Particle-in-cell code for plasma simulation

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

MCFOST radiative transfer code

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.

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.

Physical vector and particle types for Julia

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

Solve many-body problem via numerical minimization of orbits action

Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS

Simulates the flaring activity of a single magnetar using the Monte Carlo technique.

University of Nottingham 3rd Year Astrophysics Project - Searching for Galaxy Clusters in the Dark Energy Survey