Introduction to Numerical Relativistic Hydrodynamics - Lecture 3

Delve into the third 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 model high-energy astrophysical phenomena. Gain insights into the mathematical and computational techniques used to simulate mergers of black holes and neutron stars, stellar collapses, and accreting black holes. Learn how these simulations contribute to our understanding of gravitational waves and multi-messenger astronomy. Discover the importance of Numerical Relativity in interpreting observational data from gravitational-wave, electromagnetic, and neutrino observatories. Enhance your knowledge of this cutting-edge area of astrophysics, essential for graduate students and researchers in gravitational-wave astronomy and related fields.

Introduction to Numerical Relativistic Hydrodynamics (Lecture 3) by Kenta Kiuchi