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Supplementary Material for my Master's Thesis:

"Effects of strongly quantizing magnetic field on outer crust of cold non-accreting neutron stars"

Overview

This repository contains additional resources, data and code related to the research presented in the thesis.

Contents

  • Master's thesis, file: MSc_thesis_Mavroudis.pdf

  • The folder thesis_code contains:

  1. the main code (outer_crust.py)

Requirements

To run this code, you’ll need the following Python3 libraries installed:

numpy

pandas

scipy

matplotlib.pyplot

fortranformat

time

  1. and the auxiliary code (plots_all_models_together.py)

Requirements

To run this code, you’ll need the following Python3 libraries installed:

numpy

matplotlib.pyplot

os

  • The folders SEMF, FRDM2012, WS4RBF, BSKG3, HFB31, DDMED, DDPC1, SVMIN and UNEDF0 correspond to the respective used nuclear model. They contain:

  1. the main code (outer_crust.py)

  2. the file AME2020_table.dat, which contains the atomic mass excesses from AME2020

  3. the file <MODEL>_table.dat (apart from the folder SEMF), which contains the theoretically predicted atomic mass excesses or nuclear binding energies

  4. the generated - saved pictures (.png files) from the execution of the main code (outer_crust.py)

  5. the saved arrays (.npy files) from the execution of the main code (outer_crust.py)

  6. and the generated - saved tabular data (.dat files) from the execution of the main code (outer_crust.py)

  • The folder ALL_PLOTS contains:

  1. the auxiliary code (plots_all_models_together.py)

  2. the saved arrays (.npy files) from the folders SEMF, FRDM2012, WS4RBF, BSKG3, HFB31, DDMED, DDPC1, SVMIN and UNEDF0

  3. and the generated - saved pictures (.png files) from the execution of the auxiliary code (plots_all_models_together.py)

  • The folder tabulated generated data contains the generated - saved tabular data from the folders SEMF, FRDM2012, WS4RBF, BSKG3, HFB31, DDMED, DDPC1, SVMIN and UNEDF0, more organized as .ods files

If you have any questions or need further clarification, don't hesitate to reach out.

Citation

If you find this supplementary material useful for your research, please consider citing the master's thesis:

Ioannis Mavroudis (2024). Effects of strongly quantizing magnetic field on outer crust of cold non-accreting neutron stars. Aristotle University of Thessaloniki.

License

This work © 2024 by Ioannis Mavroudis is licensed under CC BY-NC-SA 4.0 (https://creativecommons.org/licenses/by-nc-sa/4.0/); code under GNU GPLv3 License (https://www.gnu.org/licenses/gpl-3.0.html).

© 2024 Ioannis Mavroudis