Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
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Updated
Sep 15, 2024 - Fortran
Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
A framework for hydrodynamics explorations and prototyping
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.
MCFOST radiative transfer code
X-PSI: X-ray Pulse Simulation and Inference
A low Mach number stellar hydrodynamics code
The Galacticus galaxy formation model
C++17 N-body Barnes-Hut on heterogeneous hardware architectures
Astronomical simulator of solar system and local stars
Datasets for the Galacticus galaxy formation model
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.
Computational Astrophysics AST245: N-Body simulation and other exercises
A CPU/GPU Accelerated Multi-dimensional Magnetohydrodynamics Code
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
Physical vector and particle types for Julia
MSP: two-body orbital model written in Python
Pulsar 3D simulation for Physics Teaching Master's Program (MNPEF) at the University of Brasilia (UnB). Created by Lucas Ferreira (UnB/IF/MNPEF) and Vanessa Andrade (UnB/IF/MNPEF).
Module for the CRPropa code to calculate the effect of plasma instabilities on the development of electromagnetic cascades
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