The origin of helium and the other light elements

被引:29
作者
Burbidge, G
Hoyle, F
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
关键词
cosmic microwave background; early universe; nuclear reactions; nucleosynthesis; abundances;
D O I
10.1086/311756
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The energy released in the synthesis of cosmic He-4 from hydrogen is almost exactly equal to the energy contained in the cosmic microwave background radiation. This result strongly suggests that the He-4 was produced by hydrogen burning in stars and not in the early stages of a big bang. In addition, we show that there are good arguments for believing that the other light isotopes, D, He-3, Li-6, Li-7, Be-9, B-10, and B-11, were also synthesized in processes involving stars. By combining these results with the earlier, much more detailed work of Burbidge et al. and of Cameron, we can finally conclude that all of the chemical elements were synthesized from hydrogen in stars over a time of about 10(11) yr.
引用
收藏
页码:L1 / L3
页数:3
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