Particle-in-cell code for plasma simulation
Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.
C++17 N-body Barnes-Hut on heterogeneous hardware architectures
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.
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.
Module for the CRPropa code to calculate the effect of plasma instabilities on the development of electromagnetic cascades
Computational Astrophysics AST245: N-Body simulation and other exercises
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