@inproceedings{a12e508ded9744cc9c86f1ed86c6dc0d,
title = "Nucleosynthesis in Supernovae and the Early Universe",
abstract = "Universal baryon-density parameter ΩB inferred from the Big-Bang nucleosynthesis and cosmic microwave background fluctuations disagrees with each other at the 1σ level. We propose new cosmological models for the Big-Bang nucleosynthesis to try to recover the concordance of ΩB. 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.",
author = "T. Kajino and T. Sasaqui and M. Orito and K. Otsuki and Mathews, \{G. J.\} and S. Honda and W. Aoki and S. Chiba",
note = "Publisher Copyright: {\textcopyright} 2004 American Institute of Physics.; Tours Symposium on Nuclear Physics V; Tours 2003 ; Conference date: 26-08-2003 Through 29-08-2003",
year = "2004",
month = apr,
day = "12",
doi = "10.1063/1.1737145",
language = "英语",
isbn = "0735401772",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics Inc.",
pages = "488--497",
editor = "T. Wada and G. Munzenberg and M. Arnould and M. Ohta and T. Yamagata and M. Lewitowicz and H. Utsunomiya and H. Akimune",
booktitle = "Tours Symposium on Nuclear Physics V; Tours 2003",
}