用Cardy-Jacobsen和Yaffe-Svetitsky猜想解决宇宙学畴壁和暗物质过剩问题
Using Cardy-Jacobsen and Yaffe-Svetitsky Conjectures to Solve the Cosmological Domain Wall and Dark Matter Overproduction Problems
摘要：
在本文中，我将结合和使用两个Cardy-Jacobsen和Yaffe-Svetitsky结构\cite{c.1,c.2}，提出了一个机制，后期的电弱对称性破缺期间，由于离散$Z_3$对称性在$\textit{O} (10)^2$ GeV和一个psudo膨胀在$\textit{O}(10)^2$ MeV的尺度，以解决宇宙畴壁问题，以及在早期宇宙中的热和非热遗迹过剩生产。我们将看到Cardy-Jacobsen猜想和Zel'dovic关于宇宙学畴壁问题的陈述是不相容的。此外，在这里提出的伪膨胀机制将有一个潜热释放和熵注入没有指数膨胀和再加热期。
英文摘要：
In this paper I will combine and use two Cardy-Jacobsen and Yaffe-Svetitsky conjectures \cite{c.1,c.2} to present a mechanism for a late-time inflation during the electroweak symmetry breaking due to discrete $Z_3$ symmetry at $\textit{O} (10)^2$ GeV and a psudo-inflation at $\textit{O}(10)^2$ MeV scale in order to solve the cosmological domain wall problem as well as thermal and non-thermal relics overproduction in the early universe. We will see that Cardy-Jacobsen conjecture and Zel'dovic statement for cosmological domain wall problem are incompatible. Also, in the psudo-inflation mechanism presented here there would be a latent heat release and entropy injection without an exponential expansion and reheating period.
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。
