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
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
The term project of the Computational Physics (PHYS514) course. -- Koc University
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
Some examples and notes on GWFish from LGWA Workshop
Equation of States (EOS) Table Generator for White Dwarfs
Semi-analytic Solvers for Two-component General-relativistic Spherically Symmetric Stars
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