Hydrodynamics and Nucleosynthesis of Jet-driven Supernovae. I. Parameter Study of the Dependence on Jet Energetics

Rotating massive stars with initial progenitor masses M _prog ∼ 25–140 M _⊙ can leave rapidly rotating black holes to become collapsars. The black holes and the surrounding accretion disks may develop powerful jets by magnetohydrodynamics instabilities. The propagation of the jet in the stellar enve...

Ausführliche Beschreibung

Bibliografische Detailangaben

Hauptverfasser:	Shing-Chi Leung, Ken’ichi Nomoto, Tomoharu Suzuki
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2023-01-01
Schriftenreihe:	The Astrophysical Journal
Schlagworte:	Explosive nucleosynthesis Supernovae Hypernovae Hydrodynamical simulations Chemical abundances Relativistic jets
Online-Zugang:	https://doi.org/10.3847/1538-4357/acbdf5
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