Abstract
Observations of supernovae and their remnants reveal highly aspherical distributions of the newly-formed elements that are the dying stars’ contributions to the interstellar medium. Modern simulations of the supernova’s neutrino-powered central engine reveal that these inhomogeneities originate in the first seconds of the explosions. Yet, much of our understanding of supernova nucleosynthesis is based on spherically symmetric models of the explosions. Recent simulations, combining high-fidelity treatments of the neutrino field that drives the explosion, the multidimensional fluid flow that taps this energy source, and the thermonuclear kinetics responsible for the composition of the ejecta, are revealing the limitations of our spherically symmetric understanding. Here, we highlight these recent results to presage the changes in our understanding of supernova nucleosynthesis that will result from a full appreciation of the multidimensional character of core-collapse supernovae.
