Difficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni

Details Difficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni Difficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni

2008-11-28

arxiv.org/abs/0811.4645v1

Astronomy and Astrophysics

Astrophysics

To appear in the Conference Proceedings for the "10th Symposium on Nuclei in the Cosmos (NIC X)", July 27 - August 1 2008, Mac

Scientific paper

The nucleosynthetic yield from a supernova explosion depends upon a variety of effects: progenitor evolution, explosion process, details of the nuclear network, and nuclear rates. Especially in studies of integrated stellar yields, simplifications reduce these uncertainties. But nature is much more complex, and to actually study nuclear rates, we will have to understand the full, complex set of processes involved in nucleosynthesis. Here we discuss a few of these complexities and detail how the NuGrid collaboration will address them.

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