Introduction to Numerical Relativistic Hydrodynamics - Lecture 4

Delve into the fourth lecture of a comprehensive series on Numerical Relativistic Hydrodynamics, presented by Kenta Kiuchi from the Albert Einstein Institute. Explore advanced concepts in this graduate-level course, part of the Summer School on Gravitational-Wave Astronomy organized by the International Centre for Theoretical Sciences. Gain insights into the mathematical formulation and numerical methods used to solve complex equations in General Relativity and magnetohydrodynamics. Discover how these techniques are applied to model high-energy astrophysical phenomena such as black hole and neutron star mergers, stellar collapse, and accreting black holes. Learn about the crucial role of Numerical Relativity in interpreting gravitational-wave signals and multi-messenger observations. Enhance your understanding of the intersection between theoretical physics, computational methods, and observational astrophysics in this intensive 1 hour and 29 minute lecture.

Introduction to Numerical Relativistic Hydrodynamics (Lecture 4) by Kenta Kiuchi