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Most massive stars end their lives with core collapse. However, it is notclear which explode as a Core-collapse Supernova (CCSN), leaving behind aneutron star and which collapse to black hole, aborting the explosion. One pathto predict explodability without expensive multi-dimensional simulations is todevelop analytic explosion conditions. These analytic explosion conditions alsoprovide a deeper understanding of the explosion mechanism and they provide someinsight as to why some simulations explode and some do not. The analytic forceexplosion condition (FEC) reproduces the explosion conditions of sphericallysymmetric CCSN simulations. In this followup manuscript, we include thedominant multi-dimensional effect that aids explosion, neutrino drivenconvection, into the FEC. This generalized critical condition (FEC+) issuitable for multi-dimensional simulations and has potential to accuratelypredict explosion conditions of two- and three-dimensional CCSN simulations. Weshow that adding neutrino-driven convection reduces the critical condition by$\sim 30\%$, which is consistent with previous multi-dimensional simulations.

Including Neutrino-driven Convection into the Force Explosion Condition to Predict Explodability of Multi-dimensional Core-collapse Supernovae (FEC+)