Ignition of Weak Interactions and r-process Outflows in Supercollapsar Accretion Disks

The collapse of rotating massive (∼10 M _⊙ ) stars resulting in hyperaccreting black holes (BHs; “collapsars”) is a leading model for the central engines of long-duration gamma-ray bursts (GRBs) and a promising source of rapid neutron-capture ( r -process) elements. R -process nucleosynthesis in dis...

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Detalles Bibliográficos

Principais autores:	Aman Agarwal, Daniel M. Siegel, Brian D. Metzger, Chris Nagele
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2026-01-01
Series:	The Astrophysical Journal
Assuntos:	R-process Stellar accretion disks Black holes Compact objects High energy astrophysics Massive stars
Acceso en liña:	https://doi.org/10.3847/1538-4357/ae2856
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