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This 19 isotope reaction network has the same alpha-chain, (a,p)(p,g) reactions, and heavy-ion reactions as the 13 isotope network, but it includes additional isotopes to accommodate some types of hydrogen burning (PP chains and steady-state CNO cycles), along with some aspects of photodisintegration into 54Fe. This reaction network is described in Weaver,Zimmerman, & Woosley (ApJ 225, 1021, 1978) , and is still the workhorse network of the KEPLER stellar evolution code.
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Please cite the relevant references if you publish a piece of work that use these codes, pieces of these codes, or modified versions of them. If you're nice, offer co-authorship of the publication. At best, you'll love these programs so much that you'll send great wads of cash to me. |
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