Pulsar 3D simulation for Physics Teaching Master's Program (MNPEF) at the University of Brasilia (UnB). Created by Lucas Ferreira (UnB/IF/MNPEF) and Vanessa Andrade (UnB/IF/MNPEF).

LAPS (UCLA-Pseudo-Spectral) is a MPI-parallelized pseudo-spectral 3D Hall-MHD code written in Fortran.

Atmospheric escape from magma ocean exoplanets

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.

Library that calculates geodesics (orbits) using any metric compatible with General Relativity.

A real-time 3D solar system simulator featuring accurate orbital mechanics, dynamic gravity well visualization, and interactive controls. Built with performance optimizations for smooth rendering, customizable views, and educational insights into celestial dynamics.

Code and reports for computational astrophysics

This project utilizes NASA API data and Python scripting for UI in Blender in order to predict and view future solar eclipses through beautifully rendered simulations.

Comparative study of AGN host galaxies in SDSS DR7 and IllustrisTNG, focused on green valley demographics and sSFR offsets.

This repository contains simulations for accretion disks of black holes based on initial conditions. Numbers are added onto acc to stress the increasing complexity of the variables added into the functions that define an accreting black hole system.

Code and report for 3-body-problem

Data analisis of a synthetic dataset about hierarchical mergers of black holes.

Numerical simulation of an expanding universe based on the Friedmann-Lemaître model

A Jupyter Notebook for detecting stars in FITS images. Just add your FITS files to the fits folder and run the notebook to process and visualize the data.

Simulation of a system of bodies under the influence of gravity in Python

Repository for the Phase-Bifurcation Cosmogenesis model. Includes, academic paper, reproducible Δϕ simulations, numerical scripts, critical-mass analysis (mϕ,crit ≈ 1.965), and visualizations of a non-singular CPT-symmetric cosmic origin.

Example program for computing the DUSTYWAVE exact solution for linear waves in a dust-gas mixture, from Laibe & Price (2011)

Effective-field-theory embedding of a CPT-symmetric twin-universe cosmology tested against DESI DR2 data. This repository provides analysis scripts, figures, and results for the Siamese Universes V model — a holographic cosmological