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This course aims to teach learners how to utilize numerical relativity as a tool for studying the early universe. The learning outcomes include understanding the framework of numerical relativity, conducting detailed investigations into cosmological models, and developing large-scale simulations of dynamical processes in the early universe. The course covers skills such as utilizing GRMHD codes, differentiating methods, simulating gravitational wave theory, setting initial conditions, and analyzing results. The teaching method involves a presentation by an expert in the field, covering topics such as the early universe, gravitational waves, simulations, and cosmological tests. The intended audience for this course includes students, researchers, and professionals interested in astrophysics, cosmology, and numerical simulations.
