Numerical Relativity: Mathematical Formulation - Lecture 3

Delve into the third lecture of the Numerical Relativity series, focusing on the mathematical formulation presented by Thomas Baumgarte from Bowdoin College. Explore advanced concepts in solving Einstein's field equations numerically, essential for modeling high-energy astrophysical phenomena like black hole mergers, neutron star collisions, and gravitational wave events. Gain insights into the mathematical framework underpinning numerical simulations crucial for gravitational-wave astronomy and astrophysics. Enhance your understanding of the complex interplay between general relativity, computational methods, and cutting-edge observations 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 3) by Thomas Baumgarte