Nuclear Data Activities for Astrophysics at Oak Ridge National Laboratory

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Scientific paper

Nuclear structure information on neutron and proton rich nuclei and the reactions involving these nuclei are vital in order to understand and simulate important astrophysical processes. The nuclear data evaluation program at ORNL is directed to selective nuclei and their properties that are synergistic with the current nuclear astrophysics research programs at ORNL's Holifield Radioactive Ion Beam Facility. ^14O(α ,p)^17F,^ 17F(p,γ )^18Ne, ^18F(p,γ )^19Ne, ^18F(p,α )^15O, and ^82Ge(n,γ )^83Ge reactions are among those being studied. A survey of evaluation results and plans for additional work will be presented. A new computational infrastructure with unique software tools hosted at www.nucastrodata.org has also been developed to enable the rapid incorporation of the latest nuclear data in astrophysics models. Features of the program suite, its utilization, and future development will be discussed.

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