宇宙的假真空合成如何设定初始条件，允许每哈勃体积每哈勃时间的成核率变化的开始
How false vacuum synthesis of a universe sets initial conditions which permit the onset of variations of a nucleation rate per Hubble volume per Hubble time
摘要：
利用博戈米尔尼不等式和拓扑荷在新宇宙未成核时的消失，可以更简单、更直接地洞察拓扑缺陷（扭结和反扭结）如何在暴胀宇宙学开始时对初始条件做出贡献。目前，在宇宙膨胀的初始条件和新宇宙的成核之间几乎没有桥梁。这个演示展示了如何做到这一点，同时仍然采用Venezianos处方形成量子之间的联系的长度，大小的一个量子场和力的引力和规范一样。
英文摘要：
Using Bogomil'nyi inequality and the vanishing of topological charge at the unset of nucleation of a new universe permits a simpler,more direct insight into how topological defects (kinks and anti kinks) contribute to initial conditions at the onset of inflationary cosmology. Currently, there are few bridges between initial conditions for cosmological inflation and the nucleation of a new universe. This presentation shows how this can be done while still employing Venezianos prescription for forming a link between quanta of length, the magnitude of a dilaton field and forces gravitational and gauge alike.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
