The focus of the school will be the understanding and application of nuclear reaction networks to astrophysical models for systems such as novae, x-ray bursts (rp-process) and supernovae (r-process). The reaction network employed will be the public libnucnet code published by Prof. Bradley Meyer, of Clemson University and available for download on the web through http://www.webnucleo.org/.
Contact: network2@ph.tum.de
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