There are 4 repositories under astrophysical-simulation topic.
A framework for hydrodynamics explorations and prototyping
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
Astronomical simulator of solar system and local stars
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
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.
Physical vector and particle types for Julia
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.
A simple N-Body simulator, able to support a galactic environnement (under the form of a gravitational field).
A fast astrophysical N-body simulator, written in Python and Cython.
A CPU/GPU Accelerated Multi-dimensional Magnetohydrodynamics Code
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
Solve many-body problem via numerical minimization of orbits action
A modified version of NBODY6 which uses the P3T algorithm.
LEAPS 2017 Project repo: Simulating the formation of the Oort Cloud
Python code used to create spectral lines and tomograms (2D velocity distributions) from gas particle velocity data.
Analysis tools for the Galacticus galaxy formation model written in Python
University of Nottingham 3rd Year Astrophysics Project - Searching for Galaxy Clusters in the Dark Energy Survey
Simulates the flaring activity of a single magnetar using the Monte Carlo technique.
Impact of different temperature profiles and disc-to-star mass ratios on the disk's surface density profile when it reaches equilibrium
A python library for analyzing Phantom SPH data using Sarracen.
Scalar field large-scale structure formation
Analyse the orbital evolution of Extreme Mass Ratio Inspirals, according to Einstein's general theory of relativity.
Code to analyse data outputs from zoom galaxy cluster simulations investigating the effect of different mass and spatial resolutions.
Code used to analyse FLAMINGO data to investigate splashback radius of galaxy clusters in gas and observable profiles
Computational Astrophysics AST245: N-Body simulation and other exercises
Pulsar 3D simulation for Masters in Physics for the University of Brasília (UnB)
Exo3D is a JavaScript extension for exosystem web displaying, aiming to be included in The Extrasolar Planets Encyclopaedia (http://exoplanet.eu/). I was the main contributor of that project for a 6-month internship in the Observatoire of Paris, and worked with my internship tutor, Pierre-Yves Martin. Currently in pause for an undetermined time.