Nuclear cosmochronometer and universality in the r-process abundance distribution
暂无分享,去创建一个
[1] 本田 敏志. Spectroscopic studies of r-process elements in extremely metal-poor stars with SUBARU/high-dispersion-spectrograph and cosmochronometry , 2002 .
[2] T. Kajino,et al. New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light, Neutron-rich Nuclei , 2001, astro-ph/0107368.
[3] T. Beers,et al. Measurement of stellar age from uranium decay , 2001, Nature.
[4] H. Tagoshi,et al. General Relativistic Effects on Neutrino-driven Winds from Young, Hot Neutron Stars and r-Process Nucleosynthesis , 1999, astro-ph/9911164.
[5] S. Woosley,et al. Nucleosynthesis in Neutrino-Driven Winds. I. The Physical Conditions , 1996, astro-ph/9611094.
[6] T. Kajino,et al. Geometrical Effects of Baryon Density Inhomogeneities on Primordial Nucleosynthesis , 1996, astro-ph/9609130.
[7] W. M. Howard,et al. r-process nucleosynthesis in the high-entropy supernova bubble , 1992 .