Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae

Preprint

10 April 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0304185

Abstract

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).

Keywords

MODELS HAVE BEEN COMPUTED
EXPLOSIVE NUCLEOSYNTHESIS
PRESUPERNOVA EVOLUTIONS
COLLAPSE SUPERNOVAE
NUCLEOSYNTHESIS
CORE COLLAPSE
SUPERNOVAE
NEUTRONS

All Related Versions

Version 1, 2003-04-10, ArXiv
Published version: The Astrophysical Journal, 592 (1), 404.

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