Using 62-meter-resolution AMR simulations, the authors find that buoyancy-driven compression of fuel near RT-unstable flame fronts shortens carbon ignition times by 2 to over 5 orders of magnitude, with stronger effects at higher density.
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Mesoscale Turbulence in Type Ia Supernova Deflagrations: Buoyancy-Driven Fuel Heating and Prospects for Delayed-Detonations
Using 62-meter-resolution AMR simulations, the authors find that buoyancy-driven compression of fuel near RT-unstable flame fronts shortens carbon ignition times by 2 to over 5 orders of magnitude, with stronger effects at higher density.