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Topic
Simulation of the s-process under AGB conditions in a nuclear reaction network
Members
Julia Bliss - Analysis
Jianping Lai - Parameters
Kevin Siegl - Code
Initial Goals:
Determine theoretical astrophysical conditions for AGB stars during the s-process.
Create reaction network for both <sup>56<sub>Fe and solar abundance seeds.
Create toolkit to read binary file into format appropriate for abundance graphing.
Modify xnet code to allow the definition of a time-dependent neutron flux.
References