利用di夸克对作为获得新宇宙成核开始附近暗物质的一种方法
Using di quark pairs as a way to obtain dark matter near the beginning of nucleation of a new universe
摘要：
利用博戈莫尼不等式和拓扑荷在新宇宙成核开始时的消失，可以更简单、更直接地了解拓扑缺陷（扭结和反扭结）如何在暴胀宇宙学开始时对初始条件的产生产生贡献。我们发现，这是可能的，目前的暴胀宇宙学的初始条件与双夸克对形成的轴子壁作为一种方式开始形成的双夸克作为孤子反解型对。这允许向暴胀宇宙学的转变，与物质的初始成核状态一致，该状态在一开始就具有显着的暗物质成分。双夸克对成分之间的分离可能是由于物质创生初始阶段的CP破坏，并且可能是暴胀膨胀的便利触发器。
英文摘要：
Using the Bogomolnyi inequality and the vanishing of topological charge at the onset of nucleation of a new universe permits a simpler, more direct of how topological defects(kinks and anti kinks) contribute to the onset of initial conditions at the beginning of inflationary cosmology. We find that it is possible to present inflationary cosmology with initial conditions with di-quark pairs formed using an axion wall as a way to start formation of di quarks as soliton-anti soltion type pairs. This allows for a transition to inflationary cosmology congruent with with an initial nucleation state of matter which would have a significant dark matter componet in the beginning. The separation between the di-quark pairs constituents would be due to CP violations in the initial phases of matter creation and would be a convenient trigger for inflationary expansion.
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