Abstract
We report nucleosynthetic results for both 44Ti and nickel isotopes for 18 three-dimensional (3D) core-collapse supernova (CCSN) simulations extended to ∼20 s after bounce. We find that many of our long-term models are able to achieve 44Ti/56Ni ratios similar to that observed in Cassiopeia A, and modern supernova models can synthesize up to 2 × 10−4 M ⊙ of 44Ti. Neutrino-driven winds and the fact that there can be simultaneous accretion and explosion in 3D models of CCSNe play central roles in its production. We conclude that the 44Ti underproduction problem in previous CCSN models is no longer an issue. In addition, we discuss the production of both 57Ni and stable nickel/iron ratios and compare our results to observations of SN 1987A and the Crab.
Published Version
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