Fragment Distribution in Coexistence Phase of Supernova Matter

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dc.creatorIshizuka, Chikako
dc.creatorOhnishi, Akira
dc.creatorSumiyoshi, Kousuke
dc.date2002-01-11
dc.date2002-01-14
dc.date.accessioned2026-07-07T11:10:52Z
dc.date.available2026-07-07T11:10:52Z
dc.descriptionWe 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.
dc.description5 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.)
dc.identifierhttps://arxiv.org/abs/nucl-th/0201026
dc.identifierhttp://arxiv.org/abs/nucl-th/0201026
dc.identifierProg.Theor.Phys.Suppl.146:373-377,2003
dc.identifierdoi:10.1143/PTPS.146.373
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190904
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleFragment Distribution in Coexistence Phase of Supernova Matter
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