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1.cosmic abundance of elements
元素宇宙丰度收藏指正
2.Based on cosmic elemental abundance and the physics of nuclear synthesis, Gamow, Alpher and Herman boldly conceived the physical framework scenario for a Big Bang Universe during 1940s to 1950s.
基于宇宙元素丰度和核合成物理,Gamow,Alpher和Herman于1940-1950年大胆设想了宇宙“大爆炸”的物理框架图像.收藏指正
3.The article discusses Some main observed facts of the model of big-bang cosmology by the releuant theories of modern physics,for example Hubble law cosmic microwave background radiation helium abundance and so on,make an attempt on preliminary des- cribing for observed facts to theories for the model of big-bang cosmology.
本文用近代物理学有关理论讨论了大爆炸宇宙学模型的一些主要观测事实,如哈勃定律、宇宙微波背景辐射、氦的丰度等问题,尝试对大爆炸宇宙学模型从观测事实到理论作一个初步地描述.收藏指正
4.The observational cosmology and its recent progress are reviewed, including observational methods, Hubble constant, Hubble time, dark matter, dark energy, cosmic background radiation, large-scale structure, element abundance and active galactic nucleus, neutrino, gamma-ray bursts etc. . In addition, the problems and challenges are discussed as well as the perspective to the observational cosmology.
系统介绍了观测宇宙学和其最新进展,包括观测手段和哈勃常数和宇宙的年龄、宇宙的暗物质、暗能量、背景辐射、大尺度结构、元素丰度、活动星系核、中微子、γ暴等热点问题,并提出了观测宇宙学存在的问题和挑战.收藏指正
5.To the great scale of the universe age, 187 Re- 187 Os isotopic pair, which have very long half life, was used as a cosmic nuclear clock of cosmochronometr. It is a typical relationship between modern astronomy and nuclear physics. The neutral isotope abundance ratio of 187 Re over daughter nucleus 187 Os in common growth mineral can be used as the clock to measure the time.
以很长半衰期 ( 4 2× 1 0 9a)的 β-衰变的 187Re- 187Os核对作为大尺度的宇宙核钟来量度宇宙的年纪 ,是近代天文学与核物理学相结合的又一典范 .收藏指正
6.The plastic nuclear track detector CR-39 is exposed for about 10 hours in balloon observation in 1982.The relative abundance (E>3.6 GeV/n) of the galactic cosmic rays is obtained and compared the result with the satellite data.
在1982年的气球飞行中,球载塑料核径迹探测器CR-39在气球高度飞行了10小时. 测得E>3.6 GeV/n的银河宇宙线相对丰度,结果与卫星探测数据基本一致.收藏指正
7.The big bang model, which states that almost 14 billion years ago the universe started expanding from a state of extremely high density and temperature, is able to explain galaxy motions, the abundance of hydrogen and helium, and the properties of the cosmic microwave background (CMB), the remnant heat from the expanding and cooling gas.
大霹雳模型指出,宇宙于约140亿年前自极度高温、高密度的状态开始扩张,这理论不但可以解释星系运动以及宇宙中氢与氦的含量,而且还预测了宇宙扩张时,冷却中气体的残馀热辐射,也就是「宇宙微波背景」的各项性质。收藏指正
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