High Resolution Shock Capturing Scheme for Non-Relativistic Hydrodynamics - Lecture 2

Delve into the second lecture on High Resolution Shock Capturing Scheme for Non Relativistic Hydrodynamics, presented by Kenta Kiuchi from the Albert Einstein Institute. Part of the Summer School on Gravitational-Wave Astronomy organized by the International Centre for Theoretical Sciences, this 1 hour 36 minute session explores advanced numerical techniques crucial for modeling complex astrophysical phenomena. Learn about the mathematical foundations and computational methods used in simulating non-relativistic fluid dynamics, with a focus on accurately capturing shock waves and discontinuities. Gain insights into the application of these techniques in studying various high-energy astrophysical events, such as stellar collapses, supernovae, and accretion processes around compact objects. Enhance your understanding of numerical relativity and its role in interpreting gravitational wave signals and multi-messenger observations from cosmic events.

High Resolution Shock Capturing Scheme for Non Relativistic Hydrodynamics Lecture 2 by Kenta Kiuchi