Neutron-induced nucleosynthesis
| Autor: | Thomas Rauscher, H. Oberhummer, H. Herndl, H. Beer |
|---|---|
| Rok vydání: | 1996 |
| Předmět: |
Physics
Thermonuclear fusion Nuclear Theory Astrophysics::High Energy Astrophysical Phenomena media_common.quotation_subject Astrophysics (astro-ph) Theoretical models FOS: Physical sciences Astrophysics Universe Nuclear Theory (nucl-th) Neutron capture Supernova Geophysics Big Bang nucleosynthesis Geochemistry and Petrology Nucleosynthesis Astrophysics::Solar and Stellar Astrophysics Neutron Nuclear Experiment (nucl-ex) Nuclear Experiment Astrophysics::Galaxy Astrophysics media_common |
| Zdroj: | Scopus-Elsevier ResearcherID |
| ISSN: | 1573-0956 0169-3298 |
| DOI: | 10.1007/bf01931785 |
| Popis: | Neutron--induced nucleosynthesis plays an important role in astrophysical scenarios like in primordial nucleosynthesis in the early universe, in the s--process occurring in Red Giants, and in the $\alpha$--rich freeze--out and r--process taking place in supernovae of type II. A review of the three important aspects of neutron--induced nucleosynthesis is given: astrophysical background, experimental methods and theoretical models for determining reaction cross sections and reaction rates at thermonuclear energies. Three specific examples of neutron capture at thermal and thermonuclear energies are discussed in some detail. Comment: 40 pages (uses kluwer.sty), 2 postscript figures (uses psfig), accepted for publication in Surveys in Geophysics, uuencoded tex-files and postscript-files available at ftp://is1.kph.tuwien.ac.at/pub/ohu/Geo.uu |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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