Powerful Explosions from the Collapse of Rotating Supermassive Stars

Powerful Explosions from the Collapse of Rotating Supermassive Stars

We perform new general relativistic hydrodynamics simulations for collapses of rotating supermassive star cores with an approximate nuclear burning up to carbon and a detailed equation of state. For all the models we investigate, the energy generation by nuclear burning plays only a minor role, lead...

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Bibliographic Details
Main Authors: Sho Fujibayashi, Cédric Jockel, Kyohei Kawaguchi, Yuichiro Sekiguchi, Masaru Shibata
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Supermassive black holes
Massive stars
Gravitational collapse
Online Access:https://doi.org/10.3847/1538-4357/adb0b8
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