Modeling the nucleosynthesis of massive stars

T. Rauscher

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Abstract

This overview discusses issues relevant to modeling nucleosynthesis in type II supernovae and implications of detailed studies of the ejecta. After a brief presentation of the most common approaches to stellar evolution and parameterized explosions, the relevance of a number of nuclei to obtain information on the evolution and explosion mechanisms is discussed. The paper is concluded by an outlook on multi-dimensional simulations. (C) 2003 Elsevier B.V. All rights reserved.

Original languageEnglish
Pages (from-to)3-6
Number of pages4
JournalNew Astronomy Reviews
Volume48
Issue number1-4
DOIs
Publication statusPublished - Feb 2004
EventInternational Workshop on Astronomy with Radioactivities IV and Filling and Sensitivity Gap in MeV Astronomy - Kloster Seeon, Germany
Duration: 26 May 200330 May 2003

Keywords

  • NUCLEAR
  • stars : late stages of evolution
  • supernovae
  • EXPLOSION
  • CORE-COLLAPSE SUPERNOVAE
  • nucleosynthesis
  • EVOLUTION
  • nuclear processes (astrophysics)

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