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Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

X-PSI: X-ray Pulse Simulation and Inference

A low Mach number stellar hydrodynamics code

Galacticus ⭐ 22

The Galacticus galaxy formation model

MCFOST radiative transfer code

PION (PhotoIonization of Nebulae) is a C++ computational fluid-dynamics package for astrophysics, including MHD, radiative transfer, chemical kinetics and postprocessing routines. It is used mainly for modelling nebulae around massive stars.

A framework designed to simulate the signals produced by the secondary particles emerging from the interaction of the flux of primary cosmic ray with the atmosphere. These signals are simulated for any particle detector located at any place (latitude, longitude and altitude), including the real-time atmospheric, geomagnetic and detector conditions.

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