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- W1995727689 abstract "We present our first nucleosynthesis results from a numerical simulation of the thermonuclear disruption of a static cold Chandrasekhar-mass 12C/16O white dwarf. The two-dimensional sim- ulation was performed with an adaptive-mesh Eulerian hydrodynamics code, flash, that uses as a flame capturing scheme the evolution of a passive scaler. To compute the isotopic yields and their velocity distribution, 10,000 massless tracer particles are embedded in the star. The particles are advected along streamlines and provide a Lagrangian description of the explosion. We briefly describe our verification tests and preliminary results from post-processing the particle trajectories in (ρ, T) with a modest (214 isotopes) reaction network." @default.
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- W1995727689 date "2005-07-01" @default.
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- W1995727689 title "Type Ia Supernovae: Simulations and Nucleosynthesis" @default.
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- W1995727689 doi "https://doi.org/10.1016/j.nuclphysa.2005.05.083" @default.
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