论文标题
暗物质理论
A theory of the dark matter
论文作者
论文摘要
在较早的论文中，我提出了一个高度对称的半古典初始条件，以描述在电动发电机过渡之前的时期中的宇宙，并在此之后完全确定所有宇宙学。除了假定标准模型之外，没有什么。不需要通货膨胀。初始对称性不允许可调参数。它是标准模型宇宙学时期的完整理论，可预测性和可伪造。在这里，初始条件的时间演变是在经典近似中计算的。具有非平凡经典值的字段是SU（2）-Weak仪表场（宇宙学量规场或CGF）和HIGGS字段。 CGF会产生电动型转变，然后以非偏见的完美流体（$ W _ {\ Mathrm {cgf}}} \ 0 $）演变。目前，即当$ h = h_ {0} $时，CGF能量密度满足$ω__λ+ω_ {\ Mathrm {cgf}} = 1 $。 CGF是暗物质。暗物质是标准模型的经典现象。阶级宇宙仅包含暗物质，没有普通的物质。在领先顺序的旁边，标准模型字段的波动将提供可计算的，相对较少的普通物质，以便$ω_λ+ω_ {\ mathrm {cgf}}}}+ω_ {\ Mathrm {\ Mathrm {}}} = 1 $。
In an earlier paper I proposed a highly symmetric semi-classical initial condition to describe the universe in the period leading up to the electroweak transition and completely determine all cosmology after that. Nothing beyond the Standard Model is assumed. Inflation is not needed. The initial symmetry allows no adjustable parameters. It is a complete theory of the Standard Model cosmological epoch, predictive and falsifiable. Here, the time evolution of the initial condition is calculated in the classical approximation. The fields with nontrivial classical values are the SU(2)-weak gauge field (the cosmological gauge field or CGF) and the Higgs field. The CGF produces the electroweak transition then evolves as a non-relativistic perfect fluid ($w_{\mathrm{CGF}}\approx 0$). At the present time, i.e. when $H=H_{0}$, the CGF energy density satisfies $Ω_Λ+Ω_{\mathrm{CGF}}=1$. The CGF is the dark matter. The dark matter is a classical phenomenon of the Standard Model. The classsical universe contains only the dark matter, no ordinary matter. At next to leading order the fluctuations of the Standard Model fields will provide a calculable, relatively small amount of ordinary matter such that $Ω_Λ+Ω_{\mathrm{CGF}}+Ω_{\mathrm{ordinary}}=1$.
