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.
Newtonian and relativistic asteroseismology code for simple models of stars.
Semi-analytic Solvers for Two-component Rotating 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.
Kinematical studies of white dwarfs populations
Bachelor in Science major project on astrophysics: analysis of properties of dust structure around WD
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.
Finite temperature FMT EoS + TOV solver for single and multiple component white dwarfs
Semi-analytic Solvers for Two-component General-relativistic Spherically Symmetric Stars
Equation of States (EOS) Table Generator for White Dwarfs
Some examples and notes on GWFish from LGWA Workshop
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