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Sep 4, 2020 - Jupyter Notebook
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astrophysical-simulation
Here are 23 public repositories matching this topic...
A framework for hydrodynamics explorations and prototyping
python
simulation
solver
finite-volume
pde
hydrodynamics
multigrid
pyro
advection
finite-volume-methods
astrophysical-simulation
A low Mach number stellar hydrodynamics code
simulation
reactions
maestro
astrophysics
amr
cfd
pde
hydrodynamics
low-mach
astrophysical-simulation
adaptive-mesh-refinement
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Aug 21, 2019 - Fortran
Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
fortran
astronomy
particles
astrophysics
fluid-simulation-engine
fluid-solver
fluid-dynamics
gas-dynamics
hydrodynamic-modeling
magnetohydrodynamics
astrophysical-simulation
dust-gas
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Sep 29, 2020 - Fortran
X-PSI: X-ray Pulse Simulation and Inference
astronomy
modeling
astrophysics
sampling
parameter-estimation
astronomical-algorithms
likelihood-functions
statistics-modeling
x-ray-astronomy
astrophysical-simulation
posterior-sampling
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Sep 30, 2020 - Python
C++17 N-body Barnes-Hut on heterogeneous hardware architectures
astronomy
cuda
avx
simd
nbody
cpp17
avx2
vectorization
n-body-simulator
avx512
n-body
rocm
nbody-simulation
nbody-gravity-simulation
nbody-sim
astrophysical-simulation
nbody-problem
astrophyics
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May 22, 2020 - C++
A simple N-Body simulator, able to support a galactic environnement (under the form of a gravitational field).
c
astrophysics
nbody
galaxy
n-body-simulator
n-body
nbody-simulation
nbody-gravity-simulation
nbody-sim
rk4
astrophysical-simulation
globular-clusters
pece
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Sep 17, 2018 - Python
Solve many-body problem via numerical minimization of orbits action
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Mar 12, 2020 - Jupyter Notebook
abensonca
commented
Mar 9, 2020
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Variables should be "radiusDiskSatellite" not "satelliteDiskRadius". The first word should reflect what the quantity is, a radius, followed by descriptions of what this quantity relates to, in order of increasing degree of removal.
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Do not use "this" in variable names, such as "thisNode" - should be just "node".
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
astronomy
mpi
astrophysics
modelling
semi-numerical
reionization
astrophysical-simulation
galaxy-evolution
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Apr 27, 2020 - C
LEAPS 2017 Project repo: Simulating the formation of the Oort Cloud
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Jul 14, 2017 - Python
Python visualization for the PLUTO Code
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Sep 10, 2020 - Python
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Jul 26, 2018 - Python
University of Nottingham 3rd Year Astrophysics Project - Searching for Galaxy Clusters in the Dark Energy Survey
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Jun 28, 2020 - MATLAB
Analysis and modeling tools to simulate/measure spectral and kinematics properties of galaxy in slitless spectroscopy.
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Apr 13, 2020 - Jupyter Notebook
MSP: two-body orbital model written in Python
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Jun 14, 2020 - Python
Installation scripts for the Galacticus galaxy formation model
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Jul 22, 2020 - Shell
Tool to convert merger trees from Rockstar/ConsistentTrees to Galacticus format
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Jun 29, 2020 - C
Analysis tools for the Galacticus galaxy formation model written in Python
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Apr 27, 2020 - Python
Datasets for the Galacticus galaxy formation model
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Aug 10, 2020
Physical vector and particle types for Julia
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Sep 16, 2020 - Julia
Analysis tools for the Galacticus galaxy formation model written in Perl
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Apr 27, 2020 - Perl
Module for the CRPropa code to calculate the effect of plasma instabilities on the development of electromagnetic cascades
plasma
astrophysics
physics-simulation
gamma-ray-astronomy
astrophysical-simulation
gamma-gamma-interactions
crpropa
electromagnetic-cascades
plasma-instabilities
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Jan 9, 2020 - C++
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The Poisson solve absolute tolerance sets the accuracy of the Poisson solve. Given the value of abs_tol, the error level targeted in the Poisson solve is abs_tol * 4 * pi * G * rho_max, where rho_max is the maximum density on the domain. For Cartesian simulations the default value is 1.e-11, and for non-Cartesian the default value is 1.e-10.
At high resolution, and/or for complicated mass distr