cold dark matter

基本解释

Researchers created a new supercomputer model, based on observational data and the "Lambda Cold Dark Matter" theory of the universe.
研究人员在观测数据和兰姆达冷暗物质模型的基础上构建了一个新的计算模型。
It's the presence of cold dark matter that explains how the young universe went from being smooth to being lumpy, as ordinary matter coalesced first into stars and then into galaxies.
正是这种冷暗物质的存在解释了早期宇宙如何从平滑的初始状态（小尺度结构）演变成块状非均匀的大尺度结构，从而使普通物质结合，首先形成恒星，然后再构成星系。
The CDM theory makes no predictions about exactly what the cold dark matter particles are, and one large weakness in the cold dark matter theory is that it is unclear what the dark matter consists of.
CDM理论不做预言关于确切地什麽冷的神秘的物质微粒是，并且一个大弱点在冷的神秘的物质理论上是它是不明的什麽神秘的物质包括。