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arXiv:astro-ph/0011206 (astro-ph)
[Submitted on 9 Nov 2000]

Title:Exploding and Non-exploding Stars: Coupling Nuclear Reaction Networks to Multidimensional Hydrodynamics

Authors:K. Kifonidis (1), T. Plewa (2 and 1), E. Mueller (1) ((1) MPA, Garching, Germany, (2) Copernicus Astronomical Center, Warsaw, Poland)
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Abstract: After decades of one-dimensional nucleosynthesis calculations, the growth of computational resources has meanwhile reached a level, which for the first time allows astrophysicists to consider performing routinely realistic multidimensional nucleosynthesis calculations in explosive and, to some extent, also in non-explosive environments. In the present contribution we attempt to give a short overview of the physical and numerical problems which are encountered in these simulations. In addition, we assess the accuracy that can be currently achieved in the computation of nucleosynthetic yields, using multidimensional simulations of core collapse supernovae as an example.
Comments: 12 pages, LaTeX, 6 postscript figures, uses this http URL, to appear in H. Utsunomiya, ed., Proceedings of the Tours Symposium on Nuclear Physics IV, held at Tours, France, Sept. 4th - 7th, 2000
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0011206
  (or arXiv:astro-ph/0011206v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0011206
Related DOI: https://doi.org/10.1063/1.1372778

Submission history

From: Konstantinos Kifonidis [view email]
[v1] Thu, 9 Nov 2000 18:36:18 UTC (229 KB)
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