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Search results for c plus plus astrophysics

26 search results found

Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.

C++ library for ODE integration via Taylor's method and LLVM

Swiftaa ⭐ 145

The most comprehensive collection of accurate astronomical algorithms in (C++, Objective-C and) Swift.

C++ SPH/N-body library and standalone GUI application, mainly designed for astrophysical simulations

Heyoka.py ⭐ 57

Python library for ODE integration via Taylor's method and LLVM

Ramsesgpu ⭐ 50

Astrophysics MHD simulation code optimized for large cluster of GPU

Octotiger ⭐ 42

Astrophysics program simulating the evolution of star systems based on the fast multipole method on adaptive Octrees

Athenapk ⭐ 35

AthenaPK: a performance portable version of Athena++ built on Parthenon and Kokkos

Modern C++/python CPU/GPU plasma toolbox

Two-moment AMR radiation hydrodynamics (with self-gravity, particles, and chemistry) on CPUs/GPUs for astrophysics

Imfit: an open-source astronomical image-fitting program.

Python wrapper for Imfit (https://github.com/perwin/imfit)

3D Monte Carlo radiative transfer code

New generation astrophysical plasma simulation code with CPU/GPU portability

Astrodynamics ⭐ 16

Astrodynamics framework

🌎 SGP4 orbit propagation library for modern C++11

Shenanigans ⭐ 13

Semi-random funky stuff, mainly for my PhD experiments and articles. Contains calculations and algorithm implementations for various applied mathematics and astrophysics articles I worked on.

Easy, robust, and fast numerics in C++.

X-ray Astrophysics local model for Relativistic Reflection

Cadishi: CAlculation of DIStance HIstograms

Tool to generate fake galaxy catalogs with realistic positions, morphologies and fluxes from the far-ultraviolet to the far-infrared.

Tool that let you calculate star azimuth & altitude, in any given time and any given position

Compute FRED light curves of LMXBs outbursts

The fastest gravitational (quasar) microlensing code on the planet. A parallel Barnes-Hut tree code optimized for GPUs, written in OpenCL

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.

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.

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