Data for "A post-Newtonian approach to neutron star oscillations"
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Data generated and analysed for the work "A post-Newtonian approach to neutron star oscillations" (arXiv:2504.06918), which the readers can compare with theirs. Results1-3 are the data for the background stellar configurations built with PW model, AGYM model and isotropic TOV model correspondingly. FIG.1 and FIG.3 can be plotted using these files. Results4-10 are the data generated from the post-Newtonian perturbation calculations for the background star built with PW model. FIG.2 can be plotted using these files.
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Zenodo创建时间:
2025-08-13



