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This course focuses on the numerical analysis of binary neutron stars, a significant source of gravitational waves. The learning outcomes include understanding the dynamics of merging binary neutron stars, modeling their inspiral, merger, and post-merger phases, and obtaining accurate numerical solutions using hydrodynamics and MHD equations. The course teaches methods for fully nonlinear numerical modeling and reviews key results from available simulations. The teaching method involves lectures and discussions. This course is intended for individuals interested in gravitational wave astronomy, numerical analysis, and astrophysics.
