3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors
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DOI: 10.1093/mnras/staf1860
Abstract: Core-collapse supernovae (CCSNe) are among the most energetic and complex astrophysical phenomena, requiring three-dimensional (3D) simulations to capture their intricate explosion mechanisms. One of the key ingredients for such simulations is the 3D pre-collapse structure,… read more here.
Keywords: synthetic velocity; core collapse; velocity fields; initial conditions ... See more keywords