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Nucleosynthesis in Supernovae and the Early Universe

 

作者: T. Kajino,   T. Sasaqui,   M. Orito,   K. Otsuki,   G. J. Mathews,   S. Honda,   W. Aoki,   S. Chiba,  

 

期刊: AIP Conference Proceedings  (AIP Available online 1904)
卷期: Volume 704, issue 1  

页码: 488-500

 

ISSN:0094-243X

 

年代: 1904

 

DOI:10.1063/1.1737145

 

出版商: AIP

 

数据来源: AIP

 

摘要:

Universal baryon‐density parameter &OHgr;Binferred from the Big‐Bang nucleosynthesis and cosmic microwave background fluctuations disagrees with each other at the 1&sgr; level. We propose new cosmological models for the Big‐Bang nucleosynthesis to try to recover the concordance of &OHgr;B. Nuclear processes in the Big‐Bang nucleosynthesis are similar to those in the r‐process nucleosynthesis in supernovae. Even in the nucleosynthesis of heavy elements, entropy and density in the neutrino‐driven winds of Type II supernovae are so high that nuclear statistical equilibrium favors production of abundant light nuclei. In such explosive circumstances many radioactive light‐to‐intermediate mass nuclei as well as heavy mass nuclei play the significant roles. © 2004 American Institute of Physics

 

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