This code calculate some of the macroscopic properties of the neutron star such as its mass, radius, compactness and central density.
Requirments python3, math, numpy, scipy, matplotllib
It is the slightly modified version of the TOV code written by Amotonenko (https://github.com/amotornenko)
To download
'git clone https://github.com/hcdas/TOVCode'
The eos_unified_IOPB.dat can be found from the following link https://github.com/hcdas/Unfied_pasta_eos
To use unified equation of states, please follow the link https://github.com/hcdas/Unfied_pasta_eos. Please cite the following articles, if you are using those EOSs
Crustal properties of the neutron star within an effective relativistic mean-field model Phys. Rev. D 105, 043017 (2022), https://journals.aps.org/prd/abstract/10.1103/PhysRevD.105.043017 and arXiv:2111.07278 (https://arxiv.org/abs/2111.07278),
Pasta properties of the neutron star within an effective relativistic mean-field model. arXiv:2203.16827 (https://arxiv.org/abs/2203.16827)