Stronger convective overshooting widens the SNe Ia parameter space for massive white dwarfs, makes the predicted birth rate non-monotonic with a peak at δov=0.25, and raises the predicted SNe Ia-CSM fraction.
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Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
Stronger convective overshooting widens the SNe Ia parameter space for massive white dwarfs, makes the predicted birth rate non-monotonic with a peak at δov=0.25, and raises the predicted SNe Ia-CSM fraction.