Cosmology: What one needs to know

被引:0
作者
Albright, JR [1 ]
机构
[1] Purdue Univ Calumet, Dept Chem & Phys, Hammond, IN 46323 USA
来源
ZYGON | 2000年 / 35卷 / 01期
关键词
age of the earth; age of the universe; anthropic principles; Big Bang; Big Crunch; closed; flat and open universes; cosmology; dark matter; galaxy; general relativity; Hubble expansion; inflation; Local Group; microwave background radiation; Milky Way; quantum mechanics; standard cosmological model; universe; Virgo Supercluster;
D O I
10.1111/0591-2385.00267
中图分类号
D58 [社会生活与社会问题]; C913 [社会生活与社会问题];
学科分类号
摘要
Cosmology the study of the universe, has a past, which is reviewed here. The standard model-the Big Bang, or the hot, dense early universe that is still expanding-is based on observations that are basically consistent but which require additional input to improve the agreement. Out of the early universe came the galaxies and stars that shine today The future of the universe depends on the density of matter: too much mass leads to the Big Crunch; too little leads to eternal expansion and cooling. The dark-matter problem prevents us from knowing which will be the fate of the universe. The limits of what may be called "scientific" are addressed.
引用
收藏
页码:173 / 180
页数:8
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