Color confinement, dark matter and the missing of anti-matter

P. Wang
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Abstract

QCD is the fundamental theory to describe the strong interaction, where quarks and gluons have the color degrees of freedom. However, a single quark or gluon can not be separated out and all observable particles are color singlet states. Color confinement or quark confinement conjecture can be proved by considering not only the strong interaction but also the electroweak interaction which is $SU(3)_c$ invariant. Any measurable state has to be color singlet is the direct consequence of the common symmetry of the standard model. Color non-singlet objects are created from the big bang when the interaction breaks $SU(3)_c$ symmetry based on the nonlocal Lagrangian. There is nearly no interaction between colored objects and color singlet universe when the momentum transfer is not large enough. Colored objects are reasonable candidates of dark matter and the missing of anti-matter in the universe can also be easily explained. Dark matter can be produced in the laboratory which can be tested by measuring the energy loss and baryon number change in the extremely high energy collisions of particles and anti-particles.
色约束,暗物质和反物质的缺失
QCD是描述强相互作用的基本理论,其中夸克和胶子具有颜色自由度。然而,单个夸克或胶子不能分离出来,所有可观测的粒子都是彩色单重态。颜色约束或夸克约束猜想可以通过考虑强相互作用和$SU(3)_c$不变的电弱相互作用来证明。任何可测态都必须是彩色单线态,这是标准模型的共同对称性的直接结果。当相互作用打破基于非局部拉格朗日的$SU(3)_c$对称性时,从大爆炸中产生彩色非单线态物体。当动量传递不够大时,有色物体与彩色单重态宇宙之间几乎不存在相互作用。有色物体是暗物质的合理候选者,宇宙中反物质的缺失也很容易解释。暗物质可以在实验室中产生,可以通过测量粒子和反粒子在极高能量碰撞中的能量损失和重子数变化来测试。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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