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

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)