Computational methods for nucleosynthesis and nuclear energy generation

DOI10.1016/S0377-0427(99)00163-6zbMath1032.81500arXivastro-ph/9906478MaRDI QIDQ1807727

Friedrich-Karl Thielemann, W. Raphael Hix

Publication date: 23 November 1999

Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9906478

zbMATH Keywords

nuclear astrophysics

Mathematics Subject Classification ID

Nuclear physics (81V35) Computational methods for problems pertaining to quantum theory (81-08) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items (2)

Explicit integration with GPU acceleration for large kinetic networks ⋮ Algebraic stabilization of explicit numerical integration for extremely stiff reaction networks

Cites Work

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• Neutrino transport in core collapse supernovae
• How to preserve the mass fractions positivity when computing compressible multi-component flows
• The Highly Collapsed Configurations of a Stellar Mass. (Second Paper.)
• Electron Screening and Thermonuclear Reactions

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