Chikako Ishizuka, Akira Ohnishi, Kousuke Sumiyoshi
Published 2002-01-11, updated 2002-01-14Version 2
We propose a new nucleosynthesis process in which various nuclei are formed through the liquid-gas phase transition of supernova matter as a preprocess of the standard r-process, and study its possibility of realization qualitatively. In the relativistic mean field and statistical model calculations, we find that this process may take place and help the later r-process to proceed.
Comments: 5 pages, 3 figures, proceedings of Yukawa International Seminar 2001 (YKIS01), Physics of Unstable Nuclei, November 5-10, 2001, Kyoto, Japan. (v2: minor package change to adapt ptptex style file.)
Journal: Prog.Theor.Phys.Suppl.146:373-377,2003
Liquid-Gas Phase Transition of Supernova Matter and Its Relation to Nucleosynthesis
Effects of isospin and momentum dependent interactions on liquid-gas phase transition in hot asymmetric nuclear matter
Effects of the liquid-gas phase transition and cluster formation on the symmetry energy
