Reaction rates and nuclear properties relevant for nucleosynthesis in massive stars and far from stability

T. Rauscher, Carla Froehlich, K. H. Guber

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Explosive nuclear burning in astrophysical environments produces unstable nuclei which again can be targets for subsequent reactions. In addition, it involves a large number of stable nuclides which are not fully explored by experiments, yet. Thus, it is necessary to be able to predict reaction cross sections and thermonuclear rates with the aid of theoretical models. Such predictions are also of interest for investigations at radioactive ion beam facilities. An extended library of theoretical cross sections and reaction rates is presented. The problem of alpha+nucleus potentials is addressed and new parametrizations presented. The problem of properly predicting cross sections at low level densities is illustrated by the Ni-62(n,gamma) reaction.

Original languageEnglish
Title of host publicationCapture Gamma-Ray Spectroscopy and Related Topics
EditorsJ. Kvasil, P. Cejnar, M. Krticka
Place of PublicationSingapore
PublisherWorld Scientific Publishing
Pages336-342
Number of pages7
ISBN (Electronic)978-981-4485-83-8
ISBN (Print)978-981-238-391-4
Publication statusPublished - 2003
Event11th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics - PRUHONICE, Czech Republic
Duration: 2 Sept 20026 Sept 2002

Conference

Conference11th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics
Country/TerritoryCzech Republic
CityPRUHONICE
Period2/09/026/09/02

Keywords

  • STATISTICAL-MODEL CALCULATIONS
  • SCATTERING
  • CROSS-SECTIONS
  • ASTROPHYSICAL REACTION-RATES

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