Modules for Experiments in Stellar Astrophysics
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Updated
Jun 5, 2024 - Fortran
Astrophysics is the scientific discipline that deals with the physics of objects, phenomena, and processes in outer space, including (but not limited to) stars, galaxies, compact objects, and the formation of the Universe.
Modules for Experiments in Stellar Astrophysics
MCFOST radiative transfer code
The Galacticus galaxy formation model
Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
SPLASH is an interactive visualisation and plotting tool using kernel interpolation, mainly used for Smoothed Particle Hydrodynamics simulations
Simulation of metal diffusion in the ICM for the Perseus Cluster The aim of the project is to show the possible parameters for efficient metal distribution under reasonable diffusion timescales to reproduce observed abundance profile.
A 1-D version of the ZEUS 2D CODE which solves hydrodynamic equations is applied to a SuperNova Remnant(SNR). The system is evolved for a time t =5x10^5 yrs and results are discussed below.
The Arbitrary Linear Plasma Solver
Solving particle transport equations using stochastic method
dynamics, age and metallicity indicators tracing evolution
This is Nbody6++GPU, an N-body star cluster simulation code, maintained by Rainer Spurzem and team.
UCLCHEM - A gas-grain chemical code for Astrochemistry.
Compute spectral energy distributions of radiatively inefficient accretion flows (RIAFs) around black holes
An advanced N-body model for interacting multiple stellar/asteroidal systems (ξ Tauri, (216))
A CPU/GPU Accelerated Multi-dimensional Magnetohydrodynamics Code
Python bindings to CALC11
A modified version of NBODY6 which uses the P3T algorithm.
Legolas: a modern tool for MHD spectroscopy