cold dark matter

基本解釋

Researchers created a new supercomputer model, based on observational data and the "Lambda Cold Dark Matter" theory of the universe.
研究人員在觀測數(shù)據(jù)和蘭姆達冷暗物質(zhì)模型的基礎(chǔ)上構(gòu)建了一個新的計算模型。
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.
正是這種冷暗物質(zhì)的存在解釋了早期宇宙如何從平滑的初始狀態(tài)（小尺度結(jié)構(gòu)）演變成塊狀非均勻的大尺度結(jié)構(gòu)，從而使普通物質(zhì)結(jié)合，首先形成恒星，然后再構(gòu)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理論不做預(yù)言關(guān)于確切地什麼冷的神秘的物質(zhì)微粒是，并且一個大弱點在冷的神秘的物質(zhì)理論上是它是不明的什麼神秘的物質(zhì)包括。