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diffhydro: Inverse Multiphysics Modeling and Embedded Machine Learning in Astrophysical Flows

  • Authors: Benjamin Horowitz, Zarija Lukić, Kentaro Nagamine, Yuri Oku

Benjamin Horowitz et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 9.

Multigrid V-cycle solution of the Poisson equation for self-gravity in DIFFHYDRO. At the finest level ℓ = 1, the gravitational potential ϕh is computed by solving Ahxh = bh with residual rh = bh − Ahxh. The residual is restricted to successively coarser meshes (ℓ = 2, 3), where the error equations A2he2h = r2h and A4he4h = r4h are solved, using a direct solver on the coarsest grid. The coarse-grid error is then interpolated/prolongated back to finer levels and used to update the solution, xh ← xh + eh, iterating until convergence. The bottom panels illustrate the density field represented on each level, highlighting how coarse grids capture long-wavelength contributions efficiently and accelerate convergence of the self-gravity force used in the hydrodynamic evolution.

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