Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae

Details Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae

2003-04-10

arxiv.org/abs/astro-ph/0304185v1

Astrophys.J. 592 (2003) 404-433

Astronomy and Astrophysics

Astrophysics

20 pages, 10 figures, 12 tables. Accepted for publication on ApJ

Scientific paper

10.1086/375703

We present a new set of presupernova evolutions and explosive yields of massive stars of initial solar composition (Y=0.285, Z=0.02) in the mass range 13-35 Msun. All the models have been computed with the latest version (4.97) of the FRANEC code that now includes a nuclear network extending from neutrons to Mo98. The explosive nucleosynthesis has been computed twice: a first one with an hydro code and a second one following the simpler radiation dominated shock approximation (RDA).

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