1. INAF-Astrophysical Observatory Turin, Strada Osservatorio 20, 10025 Pino Torinese, Italy; 2. Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37830, USA; 3. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA
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.
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