Journal ArticleDOI
R-process nucleosynthesis from an inner explosion of a low mass iron core
TLDR
In this article, the r-process that occurs due to the explosion from an inner region of the Fe-core was investigated, and it was shown that the solar R-process abundances are rather well reproduced for a model of 13 M ⊙.About:
This article is published in Nuclear Physics.The article was published on 2005-07-25. It has received 2 citations till now. The article focuses on the topics: Nuclear reaction & Nucleosynthesis.read more
Citations
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s-process nucleosynthesis-nuclear physics and the classical model
F. Käppeler,H. Beer,K. Wisshak +2 more
TL;DR: In this article, the status of this classical approach is reviewed with emphasis on the implications for various stellar models of the s-process and in the light of results obtained by stellar spectroscopy.
Journal ArticleDOI
r-Process in Prompt Supernova Explosions Revisited
Kohsuke Sumiyoshi,M. Terasawa,Grant J. Mathews,Toshitaka Kajino,Toshitaka Kajino,Shoichi Yamada,Hideyuki Suzuki +6 more
TL;DR: In this article, a relativistic hydrodynamic simulation of adiabatic collapse and bounce was performed to evaluate the products of the $r$-process nucleosynthesis in the supernova ejecta.
References
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Journal ArticleDOI
Astrophysical reaction rates from statistical model calculations
TL;DR: Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) or T(k) less less than/or equal to 10.0 x 10 (9) are calculated in the statistical model (Hauser-Feshbach formalism) as discussed by the authors.
Journal ArticleDOI
r-Process in Neutron Star Mergers
TL;DR: Sufficient material is ejected to explain the amount of r-process nuclei in the Galaxy by decompression of neutron star material, and the calculated abundances fit the observed solar r-pattern excellently for nuclei that include and are heavier than the A approximately 130 peak.
Journal ArticleDOI
s-process nucleosynthesis-nuclear physics and the classical model
F. Käppeler,H. Beer,K. Wisshak +2 more
TL;DR: In this paper, the status of this classical approach is reviewed with emphasis on the implications for various stellar models of the s-process and in the light of results obtained by stellar spectroscopy.
Journal ArticleDOI
Stellar weak interaction rates for intermediate mass nuclei. III. Rate tables for the free nucleons and nuclei with A = 21 TO A = 60
TL;DR: In this paper, the stellar electron and positron emission rates and neutrino energy loss rates for free nucleons and 226 nuclei with masses between A = 21 and 60 were calculated in tabular form on an abbreviated temperature and density grid.
s-process nucleosynthesis-nuclear physics and the classical model
F. Käppeler,H. Beer,K. Wisshak +2 more
TL;DR: In this article, the status of this classical approach is reviewed with emphasis on the implications for various stellar models of the s-process and in the light of results obtained by stellar spectroscopy.