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

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dc.creatorHungerford, Aimee
dc.creatorFryer, Christopher L.
dc.creatorTimmes, Francis X.
dc.creatorYoung, Patrick
dc.creatorBennett, Michael
dc.creatorDiehl, Steven
dc.creatorHerwig, Falk
dc.creatorHirschi, Raphael
dc.creatorPignatari, Marco
dc.creatorMagkotsios, Georgios
dc.creatorRockefeller, Gabriel
dc.date2008-11-28
dc.date.accessioned2026-07-07T12:06:17Z
dc.date.available2026-07-07T12:06:17Z
dc.descriptionThe 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.
dc.descriptionTo appear in the Conference Proceedings for the "10th Symposium on Nuclei in the Cosmos (NIC X)", July 27 - August 1 2008, Mackinack Island, Michigan, USA
dc.identifierhttps://arxiv.org/abs/0811.4645
dc.identifierhttp://arxiv.org/abs/0811.4645
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/208610
dc.subjectAstrophysics
dc.titleDifficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni
dc.typetext

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