Code to estimate the Gravitational Wave Background sourced by extragalactic coalescing White Dwarf binaries.
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Updated
Jun 24, 2025 - Jupyter Notebook
Code to estimate the Gravitational Wave Background sourced by extragalactic coalescing White Dwarf binaries.
This repository contains excerpts from the programs made during the FRI summer fellowship and fall research in the “White Dwarfs” stream. “Kick_survial_final” and “WD_mass_loss” are our respective final programs, while the rest are functions and separate code snapshots that I contributed to or created.
Newtonian and relativistic asteroseismology code for simple models of stars.
The term project of the Computational Physics (PHYS514) course. -- Koc University
A work on the Lane-Endem equation for stars applied to non-relativistic white dwarfs of polytropic index n=3/2.
Semi-analytic Solvers for Two-component Rotating Stars
Kinematical studies of white dwarfs populations
Bachelor in Science major project on astrophysics: analysis of properties of dust structure around WD
Finite temperature FMT EoS + TOV solver for single and multiple component white dwarfs
Data and analysis pipeline for Chickles et al. 2026, ApJ — eclipsing 8.56-min mass-transferring binary.
Some examples and notes on GWFish from LGWA Workshop
Semi-analytic Solvers for Two-component General-relativistic Spherically Symmetric Stars
Equation of States (EOS) Table Generator for White Dwarfs
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