PRODUCTION OF BE-9 AND HEAVY-ELEMENTS IN THE INHOMOGENEOUS UNIVERSE

被引:49
作者
TERASAWA, N [1 ]
SATO, K [1 ]
机构
[1] UNIV TOKYO,FAC SCI,DEPT PHYS,BUNKYO KU,TOKYO 113,JAPAN
关键词
Cosmology; Diffusion; Nucleosynthesis; Stars : Be; Stars: abundances; Stars: Population II;
D O I
10.1086/185844
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
While 9Be is expected to provide a test of inhomogeneous models of primordial nucleosynthesis, we show that the previous estimate by the simplified two-zone model of neutron diffusion overestimated the 9Be abundance at least two orders of magnitude in plausible parameter space. The abundances of CNO elements expected to be the seeds of the cosmic r-process are very small in the proper range of baryon/photon ratio consistent with the abundances of light elements.
引用
收藏
页码:L47 / L49
页数:3
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