Abstract
We review our understanding of the nucleosynthesis that occurs in thermonuclear supernovae and their contribution to Galactic Chemical evolution. We discuss the prospects to improve the modeling of the nucleosynthesis within simulations of these events.
Original language | English |
---|---|
Pages (from-to) | 199-216 |
Number of pages | 18 |
Journal | Frontiers of Physics |
Volume | 8 |
Issue number | 2 |
DOIs | |
State | Published - Apr 2013 |
Funding
Acknowledgements C. Travaglio thanks Regione Lombardia, CILEA Consortium through a LISA Initiative (Laboratory for Interdisciplinary Advanced Simulation) 2010 grant, and B2FH Association, for their support. C. Travaglio also thanks R. Gallino, W. Hillebrandt and F. Roepke for their fruitful collaboration. W. R. Hix acknowledges support from the Office of Nuclear Physics of the U.S. Department of Energy and the Nuclear Theory and Stellar Astrophysics programs of the U.S. National Science Foundation. W. R. Hix thanks E. Feger, M. W. Guidry, O. E. B. Messer, S. Parete-Koon and F.-K. Thielemann for invaluable discussions.
Keywords
- chemical evolution
- explosive nucleosynthesis
- hydrodynamics
- nuclear reactions
- stellar spectra
- supernovae