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ASTROLABE: A 3D Particle-Level Surrogate for Cosmology Simulation with Physical Flow Matching
The microphysics of dark matter (DM) is imprinted on cosmological structure across an enormous dynamic range. Nonlinear cosmological observables are most reliably modeled with N-body and hydrodynamic simulations. However, systematic N-body scans over DM theory space are prohibitively expensive. Mach
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