WARNING: This code is no longer developed/maintained!
Main code written for my Master's thesis
Martin J. Steil, Structure of slowly rotating magnetized neutron stars in a perturbative approach,
Master's thesis, Technische Universität Darmstadt, 2017,
mjsteil.github.io/files/MJSteil_MSc_Thesis_2017.pdf
for various numerical computations regarding isolated neutron stars as perturbations to the Tolman-Oppenheimer-Volkoff (TOV) solution.
Includes a Mathematica implementation in I-love-Qrot.nb for the computation of I-love-Q relations (see, e.g. arxiv.org/abs/1303.1528 for details).
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gsl_wrapper– Used for interpolation and numerical (ODE) integration -
matplotlib-cpp– Used for plotting (only necessary if one wants to plot them usingmatplotlib_cpp -
eos– Used for the equation of state -
units.hpp– Used for physical units -
LiSK– Lightweight C++ library for the numerical evaluation of classical polylogarithms Li(n,x)
Martin Jakob Steil, 2017