Toward General Relativistic Magnetohydrodynamics Simulations in Stationary Nonvacuum Spacetimes

Toward General Relativistic Magnetohydrodynamics Simulations in Stationary Nonvacuum Spacetimes

Accretion of magnetized gas on compact astrophysical objects such as black holes (BHs) has been successfully modeled using general relativistic magnetohydrodynamic (GRMHD) simulations. These simulations have largely been performed in the Kerr metric, which describes the spacetime of a vacuum and sta...

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Bibliographic Details
Main Authors: Prashant Kocherlakota, Ramesh Narayan, Koushik Chatterjee, Alejandro Cruz-Osorio, Yosuke Mizuno
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Astrophysical black holes
Supermassive black holes
Accretion
Relativistic jets
Non-standard theories of gravity
Gravastars
Online Access:https://doi.org/10.3847/2041-8213/acfd1f

Internet

https://doi.org/10.3847/2041-8213/acfd1f

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