Explosion and nucleosynthesis of low-redshift pair-instability supernovae
2014; EDP Sciences; Volume: 566; Linguagem: Inglês
10.1051/0004-6361/201423641
ISSN1432-0746
AutoresAlexandra Kozyreva, Sung-Chul Yoon, N. Langer,
Tópico(s)Nuclear physics research studies
ResumoContext. Both recent observations and stellar evolution models suggest that pair-instability supernovae (PISNe) could occur in the local Universe, at metallicities below ≲Z⊙/3. Previous PISN models were mostly produced at very low metallicities in the context of the early Universe.
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