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Lecture Notes in Computational Science and Engineering
Simulations of cosmic structure formation address multi-scale, multiphysics problems of vast proportions. These calculations are presently at the forefront of today's use of supercomputers, and are important scientific drivers for the future use of exaflop computing platforms. However, continued success in this field requires the development of new numerical methods that excel in accuracy, robustness, parallel scalability, and physical fidelity to the processes relevant in galaxy and stardoi:10.1007/978-3-030-47956-5_12 fatcat:nbv54h27a5a3ll62emrej6nmfq