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S. J. Robbins (CWRU), B. S. Meyer, G. C. Jordan (Clemson University)
Detailed explorations of the science of nucleosynthesis and stellar evolution have long been largely the exclusive province of those with the time and computation resources to construct and compute nuclear reaction networks. We introduce a web site that allows any internet users to run the well-tested Clemson nuclear-reaction network code in a simple, straightforward manner. Users may enter their own network, nuclear properties, reaction-rate data, and thermodynamic trajectories for the matter being modeled in XML format or may use default values. Users run the calculations on the server professionally maintained by the College of Engineering and Science at Clemson University. They may plot the output using straightforward GUI interfaces or download the data directly to their own computers. This web site, located at\\ \\ http://www.ces.clemson.edu/physics/nucleo/pages/nuclear_nework/\\ \\ should be of particular use to nuclear physicists seeking to understand to effects of particular nuclear or reaction-rate data and to students wishing to study the details of nucleosynthesis.
If you would like more information about this abstract, please follow the link to http://www.ces.clemson.edu/physics/nucleo/srobbins/index.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: sjr16@cwru.edu
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.