Introduction to Numerical Relativistic Hydrodynamics - Lecture 2

Delve into the second lecture of a comprehensive series on Numerical Relativistic Hydrodynamics, presented by Kenta Kiuchi from the Albert Einstein Institute. Explore advanced concepts in this critical field that combines General Relativity with magnetohydrodynamics to simulate high-energy astrophysical phenomena. Gain insights into the mathematical and computational techniques used to model mergers of black holes and neutron stars, stellar collapses, and accreting black holes. Understand the crucial role of these simulations in interpreting gravitational-wave signals and multi-messenger observations. Learn how this cutting-edge research contributes to our understanding of extreme cosmic events and supports observations from current and future gravitational-wave, electromagnetic, and neutrino observatories.

Introduction to Numerical Relativistic Hydrodynamics (Lecture 2) by Kenta Kiuchi