KADoNiS‐ The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars

By I. Dillmann, M. Heil, Franz Kappeler, R. Plag, T. Rauscher, Friedrich-Karl Thielemann. 2006

136 citations recorded by the source corpus.

The “Karlsruhe Astrophysical Database of Nucleosynthesis in Stars” (KADoNiS) project is an online database for experimental cross sections relevant to the s process and p process. It is available under http://nuclear‐astrophysics.fzk.de/kadonis and consists of two parts. Part 1 is an updated sequel to the previous Bao et al. compilations from 1987 and 2000 for (n,γ) cross sections relevant to the big bang and s‐process nucleosynthesis. The second part will be an experimental p‐process database, which is expected to be launched in winter 2005/06. The KADoNiS project started in April 2005, and a first partial update is online since August 2005. In this paper we present a short overview of the first update of the s‐process database, as well as an overview of the status of stellar (n,γ) cross sections of all 32 p isotopes.

Subfields: Instrumentation, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a7593f574139a75f673b9a6cf5d8b25a24b717dc

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In Instrumentation

1. Aaron Dotter
2. U. Frischknecht
3. Alexander Heger
4. Falk Herwig
5. M. Pignatari
6. Chris L. Fryer
7. P. Young
8. S. Diehl

In Nuclear and High Energy Physics

1. Alexander Heger
2. C. Travaglio
3. Chris L. Fryer
4. U. Frischknecht
5. Francis Timmes
6. A. Hungerford
7. R. Hirschi
8. Aaron Dotter

Citations in the corpus

• CONVECTIVE–REACTIVE PROTON–12C COMBUSTION IN SAKURAI'S OBJECT (V4334 SAGITTARII) AND IMPLICATIONS FOR THE EVOLUTION AND YIELDS FROM THE FIRST GENERATIONS OF STARS (2010, methodology): “For neutron capture reactions of stable isotopes we refer to Dillmann et al. (2006) (KADoNIS compilation).”
• NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z = 0.02 and Z = 0.01 (2013, methodology): “Experimental neutron capture reaction rates are taken, when available, from the KADoNIS compilation (Dillmann et al. 2006).”
• ENDF/B-VII.1 Nuclear Data for Science and Technology: Cross Sections, Covariances, Fission Product Yields and Decay Data (2011, methodology): “The idea is to compare integral cross sections between major evaluated nuclear data libraries, including data from the Atlas of Neutron Resonances [35] and the Karlsruhe astrophysics database KADoNiS [36].”