Description
Chair: J. deBoer
Mr
David Godos Valencia
(IF-UNAM, CEAFMC - Universidad de Huelva)
6/10/24, 4:00 PM
The $^{44}$Ti nucleosynthesis takes place in Core Collapse Supernova (CCSN) explosions, the final process suffered by stars with initial mass greater than 8 M$_\odot$. This, alongside its characteristic gamma decay chain, turns the isotope into a good gamma tracer of Supernovae events. Besides, the comparison between observations and models of the synthesized $^{44}$Ti in CCSN gives important...