Sensitivity of ${}^{44}$Ti and ${}^{56}$Ni production in CCSN shock-driven nucleosynthesis to reaction rates

Shiv K. Subedi, Zach Meisel, Grant Merz

Recent observational advances have enabled high resolution mapping of ${}^{44}$Ti in core-collapse supernova (CCSN) remnants. Comparisons between observations and models provide st…