1) the very early universe
极早期宇宙
1.
After giving the basic description of the very early universe, the author point out that the space-time topology and the inflation are the two most important problems in the research of the very early universe and then do some remarks on the inflation + cold and dark matter model—the most popular cosmological model nowadays.
在对极早期宇宙作了一般性描述的基础上,指出暴涨和时空拓扑是极早期宇宙研究的两大课题并着重评析了现今最流行的暴涨+冷暗物质宇宙模型。
2) early universe
早期宇宙
1.
The number density and energy density of particles with weak interaction in early universe were discussed.
讨论了早期宇宙中具有弱相互作用的粒子的数密度和能量密度的问题,从中看出,化学势是讨论早期宇宙热力学问题所不可缺少的一个重要参量。
2.
According to uniformity in space and constancy in time of the coordinate temperature of an equilibrium system, the space-time duality between Einstein turntable and early universe directly .
考虑到引力场中坐标温度的均恒性 ,爱因斯坦转盘与早期宇宙的时空对偶性直接给出宇宙介质固有温度反比于标度因子R(t)的结
3) early universe nucleon
宇宙早期核子
4) particle of the early universe
宇宙早期粒子
5) cosmological cycle
宇宙周期
1.
This paper analyzes its cosmogony from three aspects:(1)cosmological outspread and vitalism;(2)cosmological cycle and time;(3)God as body and conflagration.
本文对斯多亚学派的宇宙论作了三方面的分析:(1)宇宙扩张论和生机论;(2)宇宙周期论和时间观;(3)“神”作为物体和宇宙大火。
6) cosmogony of Taiji
太极宇宙观
补充资料：宇宙膨胀理论(见大爆炸宇宙学)
宇宙膨胀理论(见大爆炸宇宙学)
theory of universal expansion
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说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条