Numerical relativistic hydrodynamics in curved spacetime

量子物理学・ナノサイエンス第109回特別セミナー

概要

Numerical simulations of relativistic hydrodynamics and magnetohydrodynamics have become indispensable tools in studying high-energy astrophysical phenomena, including accretion flows around black holes and the dynamics of neutron stars. In strongly curved spacetimes, the equations governing fluid motion generally lack analytic solutions, the numerical simulation is the only way to achieve meaningful insight. In this presentation, I will provide an overview of the finite volume method for solving the equations of relativistic hydrodynamics in curved spacetime. I will also discuss recent applications of this approach.

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• 量子物理学・ナノサイエンス第109回特別セミナー

• 東京科学大学理学院・物理学系 ナノサイエンスを拓く量子物理学拠点 共催