The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project – Status and Prospects

Journal Article · Sun Jun 15 00:00:00 EDT 2014 · Nuclear Data Sheets

DOI:https://doi.org/10.1016/J.NDS.2014.07.038· OSTI ID:22436715

für Schwerionenforschung Darmstadt, GSI Helmholtzzentrum ^[1]; Szücs, T. ^[2]; Plag, R. ^[3]; für Schwerionenforschung Darmstadt, GSI Helmholtzzentrum ^[1]; Fülöp, Z. ^[2]; Käppeler, F. ^[4]; Mengoni, A. ^[5]; Rauscher, T. ^[6]

---

1. Germany
2. Institute for Nuclear Research (MTA Atomki), Debrecen (Hungary)
3. Institut für Angewandte Physik, Goethe-Universität Frankfurt (Germany)
4. Karlsruhe Institute of Technology (KIT), Institut für Kernphysik, Campus Nord, Karlsruhe (Germany)
5. Agenzia Nazionale per le Nuove Tecnologie, l'Energia e lo Sviluppo Economico Sostenibile (ENEA), Bologna (Italy)
6. Centre for Astrophysics Research, School of Physics, Astronomy and Mathematics, University of Hertfordshire (United Kingdom)

The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) project is an astrophysical online database for cross sections relevant for nucleosynthesis in the s process and the γ process. The s-process database ( (http://www.kadonis.org)) was started in 2005 and is presently facing its 4th update (KADoNiS v1.0). The γ-process database (KADoNiS-p, (http://www.kadonis.org/pprocess)) was recently revised and re-launched in March 2013. Both databases are compilations for experimental cross sections with relevance to heavy ion nucleosynthesis. For the s process recommended Maxwellian averaged cross sections for kT=5−100 keV are given for more than 360 isotopes between {sup 1}H and {sup 210}Bi. For the γ-process database all available experimental data from (p,γ),(p,n),(p,α),(α,γ),(α,n), and (α,p) reactions between {sup 70}Ge and {sup 209}Bi in or close to the respective Gamow window were collected and can be compared to theoretical predictions. The aim of both databases is a quick and user-friendly access to the available data in the astrophysically relevant energy regions.

• OSTI ID: 22436715
• Journal Information: Nuclear Data Sheets, Vol. 120; Other Information: Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA); ISSN 0090-3752
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ASTROPHYSICS
BISMUTH 209
BISMUTH 210
CROSS SECTIONS
GERMANIUM 70
HEAVY IONS
HYDROGEN 1
NUCLEAR REACTIONS
NUCLEOSYNTHESIS
S PROCESS
STARS