Resources for Computational Astrophysics, Summer Project 2021, IIT Kanpur
SiMon -- Simulation Monitor
PLUTO: A Numerical Code for Computational Astrophysics
Research Project Under Prof. Gulab Chand Dewangan (Senior Professor, IUCAA, Pune) during Visiting Student @ IUCAA 2025
CompactStar is a modular C++ framework for modeling neutron stars, hybrid stars, and exotic compact objects. It includes GR stellar-structure solvers (TOV + Hartle), thermal–chemical–spin evolution, baryon-number–violating (BNV) microphysics, and a full EOS engine for dense matter.
Astrophysical Shockwave and Turbulence Research for Interstellar Applications
Developed for "Laboratory of Computational Physics Mod. A", this project employs graphical and machine learning tools to identify the features with the greatest impact on the fate of binary black holes in Nuclear Star Clusters (NSC), Globular Clusters (GC), and Young Star Clusters (YSC).
A computational science blogging site.
Personal project to find periodic orbits around 216-Kleopatra Asteroid. Based on Abad et al., 2024
Open-source repository for my astrophysics research/studies.
Smoothed Particle Hydrodynamics (SPH) simulations in 2D: custom developed SPH solver for modeling cloud-cloud collisions in astrophysical context.
Repository for the Computational Astrophysics course - 2023 - UniPD
"Computational Cost Optimization for Numerical Integration of the Smoluchovski Coagulation Equation via Stochastic Kernel Sampling" - M.Sc. thesis that I am currently writing at the Heidelberg Institute for Theoretical Astrophysics under the supervision of Prof. Dr. Cornelis Dullemond
"Computational Cost Optimization for Numerical Integration of the Smoluchovski Coagulation Equation via Stochastic Kernel Sampling" - M.Sc. thesis that I am currently writing at the Heidelberg Institute for Theoretical Astrophysics under the supervision of Prof. Dr. Cornelis Dullemond
Repository for ASP Undergraduate Thesis
Methods of Computational Astrophysics
Lightweight C/Python toolkit for astronomical N-body simulations. Reconciles SPARC rotation curves and JWST morphology via a 1.21e-10 m/s^2 threshold patch. 解決星系旋轉殘差、JWST 數據偏差及數值不穩定問題。
Tools to play with pre-supernova progenitor stars.
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