Modern Numerical Methods in Computational Relativity - Lecture 2
Offered By: International Centre for Theoretical Sciences via YouTube
Course Description
Overview
Delve into the second lecture of the Modern Numerical Methods in Computational Relativity series, delivered by Geoffrey Lovelace as part of the Summer School on Gravitational-Wave Astronomy. Explore advanced techniques and methodologies used in solving complex equations of General Relativity and magnetohydrodynamics through supercomputer simulations. Gain insights into the crucial role of Numerical Relativity in modeling high-energy astrophysical phenomena such as black hole mergers, neutron star collisions, and massive star collapses. Understand the significance of these simulations in interpreting gravitational-wave signals and multi-messenger observations. Benefit from this graduate-level course, designed for students and researchers in gravitational-wave astrophysics, offering a deep dive into the cutting-edge numerical methods shaping our understanding of the universe's most extreme events.
Syllabus
Modern Numerical Methods in Computational Relativity (Lecture 2) by Geoffrey Lovelace
Taught by
International Centre for Theoretical Sciences
Related Courses
Introduction to AstronomyDuke University via Coursera Confronting The Big Questions: Highlights of Modern Astronomy
University of Rochester via Coursera Analyzing the Universe
Rutgers University via Coursera Astronomy - State of the Art
University of Arizona via Udemy AstroTech: The Science and Technology behind Astronomical Discovery
University of Edinburgh via Coursera