Emergent Nucleosynthesis from a 1.2 s Long Simulation of a Black Hole Accretion Disk

Emergent Nucleosynthesis from a 1.2 s Long Simulation of a Black Hole Accretion Disk

We simulate a black hole accretion disk system with full-transport general relativistic neutrino radiation magnetohydrodynamics for 1.2 s. This system is likely to form after the merger of two compact objects and is thought to be a robust site of r -process nucleosynthesis. We consider the case of a...

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Bibliographic Details
Main Authors: Trevor M. Sprouse, Kelsey A. Lund, Jonah M. Miller, Gail C. McLaughlin, Matthew R. Mumpower
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
R-process
Nucleosynthesis
Nuclear astrophysics
Nuclear physics
Magnetohydrodynamical simulations
Stellar accretion disks
Online Access:https://doi.org/10.3847/1538-4357/ad1819

Internet

https://doi.org/10.3847/1538-4357/ad1819

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