Published July 1, 2008
| Version v1
Report
Thermonuclear Reaction Rate Libraries and Software Tools for Nuclear Astrophysics Research
Description
Thermonuclear reaction rates are a crucial input for simulating a wide variety of astrophysical environments. A new collaboration has been formed to ensure that astrophysical modelers have access to reaction rates based on the most recent experimental and theoretical nuclear physics information. To reach this goal, a new version of the REACLIB library has been created by the Joint Institute for Nuclear Astrophysics (JINA). A complementary effort is the development of software tools in the Computational Infrastructure for Nuclear Astrophysics, to streamline, manage, and access the workflow of the reaction evaluations from their initiation to peer review to incorporation into the library. Details of these new projects will be described
Availability note (English)
Available from Oak Ridge National Laboratory, Oak Ridge, TN (US)Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 3 p.
- Report number
- ORNL/PTS--9759
Conference
- Title
- 10. International Symposium on Origin of Matter and Evolution of Galaxies
- Dates
- 3-7 Dec 2007
- Place
- Sapporo (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 39116477
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- ASTROPHYSICS; GALAXIES; NUCLEAR PHYSICS; ORIGIN; REACTION KINETICS; THERMONUCLEAR REACTIONS
- Descriptors DEC
- KINETICS; NUCLEAR REACTIONS; NUCLEOSYNTHESIS; PHYSICS; SYNTHESIS
Optional Information
- Contract/Grant/Project number
- KB0301042; ERKBP07; AC05-00OR22725
- Notes
- pages 466-468; http://www.nscl.msu.edu/~nero/db; nucastrodata.org
- Funding organization
- SC USDOE - Office of Science (Seychelles) (US)