Explosion dynamics of parametrized spherically symmetric core-collapse supernova simulations

We analyze the explosion properties and dynamics of spherically symmetric, parametrized core-collapse supernovae derived with the new PUSH method. To this end, we explore the progenitor mass range between 18 and 21 M-circle dot. We find that it is possible to suggest a distinction between low and high compactness progenitors. We discuss the differences on the example of two reference runs.