Numerical Relativity: Mathematical Formulation - Lecture 5

Delve into the fifth lecture of the Numerical Relativity series, focusing on the mathematical formulation presented by Thomas Baumgarte. Explore advanced concepts in solving Einstein's field equations computationally, essential for modeling high-energy astrophysical phenomena such as black hole mergers, neutron star collisions, and stellar collapses. Gain insights into the mathematical framework underpinning numerical simulations crucial for gravitational wave astronomy and multi-messenger observations. Enhance your understanding of the complex interplay between general relativity and computational methods in this graduate-level presentation from the Summer School on Gravitational-Wave Astronomy at the International Centre for Theoretical Sciences.

Numerical Relativity: Mathematical Formulation (Lecture 5) by Thomas Baumgarte