Basis Function Expansion C++ library and Python package for running N-body galactic simulations and dynamical discovery
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Updated
Aug 16, 2026 - C++
Basis Function Expansion C++ library and Python package for running N-body galactic simulations and dynamical discovery
A Python package for performing self-consistent population synthesis and galactic dynamics simulations
Tools for analysis of N-body models with Basis Function Expansions and perturbation theory themes.
Stellar system linear response theory in Julia
SteParKin code determine Galactic-space velocity components (U, V, W), evaluate their membership to young kinematic moving groups and associations and assign their stellar populations.
Python module to compute and interactively visualize Poincaré sections
HuBBLE is a Galactic Dynamics Simulation project made in C++
Interoperability Between Galactic Dynamics Libraries
Gala Studio Is An Interactive visualization Lab for the Gala dynamics Library with Nobel-Tier Features
N-body python package designed for galactic dynamics.
Deterministic reproducibility capsule for GIFT Paper 1. Reproduces the deep-regime scaling and normalization of the RAR and BTFR from the SPARC dataset using fixed-slope ODR fits. Code, derived data, and verification figures included. Archived snapshot: Zenodo DOI 10.5281/zenodo.18513729.
Code and data for analyzing action coherence in a galactic simulation, as part of the paper of 'Evolution of action-space coherence in a MIlky Way-like simulation' by Arunima et al
Repository for hosting MHD codes for Galatic Dynamo simulations.
The ACM Trunk: a rigid holographic framework for galactic dynamics. This repository provides the core analytical engine for predicting galaxy rotation behavior from baryonic distributions via linear holographic screening. Tagline No galaxy-by-galaxy fits. No hidden knobs. Just the physics of the background floor.
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Planet 9 disproved by Galactic Dominance Beyond Solar Gravitational Boundary
All 8 Virgo galaxies show DECLINING rotation curves. All 10 field galaxies show FLAT rotation curves. This is exactly what MOND/Entropic Gravity predicts.
Wide binary stars at large separations show 27.7% higher orbital velocities than Newtonian prediction — exactly as MOND predicts.
Covariance-aware BIC sensitivity implementation stopped when the frozen diagonal galaxy fit failed deterministic reproduction.
Burkert-backbone + BIC-selected Gaussian shells fit to 102 SPARC rotation curves (T=2–9). Companion code and data for Bibb (2026).
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