Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae

We present the results of simulations of nucleosynthesis in a core-collapse supernova including the neutrino process. Using the Si layer of a 13 M _⊙ zero-metal progenitor as the initial composition, we calculate the nucleosynthesis by adopting the temperature, density, neutrino flux, and duration o...

Description complète

Détails bibliographiques

Auteurs principaux:	Ryota Hatami, Nozomu Tominaga, Takashi Yoshida, Hideyuki Umeda, Tomoya Takiwaki
Format:	Artigo
Langue:	Inglês
Publié:	IOP Publishing 2026-01-01
Collection:	The Astrophysical Journal
Sujets:	Nucleosynthesis Explosive nucleosynthesis Core-collapse supernovae Supernova dynamics Stellar abundances
Accès en ligne:	https://doi.org/10.3847/1538-4357/ae2fbc
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!