Dec 11 – 15, 2023
Tsung-Dao Lee Institute
Asia/Shanghai timezone

Bridging the Outflow from the Black Hole Scale to its Long-term Electromagnetic Observables: A Study using a Moving-Mesh General Relativistic Hydrodynamics Code with HLLC Riemann Solver

Not scheduled
20m
Tsung-Dao Lee Institute

Tsung-Dao Lee Institute

Contributed talk in mini symposium

Speaker

Xiaoyi Xie (Max Planck Institute for Gravitational Physics)

Description

We present the general relativistic framework that underpins a moving-mesh relativistic hydrodynamic code. To enhance the performance of this framework, we have developed a specialized tetrad formulation that optimizes the use of the HLLC Riemann solver in a moving mesh. Our research examines the ejecta that emerge from compact object mergers or collapses. By incorporating this new framework, we can trace the radial movement of the ejecta starting from the point where strong gravity is present. Our findings demonstrate that the code can evolve the ejecta structure from the central black hole scale with a primary mass of M to distances of one hundred thousand M and beyond. Additionally, we provide the analysis of investigating the microphysics of ejecta outflow from compact object simulations, along with its long-term electromagnetic observations.

Primary author

Xiaoyi Xie (Max Planck Institute for Gravitational Physics)

Presentation materials

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