作者: AM Lisewski , W Hillebrandt
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摘要: We present a model which shows the in uence of turbulence to a thermonuclear ame during a Type Ia Supernova (Type Ia SN). Based on a statistical description of turbulence, it provides a method for investigating the physics in the distributed burning regime. Possible consequences for a de agration to detonation transition (DDT) are discussed.