Author/Authors :
Michael S. Smith، نويسنده , , Richard A. Meyer، نويسنده , , Daniel W. Bardayan، نويسنده , , Jeffery C. Blackmon، نويسنده , , Kyungyuk Chae، نويسنده , , Michael W. Guidry، نويسنده , , W. Raphael Hix، نويسنده , , R.L. Kozub، نويسنده , , Eric J. Lingerfelt، نويسنده , , Zhanwen Ma، نويسنده , , Jason P. Scott، نويسنده ,
Abstract :
Recent measurements with radioactive beams at ORNLʹs Holifield Radioactive Ion Beam Facility (HRIBF) have prompted the evaluation of a number of reactions involving unstable nuclei needed for stellar explosion studies. We discuss these evaluations, as well as the development of a new computational infrastructure to enable the rapid incorporation of the latest nuclear physics results in astrophysics models. This infrastructure includes programs that simplify the generation of reaction rates, manage rate databases, and visualize reaction rates, all hosted at a new website http://www.nucastrodata.org.
