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Signatures of $^{56}$Ni Mixing and Neutron-rich Ejecta in Supernovae
Supernova lightcurves are often interpreted with one-zone radioactive-decay models that ignore a key variable that can affect interpretation and inferred parameters: the distribution of radioactive material. Using a multi-shell model, we explore the impact of $^{56}$Ni mixing in supernovae and r-pro
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