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What Does the Fuel Layer Look Like Right Before the Flash?
A major part of the challenge in doing these simulations is knowing how to initialize the grid.
- What sort of temperature perturbation (size, shape, duration) is required to get the event underway?
Evolution right up to the point of ignition by a multi-d code is currently not available.
- Good initial conditions, right before the runaway are hard to get.
Most models suppose that the ignition begins at a single point, and propagates across the star.