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Main Authors: Mizuno, Yosuke, Rezzolla, Luciano
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2404.13824
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author Mizuno, Yosuke
Rezzolla, Luciano
author_facet Mizuno, Yosuke
Rezzolla, Luciano
contents Recent years have seen a significant progress in the development of general relativistic codes for the numerical solution of the equations of magnetohydrodynamics in spacetimes with high and dynamical curvature. These codes are valuable tools to explore the large-scale plasma dynamics such as that takes place when two neutron stars collide or when matter accretes onto a supermassive black hole. This chapter is meant to provide a very brief but complete overview of the set of equations that are normally solved in modern numerical codes after they are cast into a conservative formulation within a 3+1 split of spacetime.
format Preprint
id arxiv_https___arxiv_org_abs_2404_13824
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle General-Relativistic Magnetohydrodynamic Equations: the bare essential
Mizuno, Yosuke
Rezzolla, Luciano
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Recent years have seen a significant progress in the development of general relativistic codes for the numerical solution of the equations of magnetohydrodynamics in spacetimes with high and dynamical curvature. These codes are valuable tools to explore the large-scale plasma dynamics such as that takes place when two neutron stars collide or when matter accretes onto a supermassive black hole. This chapter is meant to provide a very brief but complete overview of the set of equations that are normally solved in modern numerical codes after they are cast into a conservative formulation within a 3+1 split of spacetime.
title General-Relativistic Magnetohydrodynamic Equations: the bare essential
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2404.13824