Cosmological deuterium production in non-standard scenarios

被引:8
作者
Jedamzik, K
机构
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
[2] Univ Montpellier 2, Lab Phys Math & Theor, CNRS, UMR5825, F-34095 Montpellier 5, France
关键词
Big Bang nucleosynthesis; light elements; early Universe;
D O I
10.1016/S0032-0633(02)00089-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is widely believed that the cosmic baryon density may be obtained by inferring deuterium abundances in low-metallicity quasar absorption line systems. The implicit assumptions which enter this argument are critically assessed. In particular, the production of deuterium in non-standard Big Bang nucleosynthesis scenarios, the putative production-of deuterium in astrophysical environments, and the possible destruction of deuterium via non-standard chemical evolution are discussed. (C) 2002 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:1239 / 1244
页数:6
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