no free parameters. 5. scalar radius of the pion - The value of this radius can be extracted from pion-pion scattering data and the most reliable estimate is ( r~2 )s~T = 0.61 ± 0.04 fm~2. The extension of the model described in section 4 to the pion gives rise to a picture in which it is embedded into the condensate. As one moves towards its center, the condensate is gradually replaced by a mesonic cloud. When this process is completed, a phase transition occurs, at a distance R 0.6 fm. A version of the model, including scalar resonances, yields (r~2)s~x = 0.59 fm~2. 6. conclusion - The QCD vacuum is an active component of low-energy hadronic processes, essential to a consistent description of Nuclear Physics.
机译:此贡献包含六个部分,即:1。从QCD到手性扰动理论 - QCD被广泛接受作为强互动理论,但直接应用到低能量的辐射过程很难。在这一制度中,光夸克U和D占优势,并且可以采用严格的等效有效理论,以基于Hadronic自由度的手性扰动理论。 2.强大的真空和磁线 - 手性对称在现实世界中并不是精确的。然而,没有奇偶校验的差分和π粒子的小,表明它是一种良好的近似对称性,在Nambu-Goldstone模式中实现。它的基因态,真空填充有克克古克配对的冷凝物。在第1-3节中,介绍了受QCD真空强烈影响的可观察者的实例。 3.核动力 - 在过去的几年里,手性扰动理论已经产生了两个和三核力的非常可靠的画面。特别地,重要的索坦独立的中心电位V〜+ _c被很好地理解并且已知通过核子的标量形式来支配,该功能描述了它在真空上产生的干扰。 4.核子标量形因素 - 核子标量子因子的空间整合导致核心A期。可以从实验中提取该数量的值,目前接受的经验值为45±8 MeV。一种简单的模型,基于核子的孔膜在周围冷凝物的费用中构建的思想,产生43-49meV的范围,没有游离参数。 5.标量的磁线半径 - 可以从磁链散射数据中提取该半径的值,最可靠的估计是(R〜2)S〜T = 0.61±0.04 fm〜2。第4节中描述的模型的延伸导致嵌入冷凝物中的图像。随着朝向其中心的移动,凝结物逐渐被设计云逐渐取代。完成此过程后,发生相位转换,在距离R 0.6 FM时发生。模型的版本,包括标量谐振,产量(R〜2)S〜x = 0.59 fm〜2。 6.结论 - QCD真空是低能量辐射过程的活性成分,对于核物理学的一致描述至关重要。

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