Multi-dimensional nucleosynthesis calculations of Type II SNe

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dc.creatorTravaglio, C.
dc.creatorKifonidis, K.
dc.creatorMueller, E.
dc.date2003-05-22
dc.date.accessioned2026-07-07T02:08:34Z
dc.date.available2026-07-07T02:08:34Z
dc.descriptionWe investigate explosive nuclear burning in core collapse supernovae by coupling a tracer particle method to one and two-dimensional Eulerian hydrodynamic calculations. Adopting the most recent experimental and theoretical nuclear data, we compute the nucleosynthetic yields for 15 Msun stars with solar metallicity, by post-processing the temperature and density history of advected tracer particles. We compare our results to 1D calculations published in the literature.
dc.description10 pages, to appear in Carnegie Observatories Astrophysics Series, Vol. 4: Origin and Evolution of the Elements, ed. A. McWilliam and M. Rauch (Pasadena: Carnegie Observatories)
dc.identifierhttps://arxiv.org/abs/astro-ph/0305440
dc.identifierhttp://arxiv.org/abs/astro-ph/0305440
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6101
dc.subjectAstrophysics
dc.titleMulti-dimensional nucleosynthesis calculations of Type II SNe
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